├── Code_of_Conduct.md ├── LICENSE ├── README.md ├── Timeline.md ├── Web_Banner.gif ├── Week1_Unix_Git_Papers ├── .ipynb_checkpoints │ ├── Python Tutorial-checkpoint.ipynb │ ├── Python and Jupyter Intro-checkpoint.ipynb │ └── unix_git_slides-checkpoint.ipynb ├── PaperWritingGuide.pdf ├── Python and Jupyter Intro.ipynb ├── README.md ├── Unix_Git_Tutorial.ipynb ├── Unix_Git_Tutorial.slides.html ├── data │ ├── closest20kstars.csv │ └── pdi_pi_collapsed.fits ├── how_to_read_scientific_papers.md ├── images │ ├── git_diagram_1.png │ ├── git_xkcd.png │ └── screenshot_01.png └── notebook_names.txt ├── Week2_Python_Packages ├── .ipynb_checkpoints │ ├── Introduction to Numpy, Scipy and Astropy-checkpoint.ipynb │ ├── Problem_Set_on_Numpy_Scipy_Astropy-checkpoint.ipynb │ ├── Python Tutorial-checkpoint.ipynb │ └── pandas_tutorial-checkpoint.ipynb ├── Astropy- code_astro.pdf ├── Diurnal_arc.jpeg ├── Introduction to Numpy, Scipy and Astropy.ipynb ├── Problem_Set_on_Numpy_Scipy_Astropy.ipynb ├── Python Tutorial.ipynb ├── Python and Jupyter Intro.ipynb ├── README.md ├── astropy_upload.ipynb ├── baby-names.csv ├── cmb_data.txt ├── data │ ├── closest20kstars.csv │ └── pdi_pi_collapsed.fits ├── dataframe.txt ├── example_data.fits ├── franck_hertz.xlsx ├── pandas_tutorial.ipynb ├── plot.pdf ├── s0002.fits ├── save_the_pandas.csv └── temperatures_ghana.txt ├── Week3_Matplotlib_Exoplanets ├── .ipynb_checkpoints │ ├── Inroduction_to_Matplotlib-checkpoint.ipynb │ └── nasa_exoplanet_archive_tutorial-checkpoint.ipynb ├── Inroduction_to_Matplotlib.ipynb ├── Introduction_to_Matplotlib.ipynb ├── Introduction_to_matplotlib.pptx ├── README.md ├── data │ ├── closest_100.csv │ ├── confirmed_example.csv │ ├── confirmed_kepler_transiting.csv │ ├── confirmed_mydata.csv │ └── m45.csv ├── example_data.fits ├── franck_hertz.xlsx ├── nasa_exoplanet_archive_tutorial.ipynb ├── plot.pdf └── s0002.fits ├── Week4_TESS_Gaia ├── GaiaTutorialAssignment.ipynb ├── Introduction_to_TESS.ipynb ├── README.md └── data │ ├── closest_100.csv │ ├── confirmed_example.csv │ ├── confirmed_kepler_transiting.csv │ ├── confirmed_mydata.csv │ ├── m45.csv │ ├── m5.csv │ ├── m5_random_sorted.csv │ ├── m92.csv │ └── stars_100.csv ├── Week5_CV_Latex_Overleaf_website ├── CV_guidelines.md ├── LaTeX Tutorial │ ├── LaTeX_tutorial.aux │ ├── LaTeX_tutorial.bbl │ ├── LaTeX_tutorial.blg │ ├── LaTeX_tutorial.log │ ├── LaTeX_tutorial.nav │ ├── LaTeX_tutorial.out │ ├── LaTeX_tutorial.pdf │ ├── LaTeX_tutorial.snm │ ├── LaTeX_tutorial.synctex.gz │ ├── LaTeX_tutorial.tex │ ├── LaTeX_tutorial.toc │ ├── LaTeX_tutorial.vrb │ ├── _minted-LaTeX_tutorial │ │ ├── 08A2B04D709025F9E47DCD217156ACB0762556F0E7C29D55187A847219DF9D00.pygtex │ │ ├── 090F811B9D0829E71A68D1EBD9A0B84B762556F0E7C29D55187A847219DF9D00.pygtex │ │ ├── 0B900B9E10F36A0243E3C9B4201F23A9762556F0E7C29D55187A847219DF9D00.pygtex │ │ ├── 10AB49616DE5A2CDBD26C9C90440C8F6762556F0E7C29D55187A847219DF9D00.pygtex │ │ ├── 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DB37065C3E4DBC50004E1CA7A7A688EEC45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── DF9A8AEB9C2C28EACA448DB25C32EB223A849686415DCD100B110891C4714664.pygtex │ │ ├── E140DA65018884348D03B6AA65D8E722C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── E3473F67403A61C52A5FB3B1D178806FC45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── EA9A4B565BFB9D18AD438162DEF7E827C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── EBB459281CDC74D5C5BFAD4D42BBABB5C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── EBB638C8CB96C7C05313A4418FEBE037C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── EC9FF695186FE107DDA0BF696C08B1F6C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── F0ACE40C17BC9426E76A96F6EF456B2C71F9999B52087C299F834088D65652D5.pygtex │ │ ├── F923673E8AF42976116B63BC8D457216C45D995AE810B8705B9F959AF97E5C0D.pygtex │ │ ├── default-pyg-prefix.pygstyle │ │ └── default.pygstyle │ ├── figures │ │ ├── air_network.pdf │ │ ├── cat.png │ │ ├── file_extensions.png │ │ ├── latex-comic.jpeg │ │ ├── learnlatex.png │ │ ├── phy_bachelors_employment.png │ │ ├── programming-comic.jpg │ │ ├── sps-logo.jpg │ │ └── texstackexchange.png │ └── references.bib ├── README.md ├── Templates │ ├── Homework Assignment │ │ ├── RR_PHYXXX_HWX.pdf │ │ └── RR_PHYXXX_HWX.tex │ ├── Physics Lab Report │ │ ├── PhysicsLabTemplate.pdf │ │ └── PhysicsLabTemplate.tex │ └── Project Report │ │ ├── RR_PHYXXX_Project1.pdf │ │ ├── RR_PHYXXX_Project1.tex │ │ ├── RR_PHYXXX_Project2.pdf │ │ └── RR_PHYXXX_Project2.tex └── notsoshort.pdf ├── Week6_RV_Summer_Research ├── 51 Pegasi RVs.csv ├── Model Fitting Assignment -- Exploring WASP-12 b's Orbital Decay.ipynb ├── Model Fitting Assignment Key -- Exploring WASP-12 b's Orbital Decay.ipynb ├── Model Fitting Demo -- Finding Orbital Parameters of WASP-94 b.ipynb ├── README.md ├── Radial Velocities Assignment -- Finding the Orbital Parameters of ___.ipynb ├── Radial Velocities Demo -- Finding the Orbital Parameters of 51 Pegasi b.ipynb ├── Summer_research_opportunities.pptx ├── WASP-12_ETD_clean.txt └── WASP-94_data.csv ├── Week7_AO_JWST └── README.md └── Week8_Grad_school_ML ├── Categorical Classification.ipynb ├── Classification_Clustering.png ├── README.md ├── data ├── category_dataset.csv ├── extended_training.csv └── unseen_test.csv └── true_distrib.png /Code_of_Conduct.md: -------------------------------------------------------------------------------- 1 | While this is meant to be primarily an online tutorial, we find it important to remind people that we should always strive to work in and create a positive environment in which everyone is welcome. 2 | 3 | We are dedicated to providing a supportive environment for all people. We do not tolerate harassment or abuse by or toward anyone participating in this program at any level. Because we are a diverse community, we may have different ways of communicating and of understanding the intent behind actions. If you have concerns about someone's behavior, either a mentor or student in the course, please contact one of the leaders of the program. Most times the conflict can be resolved with a diaglogue between all parties. In extreme cases, drastic actions may need to be taken, but conflict resolution on the person to perioson level should be attempted first. 4 | 5 | * Intro 2 Astro interactions should be professional regardless of location: harassment is prohibited whether it occurs on or offline, and the same standards apply to both. 6 | 7 | This workshop stands behind the principle open inquiry, viewpoint diversity, and constructive disagreement in research and education. We model this principle on the Heterodox Academy. For more details, check out their website: https://heterodoxacademy.org/library/reclaiming-the-culture-of-higher-education-guide/. 8 | -------------------------------------------------------------------------------- /LICENSE: -------------------------------------------------------------------------------- 1 | MIT License 2 | 3 | Copyright (c) 2019 Howard Isaacson 4 | 5 | Permission is hereby granted, free of charge, to any person obtaining a copy 6 | of this software and associated documentation files (the "Software"), to deal 7 | in the Software without restriction, including without limitation the rights 8 | to use, copy, modify, merge, publish, distribute, sublicense, and/or sell 9 | copies of the Software, and to permit persons to whom the Software is 10 | furnished to do so, subject to the following conditions: 11 | 12 | The above copyright notice and this permission notice shall be included in all 13 | copies or substantial portions of the Software. 14 | 15 | THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR 16 | IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, 17 | FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE 18 | AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER 19 | LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM, 20 | OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE 21 | SOFTWARE. 22 | -------------------------------------------------------------------------------- /README.md: -------------------------------------------------------------------------------- 1 | # Intro-to-Astro-2024 2 | ### An introductory course to Astronomy Research for aspiring students/researchers/enthusiasts 3 | 4 | ![alt text](https://github.com/howardisaacson/Intro-to-Astro2024/blob/main/Web_Banner.gif) 5 | 6 | ## Course Website: [Link](https://sites.google.com/view/intro-2-astro) 7 | 8 | Registrations have been closed for 2024. 9 | 10 | Participants for the 2024 workshop - if you haven't received an email yet, please check your spam folder. If you still cannot find the required details, please reach out to the organizers 11 | 12 | Recordings for the course will be uploaded on YouTube: [2024 Playlist](https://www.youtube.com/playlist?list=PLCNcoalRndQy6Q4BNNaJEl_FU2PkYudn2) 13 | 14 | ## About the Course 15 | Intro2Astro is an introductory 8-week cost-free online course targeted at aspiring students, researchers, and enthusiasts to step foot in the world of astronomy research. This is the 7th year and iteration of the course dedicated to acquainting students, particularly those from communities with fewer astronomy resources, with the basic tools that astronomers need in their research, and the skills they need in order to gain entry into a more formal research project. With exposure and eventual mastering of the skills taught through the course, students will be better prepared to begin research projects either during the semester or over the summer. Combining coding skills with soft skills such as web development, scientific paper reading, and CV creation can give students an edge when applying for formal research internships. 16 | 17 | The workshop is led by [Fei Dai](https://people.ifa.hawaii.edu/faculty/bio/fei-dai/) (University of Hawaii), [Howard Isaacson](https://astro.berkeley.edu/people/howard-isaacson/) (University of California, Berkeley), and [Chetan Chawla](https://sites.google.com/view/chetanchawla). 18 | 19 | 20 | 21 | ## Dates and schedule 22 | ### Duration: 23 | Monday, July 1st, 2024 to Monday, August 19th, 2024 (8 weeks) 24 | 25 | ### Sessions: 26 | The live Instructor-led sessions on tools used in astronomy research will be conducted at 5pm Pacific Time on Mondays Virtually on Zoom. The sessions will be uploaded on YouTube later on for asynchronous reference. 27 | 28 | ### Time Commitment: 29 | Students are expected to commit 5-10 hours per week outside of the sessions to the tutorials, assignments, and readings. 30 | 31 | ### Mentor Chats and Q&A: 32 | Students can ask questions and chat with the mentors in Office hours on Discord. They can also interact with their fellow students on the same. 33 | 34 | 35 | ### Specific topics include, but are not limited to the following: 36 | - Introduction to programming (in Python) 37 | - Creating scatter plots of real astronomical data 38 | - Fitting transit light curves and modeling radial velocities for exoplanets. 39 | - Querying online data archives (Gaia, MAST, Exoplanet Archive) 40 | - Planetary Geology 41 | - Machine Learning in Astronomy 42 | - Studying Galaxies 43 | - Creating professionally oriented research websites and CVs 44 | - Writing a research proposal on the topic of their choice 45 | 46 | 47 | 48 | 49 | 50 | ## Target Audience 51 | ### Students: 52 | First and second-year undergraduate students, and advanced high school students who are interested in gaining experience in astronomy research but have no previous research experience. There are no prerequisites in terms of content or programming. Although the course is targeted at the above-mentioned group, students from a non-traditional path and those without any affiliation can also apply. No students will be turned away for lack of experience or affiliation, i.e., anyone can sign up to be a part. Please sign up here [Registration Form](https://docs.google.com/forms/d/1dKbhgDU1bAWWnbv4XveYk4fIKCawatLnW8mg1yLli58/edit?usp=drive_web). 53 | 54 | 55 | ### Mentors: 56 | Graduate-level students and advanced undergraduates working on astronomy research who are interested in mentoring undergraduate students, developing open-source educational tutorials, and sharing their astronomy inspiration. Please fill out the Mentor [Interest Form](https://docs.google.com/forms/d/e/1FAIpQLScluDhVd9MGcx2OUu73DXewXJ36aCy_GYFKeESku2nVH5MYDg/viewform?usp=pp_url) 57 | 58 | 59 | ## Our Goals 60 | After the completion of these tutorials, students will have the skills needed to quickly ramp up on new astronomy research projects, without the need to brush up on basic skills. The astronomy skills will be focused on, but not limited to exoplanet topics. Students are encouraged to use these skills to explore other realms of Astronomy. Once you have completed all of the tutorials, you will be well-qualified for a paid internship in astronomy research. Many of these opportunities fall under the title: Research Experience for Undergraduates and serve as an excellent way to become qualified for graduate studies in astronomy. 61 | 62 | ## The Future of the Project: 63 | We hope this project becomes self-sustaining in such a way that others can contribute and add value to the current set of research skills presented here. If you have questions, comments, or ideas, please feel free to contact us through the issue tracker on this repo. If you work in another field such as biology, chemistry, another specialty within astronomy, and are interested in replicating this project for your specific field, please email me directly. 64 | 65 | ## Code of Conduct 66 | We strive to maintain a welcoming and supportive community for everyone regardless of race, religion, background or identity. For more details, see our [Code of Conduct page](https://sites.google.com/view/intro-2-astro/code-of-conduct). 67 | -------------------------------------------------------------------------------- /Timeline.md: -------------------------------------------------------------------------------- 1 | # Timeline for Summer 2023. June 12th - August 4th 2 | 3 | ## Week 1. Group Leaders: Chetan, Maria, Priya 4 | * GitHub: Version Control, git-clone vs downloading repositories. 5 | * Unix primer: (cd, ls, ssh, emacs) (Google cloud instance) 6 | * Coding programs: Textwrangler, PyCharm, Atom, or Sublime Text. 7 | 8 | ### Accounts needed: 9 | * Github.com 10 | * Google Drive (general gmail account) 11 | * DropBox.com 12 | * Overleaf.com 13 | * Kaggle.com 14 | * Papers and/or ADS experience (Building a library of papers) 15 | * Piazza.com ( Course Q&A website) 16 | ### Other topics: 17 | * How to write a professional email. 18 | * Make sure everyone has python installed. 19 | * Effective Paper Reading 20 | 21 | ### Part II of Week 1. 22 | * Python 23 | * Ipython 24 | * Jupyter 25 | * [Jupyter labs](https://github.com/jupyterlab/jupyterlab) 26 | 27 | ### Part III of Week 1. 28 | How to read a research paper. 29 | 30 | ### Paper of the week: 31 | Exoplanets Review by Lee (2018). Available here: https://arxiv.org/abs/1804.08907 32 | -------------------------------------------------------------------------------- /Web_Banner.gif: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Web_Banner.gif -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/PaperWritingGuide.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week1_Unix_Git_Papers/PaperWritingGuide.pdf -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/README.md: -------------------------------------------------------------------------------- 1 | ## First Meeting: July 1st, 2024: 5:00pm Pacific Daylight Time (UT-7). 2 | 3 | 4 | ## Agenda: 5 | * Introductions 6 | * Motivation 7 | * Overview of the course (discuss Github, Discord) 8 | * Tutorial on Unix 9 | * Tutorial on Git/GitHub 10 | * An introduction to Python and Jupyter notebooks 11 | * How to read scientific papers (ADS, Mendeley, arXiv) 12 | 13 | 14 | ## Assignments for Week 1 15 | 16 | ### If you have not already: 17 | * Ensure that you have a working version of Python installed on your computer. 18 | * [This link](https://carpentries.github.io/workshop-template/#python) has a section for downloading the Anaconda version of Python for Mac, Linux, or Windows 19 | * Finish writing your goals for this program if you did not finish during the session. 20 | 21 | ### Assignment 1) Go through the slides for Unix and complete the 2 assignments written there 22 | 1. Perform a set of commands mentioned in the slides 23 | 2. Complete the Data Carpentry workshop on the Unix command shell 24 | The Unix shell is the basis for scientific computing. By mastering shell commands, you will save 25 | yourself hours in the future. What seems like a small investment will pay dividends again and again. 26 | 27 | **Link to slides for Unix**: [Slides](https://unix-git-tutorial.netlify.app/) 28 | 29 | **Deliverable:** 30 | On Discord, you can send a file having list of all of the Unix commands that you learned, with a brief description of each. 31 | 32 | ### Assignment 2) Complete the Git tutorial: 33 | 34 | Git is a powerful and ubiquitous versioning tool for software development, 35 | though all of the vocabulary and mechanics can take some getting used to. Work through this Git tutorial to 36 | reinforce some of the features we discussed this week and learn about concepts we didn't have a chance to cover. 37 | 38 | **Link to slides for Unix**: [Slides](https://unix-git-tutorial.netlify.app/) 39 | 40 | **Deliverable**: 41 | * Go through the commands and do the assignment for Git by following the commands as mentioned on the slides. 42 | * Create a GitHub account if you don't already have one! You can sign up at https://github.com. 43 | 44 | 45 | *Bonus: If you want to learn it in more depth, you can also go through this short [Software Carpentry Workshop](https://swcarpentry.github.io/git-novice/)* 46 | 47 | 48 | 49 | ### Paper of the week: Assignment 3) Read this exoplanet review paper: 50 | 51 | * Exoplanets Review by Lee (2018). (https://arxiv.org/abs/1804.08907) 52 | * Read the paper, and save a list of questions you may have. 53 | * Read the paper again a few days later, and revisit your list of questions 54 | * Post at least one question on Discord, and respond to at least one of your classmates' questions. 55 | * Link for [How to read scientific papers](https://github.com/howardisaacson/Intro-to-Astro2024/blob/main/Week1_Unix_Git_Papers/how_to_read_scientific_papers.md) 56 | * In case the Figure on Page 6 does not render properly on your machine, you can refer to this [link](https://github.com/user-attachments/files/16120759/Lee-2018-Exoplanets-Fig1.pdf) 57 | 58 | 59 | 60 | ### Bonus Round (Intended for everyone. See how far you can get) 61 | Command line Ninjas begin their training with the simplest commands they use every day and eventually obtain 62 | more and more skills. Follow the link below and see how far you get in the command-line challenge. Be sure to 63 | keep track of your progress so that you can report back. 64 | 65 | https://cmdchallenge.com 66 | 67 | ## Writing Prompt (5-7 mins): 68 | * What are your goals for this course? 69 | * What topics in astronomy interest you? e.g. astrobiology, exoplanets, dark energy, black holes, space launches, mars exploration, the rings of Saturn, Earth-like planets, etc. 70 | -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/data/pdi_pi_collapsed.fits: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week1_Unix_Git_Papers/data/pdi_pi_collapsed.fits -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/how_to_read_scientific_papers.md: -------------------------------------------------------------------------------- 1 | # How to Read Scientific Papers 2 | 3 | by Isabel Angelo, Sarah Blunt & Tim Holt (2018, updated 2022) 4 | 5 | In this introduction, we suggest some techniques for effectively reading a scientific paper. We also provide resources that are commonly used in astronomy to make finding, reading, and storing papers much easier. 6 | 7 | ## Finding Scientific Papers: 8 | Use the Astrophysics Data System or ADS: 9 | 10 | https://ui.adsabs.harvard.edu 11 | 12 | ADS is a database where journal articles in astrophysics are stored. You can query the database by typing in the author, title, or other relevant information about a paper. The search engine will return a list of matches to your search, from which you can find the paper you are looking for. 13 | 14 | Use the ADS to find the discovery paper for your favorite exoplanet system using the ADS, write a brief description of the article in your own words. You should also copy the LaTax citation or store the article in the citation manager of your choice. 15 | 16 | ## Downloading and Storing Papers: 17 | Mendeley is a great application to track the many scientific papers that you will use throughout your careers. 18 | 19 | https://www.mendeley.com 20 | 21 | Mendeley allows you to download papers and keep them stored in a single, organized library on your own computer. You can also sort papers into cetegories and annotate them (similar to google docs) so you can have notes, definitions, etc. on-hand. 22 | 23 | ## Closely Reading Science Papers: 24 | 25 | For your assignment this week, please read the paper of the week thoroughly (Lee, 2018 https://arxiv.org/abs/1804.08907). Try to observe the following note-taking strategy (or use something similar that works for you!): 26 | 27 | - Highlight words you don't know in one color. Look up their definitions and write them down as in-text notes as you read. 28 | - Highlight key ideas in another color. 29 | - Keep a general note with summaries of each paragraph 30 | - Keep a general note with summaries of each section 31 | - Keep a note with 10-word or less summaries of each figure 32 | - Keep a note with overall questions you have about the paper. Some of these you may resolve as you read-- once you've finished reading the paper, revisit this note and see how many of your own questions you can answer! 33 | 34 | For more on how to effectively read a science paper, see the advice on astrobites, an website of astronomy- and academia-related articles run by astronomers and students: 35 | 36 | https://astrobites.org/2011/04/19/journal-articles-in-astronomy/ 37 | https://www.science.org/content/article/how-seriously-read-scientific-paper 38 | -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/images/git_diagram_1.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week1_Unix_Git_Papers/images/git_diagram_1.png -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/images/git_xkcd.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week1_Unix_Git_Papers/images/git_xkcd.png -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/images/screenshot_01.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week1_Unix_Git_Papers/images/screenshot_01.png -------------------------------------------------------------------------------- /Week1_Unix_Git_Papers/notebook_names.txt: -------------------------------------------------------------------------------- 1 | 2 | Python Tutorial.ipynb 3 | Python and Jupyter Intro.ipynb 4 | Unix_Git_Tutorial.ipynb 5 | -------------------------------------------------------------------------------- /Week2_Python_Packages/Astropy- code_astro.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/Astropy- code_astro.pdf -------------------------------------------------------------------------------- /Week2_Python_Packages/Diurnal_arc.jpeg: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/Diurnal_arc.jpeg -------------------------------------------------------------------------------- /Week2_Python_Packages/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT, Monday July 8th 2024. 2 | Zoom channel see Discord or google group 3 | 4 | 5 | #### Agenda: 6 | 7 | 1) Review/Checkin from last week: 8 | - How did the tutorials go? 9 | - What should the instructors do differently this week? 10 | 11 | 2) Short Tutorial on pandas (python data spreadsheets). Instructor screenshares, and: 12 | - Use git to download this repository (git folder). 13 | - Open Jupyter notebook in this repository from the command line. The instructor will add these commands to the comments in the zoom channel so you can copy paste. 14 | - Open `pandas_tutorial.ipynb`. To execute each cell, press shift+enter at the same time. The instructor will step through the first few cells, but you'll get to finish this one on your own. 15 | 16 | 3) Short Tutorial on numpy, scipy and astropy 17 | - Use git to download this repository (git folder). 18 | - Study 'Introduction to Numpy, Scipy and Astropy.ipynb' 19 | 20 | 21 | 22 | ## Assignments for this Week: 23 | 24 | ### I Paper of the week: 25 | Paper on a the planetary systems around Proxima Centauri: https://www.pnas.org/doi/pdf/10.1073/pnas.1706680114 26 | 27 | Refer to our [paper reading guide](https://github.com/howardisaacson/Intro-to-Astro-2020/blob/master/Week1_Intro_unix_python/how_to_read_scientific_papers.md) while reading this paper! 28 | 29 | Post 2-3 questions you have about this paper on Discord. In addition, please answer at least one of your classmates' questions. You can do this anonymously if you'd like! 30 | 31 | ### II Respond to Discussion Question 2 in "Discussion Questions" above 32 | 33 | ### III Numpy: 34 | 35 | Main Website: 36 | http://www.numpy.org 37 | 38 | Tutorial for this week: 39 | https://docs.scipy.org/doc/numpy/user/quickstart.html 40 | 41 | Bonus round: 100 Numpy commands 42 | https://github.com/rougier/numpy-100/blob/master/100_Numpy_exercises.ipynb 43 | (This notebook can be cloned to your local computer) 44 | 45 | ### IV Pandas: 46 | The `pandas` module is very handy for accessing data in python. You can think of it as a python version of excel filled with columns of data and rows for each item described by those columns. Because `pandas` allows us to create these "spreadsheets" in python, we can do powerful analysis when we combine `pandas` with other modules, like `numpy` and `matplotlib`. Your `pandas` assignment for this week is to complete the tutorial notebook in this section until the challenge section. After you've done this, check out the `pandas` main website where you can find all the documentation describing the use of this python module. 47 | 48 | #### 1. Pandas Assignment 49 | 50 | [Tutorial for this week](pandas_tutorial.ipynb) 51 | 52 | Main Website: 53 | https://pandas.pydata.org 54 | 55 | #### 2. Bonus Pandas Assignment 56 | 57 | [Challenge Section of this week's tutorial](pandas_tutorial.ipynb) 58 | 59 | Head over to https://stackoverflow.com and see if you can find a question about `pandas` by searching for it in the search bar. What words do you understand in this question that you didn't understand last week? What words are still new? Ask a question about one of the new words on Discord to find out its definition. 60 | 61 | #### 3. More Pandas Tutorials 62 | 63 | https://bitbucket.org/hrojas/learn-pandas/src/master/ 64 | 65 | ### V Numpy, Scipy and Astropy 66 | 67 | -Complete the problem 'Problem_Set_on_Numpy_Scipy_Astropy.ipynb'' 68 | 69 | 70 | ### VI Scipy (optional): 71 | https://scipy.org 72 | 73 | Scipy is an incredibly powerful module for conducting high level scientific computing. Because we are 74 | focusing on the basics of scientific computing in this class, only a single basic tutorial will be assigned. 75 | For those of you who desire more depth, please explore the full tutorials page linked from the scipy homepage. 76 | 77 | Tutorial for this week: 78 | https://docs.scipy.org/doc/scipy/reference/tutorial/interpolate.html 79 | This tutorial covers a very common tool used in astronomy, interpolation. 80 | For a full list of scipy tutorials [click here](https://docs.scipy.org/doc/scipy/reference/tutorial/index.html) 81 | -------------------------------------------------------------------------------- /Week2_Python_Packages/astropy_upload.ipynb: -------------------------------------------------------------------------------- 1 | { 2 | "cells": [ 3 | { 4 | "cell_type": "markdown", 5 | "id": "911b940e-2e1f-40d3-ad18-5ae24a0d6649", 6 | "metadata": {}, 7 | "source": [ 8 | "# Intro to Astropy" 9 | ] 10 | }, 11 | { 12 | "cell_type": "markdown", 13 | "id": "d35c17a3-7936-4c78-94e9-c6998a06c717", 14 | "metadata": {}, 15 | "source": [ 16 | "## Importing astropy" 17 | ] 18 | }, 19 | { 20 | "cell_type": "markdown", 21 | "id": "539b0c91-d26c-4fc9-9cce-65fa259c9964", 22 | "metadata": {}, 23 | "source": [ 24 | "You could import all of astropy, which is a huge, huge library, but it is not recommended! Ideally you import a subpackage or a class within the subpackage that is relevant to the operations of the script at hand, which is what we'll be doing in the rest of the notebook" 25 | ] 26 | }, 27 | { 28 | "cell_type": "markdown", 29 | "id": "2110f015-13fd-4014-846b-e7df615143d1", 30 | "metadata": {}, 31 | "source": [ 32 | "## Quantities" 33 | ] 34 | }, 35 | { 36 | "cell_type": "markdown", 37 | "id": "10b1db07-4f9b-48bc-aec0-ba6a2776cd3b", 38 | "metadata": {}, 39 | "source": [ 40 | "First go through the slides for an introduction, and then attempt the following problem:\n", 41 | "\n", 42 | "Calculate the gravitational force between a 3 solar mass star and its 10 Jupiter mass planet 2 au away. " 43 | ] 44 | }, 45 | { 46 | "cell_type": "code", 47 | "execution_count": null, 48 | "id": "f1ce3db0-36a0-4276-86ee-5f7d826a2837", 49 | "metadata": { 50 | "tags": [] 51 | }, 52 | "outputs": [], 53 | "source": [ 54 | "# import the subpackages to save quantities as objects with units and have pre-defined constants\n", 55 | "import astropy.units as u\n", 56 | "import astropy.constants as c" 57 | ] 58 | }, 59 | { 60 | "cell_type": "markdown", 61 | "id": "d9612000-8bb1-4a3e-98b5-9e09b857abde", 62 | "metadata": {}, 63 | "source": [ 64 | "### Examples with astropy.units" 65 | ] 66 | }, 67 | { 68 | "cell_type": "code", 69 | "execution_count": null, 70 | "id": "8f272f7b-e491-44a6-a9bd-9c4ff3eed9c4", 71 | "metadata": {}, 72 | "outputs": [], 73 | "source": [ 74 | "# create a velocity \n", 75 | "q = 15.1 * u.meter / (32.0 * u.second)\n", 76 | "print(q.value)\n", 77 | "print(q.unit)" 78 | ] 79 | }, 80 | { 81 | "cell_type": "code", 82 | "execution_count": null, 83 | "id": "f6e79fb6-f131-4c4e-b54b-899b53378425", 84 | "metadata": {}, 85 | "outputs": [], 86 | "source": [ 87 | "# create convert units\n", 88 | "x = 1.0 * u.parsec\n", 89 | "x.to(u.km) " 90 | ] 91 | }, 92 | { 93 | "cell_type": "markdown", 94 | "id": "9d3d609b-6428-4e8d-a4e8-29fe407ed140", 95 | "metadata": {}, 96 | "source": [ 97 | "### Examples with astropy.constants" 98 | ] 99 | }, 100 | { 101 | "cell_type": "code", 102 | "execution_count": null, 103 | "id": "43e15850-afaf-41f0-ac2a-31a71387c4a2", 104 | "metadata": {}, 105 | "outputs": [], 106 | "source": [ 107 | "# what does a constant object entail?\n", 108 | "print(c.G)" 109 | ] 110 | }, 111 | { 112 | "cell_type": "markdown", 113 | "id": "9ed2edc4-d6f7-4a97-8fbe-036e4dd3ccb0", 114 | "metadata": {}, 115 | "source": [ 116 | "### DIY" 117 | ] 118 | }, 119 | { 120 | "cell_type": "code", 121 | "execution_count": null, 122 | "id": "56b57287-e42f-4ddf-a987-374eb64ac8f2", 123 | "metadata": {}, 124 | "outputs": [], 125 | "source": [ 126 | "#masses with units of M_sun and M_jub\n", 127 | "\n", 128 | "#distance with unit of au\n", 129 | "\n", 130 | "#Calculate gravitational force using masses distance and the gravitational constant G\n" 131 | ] 132 | }, 133 | { 134 | "cell_type": "markdown", 135 | "id": "3c45fbf3-0508-4069-88b6-82a9c06ff984", 136 | "metadata": {}, 137 | "source": [ 138 | "## Input and Output" 139 | ] 140 | }, 141 | { 142 | "cell_type": "markdown", 143 | "id": "7a08b006-080e-46f2-a5f2-be9fa4891d14", 144 | "metadata": {}, 145 | "source": [ 146 | "### Tables\n", 147 | "\n", 148 | "Look at the slide for information" 149 | ] 150 | }, 151 | { 152 | "cell_type": "markdown", 153 | "id": "5d9e6ed4-0c1e-446b-ab1b-bea4bcee7d93", 154 | "metadata": { 155 | "tags": [] 156 | }, 157 | "source": [ 158 | "### FITS" 159 | ] 160 | }, 161 | { 162 | "cell_type": "code", 163 | "execution_count": null, 164 | "id": "477ed333-3c6f-4927-a945-35bd9800f5a0", 165 | "metadata": { 166 | "tags": [] 167 | }, 168 | "outputs": [], 169 | "source": [ 170 | "fits_img_fn" 171 | ] 172 | }, 173 | { 174 | "cell_type": "code", 175 | "execution_count": null, 176 | "id": "1cc61458-6374-48d2-8f99-d88f8ce7cc83", 177 | "metadata": { 178 | "tags": [] 179 | }, 180 | "outputs": [], 181 | "source": [ 182 | "# import i/o subpackage for reading FITS files\n", 183 | "from astropy.io import fits\n", 184 | "\n", 185 | "# Get path for data that came with astropy installation\n", 186 | "fits_img_fn = fits.util.get_testdata_filepath('test0.fits')\n", 187 | "\n", 188 | "# open HDU object for file and see what it contains\n", 189 | "hdul = fits.open(fits_img_fn) # header data unit (HDU) list\n", 190 | "hdul.info()" 191 | ] 192 | }, 193 | { 194 | "cell_type": "code", 195 | "execution_count": null, 196 | "id": "b0b1dcb9-9ac0-41a6-a894-ecce3ab617eb", 197 | "metadata": { 198 | "tags": [] 199 | }, 200 | "outputs": [], 201 | "source": [ 202 | "# what does the data look like? how do you \"get data\" from the file?\n", 203 | "\n", 204 | "# fits.getdata\n", 205 | "\n", 206 | "# hdul[1].data\n" 207 | ] 208 | }, 209 | { 210 | "cell_type": "markdown", 211 | "id": "dc57c17e-5a68-4cd4-962c-a03b1d6c8f29", 212 | "metadata": {}, 213 | "source": [ 214 | "## Planning Observations\n", 215 | "\n", 216 | "Planning observations takes into account the targets, dates and times, location of observing, moon cycle, etc." 217 | ] 218 | }, 219 | { 220 | "cell_type": "markdown", 221 | "id": "3d90c05e-468b-4aea-a414-f53163f8136f", 222 | "metadata": { 223 | "tags": [] 224 | }, 225 | "source": [ 226 | "### Example: Looking at Fomalhaut\n", 227 | "\n", 228 | "Here's a simple start-- You have to plan an observation of Fomalhaut from Subaru." 229 | ] 230 | }, 231 | { 232 | "cell_type": "markdown", 233 | "id": "2c744743-e5f1-491e-a7be-7ba1694a244c", 234 | "metadata": { 235 | "tags": [] 236 | }, 237 | "source": [ 238 | "#### Step 1: \n", 239 | "The first step is to generate the coordinates of the star and the observing site. The packages here are a hint\n" 240 | ] 241 | }, 242 | { 243 | "cell_type": "code", 244 | "execution_count": null, 245 | "id": "fd295531-5933-42b8-b752-673e8b4ff283", 246 | "metadata": { 247 | "tags": [] 248 | }, 249 | "outputs": [], 250 | "source": [ 251 | "from astropy.coordinates import SkyCoord, EarthLocation, AltAz\n", 252 | "from astroplan import Observer\n", 253 | "\n", 254 | "# get coordinates of fomalhaut\n", 255 | "\n", 256 | "# get observatory info and store its coordinates as an EarthLocation" 257 | ] 258 | }, 259 | { 260 | "cell_type": "markdown", 261 | "id": "f54cabb9-dc03-4f36-b8af-103f5d025571", 262 | "metadata": {}, 263 | "source": [ 264 | "#### Step 2:\n", 265 | "\n", 266 | "Visualise and plot its visibility on a date of your choice" 267 | ] 268 | }, 269 | { 270 | "cell_type": "code", 271 | "execution_count": null, 272 | "id": "5895d2fb-22c1-4987-a47c-c2b662d6f90c", 273 | "metadata": { 274 | "tags": [] 275 | }, 276 | "outputs": [], 277 | "source": [ 278 | "fomalhaut = SkyCoord.from_name('Fomalhaut')\n", 279 | "subaru = Observer.at_site('Subaru', timezone ='US/Hawaii')\n", 280 | "subaru_loc = EarthLocation(lat=subaru.latitude, lon=subaru.longitude)\n", 281 | "print(f'Sky Coords of Fomalhaut: {fomalhaut} and Geocentric Coords of Subaru: {subaru_loc}')" 282 | ] 283 | }, 284 | { 285 | "cell_type": "code", 286 | "execution_count": null, 287 | "id": "2b5cf9ed-a592-44fb-82c9-08f997e0212d", 288 | "metadata": { 289 | "tags": [] 290 | }, 291 | "outputs": [], 292 | "source": [ 293 | "# determine position for a give date: Let's say Jul 31 2024\n", 294 | "from astropy.time import Time\n", 295 | "# coz you'll need this\n", 296 | "import numpy as np\n", 297 | "\n", 298 | "# define midnight \n", 299 | "midnight = Time('2024-07-31 00:00:00')\n", 300 | "# Define grid of times to calculate position over:\n", 301 | "delta_midnight = np.linspace(-12, 12, 1000)*u.hour \n", 302 | "times = midnight + delta_midnight\n", 303 | "\n", 304 | "# Set up AltAz reference frame for these times and location\n", 305 | "frame= AltAz(obstime=times, location=subaru_loc)\n", 306 | "\n", 307 | "# Now we transform the Fomalhaut object to the Altitute/Azimuth coordinate system\n", 308 | "fomalhaut_altaz = fomalhaut.transform_to(frame)" 309 | ] 310 | }, 311 | { 312 | "cell_type": "code", 313 | "execution_count": null, 314 | "id": "b9854a77-0011-4b43-aaa8-abb441b1a700", 315 | "metadata": { 316 | "tags": [] 317 | }, 318 | "outputs": [], 319 | "source": [ 320 | "# now... can we see this source at night? this would depend on where the sun is\n", 321 | "from astropy.coordinates import get_sun\n", 322 | "\n" 323 | ] 324 | }, 325 | { 326 | "cell_type": "code", 327 | "execution_count": null, 328 | "id": "2db81353-aeb0-4269-b56a-a462c5bb671e", 329 | "metadata": { 330 | "tags": [] 331 | }, 332 | "outputs": [], 333 | "source": [ 334 | "# for plotting\n", 335 | "import matplotlib.pyplot as plt\n", 336 | "\n", 337 | "# astropy's visualisation tool\n", 338 | "from astropy.visualization import astropy_mpl_style\n", 339 | "\n", 340 | "\n", 341 | "plt.style.use(astropy_mpl_style)\n", 342 | "\n", 343 | "plt.figure()\n", 344 | "\n", 345 | "# Plot the sun altitude\n", 346 | "\n", 347 | "\n", 348 | "# Plot Fomalhaut's alt/az - use a colour map to represent azimuth. Scatter plot is advises\n", 349 | "\n", 350 | "\n", 351 | "# Now plot the range when the sun is below the horizon, and at least 18 degrees below \n", 352 | "# the horizon - this shows the range of twilight (-0 to -18 deg) and night (< -18 deg)\n", 353 | "plt.fill_between(delta_midnight.to('hr').value, 0, 90,\n", 354 | " sun_altaz.alt < 0*u.deg, color='0.7', zorder=0)\n", 355 | "plt.fill_between(delta_midnight.to('hr').value, 0, 90,\n", 356 | " sun_altaz.alt < -18*u.deg, color='0.4', zorder=0)\n", 357 | "\n", 358 | "#now for the details\n", 359 | "plt.colorbar().set_label('Azimuth [deg]')\n", 360 | "plt.legend(loc='upper left')\n", 361 | "plt.xlim(-12, 12)\n", 362 | "plt.xticks(np.arange(-12, 14, 2))\n", 363 | "plt.ylim(20, 90)\n", 364 | "plt.xlabel('Hours from UT Midnight')\n", 365 | "plt.ylabel('Altitude [deg]')\n", 366 | "plt.show()\n" 367 | ] 368 | }, 369 | { 370 | "cell_type": "code", 371 | "execution_count": null, 372 | "id": "567576d7-2ff0-4663-8ab1-1978d842c87f", 373 | "metadata": {}, 374 | "outputs": [], 375 | "source": [] 376 | } 377 | ], 378 | "metadata": { 379 | "kernelspec": { 380 | "display_name": "Python 3 (ipykernel)", 381 | "language": "python", 382 | "name": "python3" 383 | }, 384 | "language_info": { 385 | "codemirror_mode": { 386 | "name": "ipython", 387 | "version": 3 388 | }, 389 | "file_extension": ".py", 390 | "mimetype": "text/x-python", 391 | "name": "python", 392 | "nbconvert_exporter": "python", 393 | "pygments_lexer": "ipython3", 394 | "version": "3.11.4" 395 | } 396 | }, 397 | "nbformat": 4, 398 | "nbformat_minor": 5 399 | } 400 | -------------------------------------------------------------------------------- /Week2_Python_Packages/cmb_data.txt: -------------------------------------------------------------------------------- 1 | 2.27 5.440747e-05 2 | 2.83 7.586293e-05 3 | 3.40 9.661513e-05 4 | 3.96 1.040373e-04 5 | 4.53 1.070719e-04 6 | 5.10 1.120196e-04 7 | 5.66 1.122569e-04 8 | 6.23 1.096516e-04 9 | 6.80 1.054286e-04 10 | 7.36 9.841153e-05 11 | 7.93 8.981281e-05 12 | 8.50 8.198409e-05 13 | 9.06 7.168298e-05 14 | 9.63 6.876334e-05 15 | 10.19 5.938393e-05 16 | 10.76 5.080545e-05 17 | 11.33 4.531691e-05 18 | 11.89 3.387597e-05 19 | 12.46 3.078197e-05 20 | 13.03 2.477285e-05 21 | 13.59 2.227385e-05 22 | 14.16 1.683310e-05 23 | 14.72 1.739617e-05 24 | 15.29 1.391096e-05 25 | 15.86 9.657071e-06 26 | 16.42 1.101075e-05 27 | 16.99 6.367935e-06 28 | 17.56 6.094620e-06 29 | 18.12 6.745990e-06 30 | 18.69 1.121086e-06 31 | 19.26 2.796062e-06 32 | 19.82 4.581407e-06 33 | 20.39 2.584110e-06 34 | 20.95 -4.177701e-07 -------------------------------------------------------------------------------- /Week2_Python_Packages/data/pdi_pi_collapsed.fits: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/data/pdi_pi_collapsed.fits -------------------------------------------------------------------------------- /Week2_Python_Packages/dataframe.txt: -------------------------------------------------------------------------------- 1 | qnamesqcountqpercentage 2 | 0qLiamq19837q0.0102 3 | 1qEmmaq18688q0.0101 4 | 2qNoahq18267q0.0097 5 | 3qOliviaq17921q0.0095 6 | 4qAvaq14924q0.0081 7 | -------------------------------------------------------------------------------- /Week2_Python_Packages/example_data.fits: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/example_data.fits -------------------------------------------------------------------------------- /Week2_Python_Packages/franck_hertz.xlsx: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/franck_hertz.xlsx -------------------------------------------------------------------------------- /Week2_Python_Packages/plot.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/plot.pdf -------------------------------------------------------------------------------- /Week2_Python_Packages/s0002.fits: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week2_Python_Packages/s0002.fits -------------------------------------------------------------------------------- /Week2_Python_Packages/save_the_pandas.csv: -------------------------------------------------------------------------------- 1 | ,names,count,percentage 2 | 0,Liam,19837,0.0102 3 | 1,Emma,18688,0.0101 4 | 2,Noah,18267,0.0097 5 | 3,Olivia,17921,0.0095 6 | 4,Ava,14924,0.0081 7 | -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/Introduction_to_matplotlib.pptx: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week3_Matplotlib_Exoplanets/Introduction_to_matplotlib.pptx -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT (UT-7), Monday July 15th, 2024. 2 | 3 | 4 | #### Agenda: 5 | * Intro 6 | * Matplotlib 7 | * Exoplanet Detection 8 | * NASA Exoplanet Archive tutorial 9 | 10 | ### Intro 11 | 12 | Feel free to share some of your thoughts on [Discord] to continue the discussion! 13 | 14 | ### Tutorials 15 | 1. Matplotlib 16 | - Scatter plot 17 | - histogram 18 | - errorbar 19 | - images 20 | 2. NASA Exoplanet Archive 21 | - What is the NASA Exoplanet Archive? 22 | - What kind of data does it contain? 23 | - How can I access the data myself? 24 | - How do I visualize the data? 25 | 26 | 27 | ### Discussion Questions 28 | 1. O, B, and A-type stars are the most massive (i.e. most luminous) types of stars. This means they also have the largest habitable zones (see the last figure in ["Life Outside the Solar System"](https://drive.google.com/file/d/1V9Aw3sex06C6Gtlo7yzfwpsQZ2VUP9BZ/view?usp=sharing)). Why, then, are they poor targets in the search for life-bearing planets? 29 | 2. How does the multiplicity of stellar systems (i.e. single stars vs binaries, triples, etc.) affect the prospects for finding life on planets? 30 | 3. If you had to distill the "ingredients" for producing intelligent life on a planet down to a short list, what would it be? 31 | 4. After reading ["Life Outside the Solar System"](https://drive.google.com/file/d/1V9Aw3sex06C6Gtlo7yzfwpsQZ2VUP9BZ/view?usp=sharing), has your opinion changed about whether or not we'll ever discover life around another star? 32 | 33 | ## Assignments for this Week 34 | 35 | ### I Matplotlib 36 | Complete Exercise 1 and 2 in python notebook demonstration 37 | 38 | 39 | ### II NASA Exoplanet Archive tutorial 40 | Complete sections 3 and 4 in the Jupyter notebook tutorial on how to use the NASA Exoplanet Archive (see instructions inside notebook). 41 | 42 | 43 | ### III Paper of the Week 44 | Read ["Growth model interpretation of planet size distribution"](https://www.pnas.org/content/116/20/9723) by Li Zeng *et al*. Refer to our [paper reading guide](https://github.com/howardisaacson/Intro-to-Astro-2021/blob/master/Week1_Intro_unix_python/how_to_read_scientific_papers.md). Post 2-3 questions you have about this paper on our class [Discord] page. In addition, please answer at least one of your classmates' questions. You can do this anonymously if you'd like! 45 | -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/data/closest_100.csv: -------------------------------------------------------------------------------- 1 | source_id,ra,ra_error,dec,dec_error,parallax,parallax_error 2 | 4062964299525805952,272.2378287453136,1.276152153583349,-27.6459156411923,0.8306178540097751,1851.8821404624455,1.2850939446366927 3 | 4065202424204492928,274.9068719056276,1.2517478977843421,-25.255882032689016,1.5714988862767636,1847.4333489420278,1.8749374489804027 4 | 4051942623265668864,276.22319346395074,0.6829586324023676,-27.140478978057512,0.5007500183060605,1686.2659581841303,1.473535368592552 5 | 4048978992784308992,273.11242146179956,1.0926370638449316,-31.184669714567487,1.3628242746600558,1634.2833535533089,1.9712314983621555 6 | 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https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week3_Matplotlib_Exoplanets/example_data.fits -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/franck_hertz.xlsx: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week3_Matplotlib_Exoplanets/franck_hertz.xlsx -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/plot.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week3_Matplotlib_Exoplanets/plot.pdf -------------------------------------------------------------------------------- /Week3_Matplotlib_Exoplanets/s0002.fits: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week3_Matplotlib_Exoplanets/s0002.fits -------------------------------------------------------------------------------- /Week4_TESS_Gaia/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT (UT-7), Monday July 22nd, 2024. 2 | Connection details will be sent via email 3 | 4 | Instructors: 5 | 6 | ### Agenda: 7 | * Intro 8 | * TESS tutorial 9 | * Gaia tutorial 10 | * Paper discussion of [Exoplanet Size Distribution](https://www.pnas.org/content/116/20/9723) 11 | 12 | ### 1: Intro 13 | * Check-in. How did the tutorials go? 14 | * What should the instructors do differently this week? 15 | 16 | ### 2: TESS Tutorial: 17 | * Brief Intro to the TESS mission 18 | * Downloading and plotting TESS's first planet 19 | * Walkthrough of the TOI list. 20 | 21 | ### 3. Tutorial on Gaia: 22 | * What is Gaia? 23 | * How can I access Gaia data? Basic and advanced queries. 24 | * A bit on ADQL 25 | * Plotting a color-magnitude diagram 26 | 27 | ### Paper for next Week: 28 | [Exoplanets with James Webb Space Telescope](https://ntrs.nasa.gov/api/citations/20180004151/downloads/20180004151.pdf) 29 | 30 | ### Assignments for this Week 31 | 32 | 1. Complete the TESS tutorial. Which TESS planet did you choose to rediscover and why? 33 | 2. Gaia Database tutorial 34 | The tutorial questions are at the bottom of the 'GaiaTutorialAssignment.ipynb' file. Make sure you try working with ADQL and do some test queries beforehand! You'll be plotting a Color-Magnitude Diagram of the 10,000 Closest Stars. 35 | Bonus Questions: 36 | - Compare your results against Figure 1 and Figure 2 in this paper: [Babusiaux et al. (2018)](https://arxiv.org/pdf/1804.09378.pdf) 37 | - What similarities and differences do you notice? 38 | 3. Look through this [Dropbox](https://www.dropbox.com/sh/jkslarj06iuvq2e/AAB5PENEy83B5rHihd2x9nEQa?dl=0) full of readings about race, gender, and other identities & the scientific community. Spend an hour (time yourself) reading whatever interests you. Write a two paragraph reflection about what you read. 39 | -------------------------------------------------------------------------------- /Week4_TESS_Gaia/data/closest_100.csv: -------------------------------------------------------------------------------- 1 | source_id,ra,ra_error,dec,dec_error,parallax,parallax_error 2 | 4062964299525805952,272.2378287453136,1.276152153583349,-27.6459156411923,0.8306178540097751,1851.8821404624455,1.2850939446366927 3 | 4065202424204492928,274.9068719056276,1.2517478977843421,-25.255882032689016,1.5714988862767636,1847.4333489420278,1.8749374489804027 4 | 4051942623265668864,276.22319346395074,0.6829586324023676,-27.140478978057512,0.5007500183060605,1686.2659581841303,1.473535368592552 5 | 4048978992784308992,273.11242146179956,1.0926370638449316,-31.184669714567487,1.3628242746600558,1634.2833535533089,1.9712314983621555 6 | 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to create scientific documents for publication. We write our text in LaTeX 8 | so that we can control the way the text is formatted and presented. To read more about LaTex, visit The LATEX project: 9 | https://www.latex-project.org/ 10 | 11 | For our tutorial, we will use a LaTex text editor called "Overleaf". Overleaf is a website that provides LaTeX templates 12 | to edit yourself. This makes it user-friendly and a great introduction to learning LaTeX. 13 | 14 | **Step 1:** 15 | Make an account on overleaf (https://www.overleaf.com/). 16 | 17 | **Step 2:** 18 | Upload the template files (available under the Week 5 github page for Intro2Astronomy), or select a different Resume/CV template that you would like to use. 19 | 20 | **Step 3:** 21 | Edit the source text/LaTeX code on the left side of the template with your information to create your own personal CV! 22 | 23 | ### What goes in a CV? 24 | 25 | A Curriculum Vitae (CV), or an academic resume, serves to summarize your accomplishments in a compact format. It is used for job interviews, grant proposals, and tends to be of general interest to people who want to connect with you in academia. Your CV should reflect you. There is no one right or wrong way to format your CV or what you should include or exclude in your CV. Usually CVs are broken down into sections. Sections can vary depending on your specific qualifications and your own personal tastes, but there are some common sections that go in most academic CV's. There are others that are common but not mandatory, and are meant to highlight the unique skills and experience of the individual. 26 | 27 | **common categories:** education, research experience, honors and awards, publications, posters/talks/conferences attended, teaching/volunteer work/outreach, coursework, technical skills (the last two are less common post-undergrad, but are super helpful for applying to more entry-level research positions) 28 | 29 | **other optional categories:** research interests, observing experience and/or high performance computing experience, languages (both for human languages and/or computer languages), extracurriculars, references, news/media (if your research is talked about in an article, if you have a blog, etc), or any category that can highlight a skill you have 30 | 31 | **categories that don't belong:** date of birth, citizenship, address, non-academic work experience (unless relevant to your academic work), extracurricular activities (sports teams, clubs, etc.), volunteer experience (unless is is related to your academic field, in which case it can go under "outreach") 32 | 33 | *note: if you don't have anything to fill out for some of these categories, don't worry! They are a good thing to keep in mind for the future, but are by no means necessary for starting research. These categories can take years (often an entire undergraduate career) to build up* 34 | 35 | ### How should a research project be described? 36 | You want to make this part concise but still highlight your accomplishments. A description of a research project should include the following: 37 | 38 | (1) your position title and institution 39 | 40 | (2) name of your advisor(s) 41 | 42 | (3) basic mission of the research 43 | 44 | (4) final output (publication, poster, presentation, written code, etc.) 45 | 46 | you may also want to describe any major skills you used (adapting code for supercomputer, developing MCMC, etc.) 47 | 48 | ### General Tips for Making a Good CV 49 | 50 | *1. Keep a list of things you want to add to it.* When you think of something that can go on your CV, write it down in a notebook or in a note on your phone. Then when you go to update your CV, you won't have to rack your brain for what to put on it. It's amazing how much this helps! 51 | 52 | *2. Look at other CV's for examples.* Go onto websites of people in your field and look at their CV's (see this week's README for examples). This can give you ideas for what categories to use and what a good CV can look like. 53 | 54 | *3. Tailor to your career stage.* Undergraduates: major, grades/GPA, honors, universities, research programs, internships, awards, conferences/talks/posters. Graduate Students: + publications. Postdocs: + more publications, evidence for independent research. Faculty: + student supervision, grant, proposals, committee, outreach, management skills. 55 | 56 | *4. Put your best accomplishments at the top!* Most of the time education and research are the first categories in a CV, but after that it is more open-ended. If you are particularly proud of your teaching experience or awards, don't be afraid to put that where the reader can see it. Employers may have limited time to review your CV, so ensure your most impressive accomplishments are easily visible. 57 | 58 | *5. Customize for each application.* : Whenever possible, tailor your CV to align with the specific institute you are applying. Is it a observing or theoretical focused institute? What qualities and skills are they seeking in applicants? 59 | 60 | *6. Seek feedback.* Have a friend/advisor/mentor review your essays (CV, statements, cover letters, websites). Their feedback can offer different perspectives, often valuable. 61 | 62 | *7. Remember, your CV is not everything.* It is okay to be unique. It is ok to have non-traditional background. It is ok to have failures. After reviewing others' CVs, reflect on your own accomplishments. If you have a strong list, great and congrats! If not, understand that career paths vary widely. Stay open-minded, have a growth mindset, and keep exploring opportunities. If you find a promising path, pursue it diligently and strive for excellence - it will pay off in the long run. 63 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/LaTeX_tutorial.aux: -------------------------------------------------------------------------------- 1 | \relax 2 | \providecommand\hyper@newdestlabel[2]{} 3 | \providecommand\HyperFirstAtBeginDocument{\AtBeginDocument} 4 | \HyperFirstAtBeginDocument{\ifx\hyper@anchor\@undefined 5 | \global\let\oldcontentsline\contentsline 6 | \gdef\contentsline#1#2#3#4{\oldcontentsline{#1}{#2}{#3}} 7 | \global\let\oldnewlabel\newlabel 8 | \gdef\newlabel#1#2{\newlabelxx{#1}#2} 9 | \gdef\newlabelxx#1#2#3#4#5#6{\oldnewlabel{#1}{{#2}{#3}}} 10 | \AtEndDocument{\ifx\hyper@anchor\@undefined 11 | \let\contentsline\oldcontentsline 12 | \let\newlabel\oldnewlabel 13 | \fi} 14 | \fi} 15 | \global\let\hyper@last\relax 16 | \gdef\HyperFirstAtBeginDocument#1{#1} 17 | \providecommand\HyField@AuxAddToFields[1]{} 18 | \providecommand\HyField@AuxAddToCoFields[2]{} 19 | \providecommand \oddpage@label [2]{} 20 | \@writefile{nav}{\headcommand {\slideentry {0}{0}{1}{1/1}{}{0}}} 21 | \@writefile{nav}{\headcommand {\beamer@framepages {1}{1}}} 22 | \@writefile{toc}{\beamer@sectionintoc {1}{What is \LaTeX ? 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\PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}figure\PYG{n+nb}{\PYGZcb{}} 3 | \PYG{k}{\PYGZbs{}centering} 4 | \PYG{k}{\PYGZbs{}includegraphics}\PYG{n+na}{[width=0.2\PYGZbs{}textwidth]}\PYG{n+nb}{\PYGZob{}}./Figures/cat.png\PYG{n+nb}{\PYGZcb{}} 5 | \PYG{k}{\PYGZbs{}caption}\PYG{n+nb}{\PYGZob{}}An image of a cat.\PYG{n+nb}{\PYGZcb{}} 6 | \PYG{k}{\PYGZbs{}label}\PYG{n+nb}{\PYGZob{}}img:cat image\PYG{n+nb}{\PYGZcb{}} 7 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}figure\PYG{n+nb}{\PYGZcb{}} 8 | \end{Verbatim} 9 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/2923E129A449A1A3B290FB9CB3335318762556F0E7C29D55187A847219DF9D00.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | The Pythagorean Theorem, 3 | \PYG{l+s+sb}{\PYGZbs{}[}\PYG{n+nb}{ a\PYGZca{}}\PYG{l+m}{2}\PYG{n+nb}{ }\PYG{o}{+}\PYG{n+nb}{ 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\PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}physics\PYG{n+nb}{\PYGZcb{}} 8 | \PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}amssymb, amsmath\PYG{n+nb}{\PYGZcb{}} 9 | \PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}cancel\PYG{n+nb}{\PYGZcb{}} 10 | 11 | \PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}document\PYG{n+nb}{\PYGZcb{}} 12 | ... 13 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}document\PYG{n+nb}{\PYGZcb{}} 14 | \end{Verbatim} 15 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/53743985B13F1F5BE2BB84B3CEE4ADFF762556F0E7C29D55187A847219DF9D00.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | \PYG{k}{\PYGZbs{}documentclass} 3 | \end{Verbatim} 4 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX 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\PYG{k}{\PYGZbs{}subsubsection}\PYG{n+nb}{\PYGZob{}}...\PYG{n+nb}{\PYGZcb{}} 3 | \PYG{k}{\PYGZbs{}paragraph}\PYG{n+nb}{\PYGZob{}}...\PYG{n+nb}{\PYGZcb{}}, \PYG{k}{\PYGZbs{}subparagraph}\PYG{n+nb}{\PYGZob{}}...\PYG{n+nb}{\PYGZcb{}} 4 | \end{Verbatim} 5 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/F923673E8AF42976116B63BC8D457216762556F0E7C29D55187A847219DF9D00.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | For \PYG{l+s}{\PYGZdl{}}\PYG{n+nb}{x }\PYG{n+nv}{\PYGZbs{}ll}\PYG{n+nb}{ }\PYG{l+m}{1}\PYG{l+s}{\PYGZdl{}} we can... 3 | \end{Verbatim} 4 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/FC93D4EBC4505F785B8ACD742844F232762556F0E7C29D55187A847219DF9D00.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | \PYG{l+s}{\PYGZdl{}}\PYG{l+m}{10}\PYG{n+nb}{\PYGZca{}}\PYG{o}{\PYGZhy{}}\PYG{l+m}{23}\PYG{l+s}{\PYGZdl{}} 3 | \end{Verbatim} 4 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/default-pyg-prefix.pygstyle: -------------------------------------------------------------------------------- 1 | 2 | \makeatletter 3 | \def\PYG@reset{\let\PYG@it=\relax \let\PYG@bf=\relax% 4 | \let\PYG@ul=\relax \let\PYG@tc=\relax% 5 | \let\PYG@bc=\relax \let\PYG@ff=\relax} 6 | \def\PYG@tok#1{\csname PYG@tok@#1\endcsname} 7 | \def\PYG@toks#1+{\ifx\relax#1\empty\else% 8 | \PYG@tok{#1}\expandafter\PYG@toks\fi} 9 | \def\PYG@do#1{\PYG@bc{\PYG@tc{\PYG@ul{% 10 | \PYG@it{\PYG@bf{\PYG@ff{#1}}}}}}} 11 | \def\PYG#1#2{\PYG@reset\PYG@toks#1+\relax+\PYG@do{#2}} 12 | 13 | \expandafter\def\csname PYG@tok@w\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.73,0.73}{##1}}} 14 | \expandafter\def\csname PYG@tok@c\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 15 | \expandafter\def\csname PYG@tok@cp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.74,0.48,0.00}{##1}}} 16 | \expandafter\def\csname PYG@tok@k\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 17 | \expandafter\def\csname PYG@tok@kp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 18 | \expandafter\def\csname PYG@tok@kt\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.69,0.00,0.25}{##1}}} 19 | \expandafter\def\csname PYG@tok@o\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 20 | \expandafter\def\csname PYG@tok@ow\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 21 | \expandafter\def\csname PYG@tok@nb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 22 | \expandafter\def\csname PYG@tok@nf\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 23 | \expandafter\def\csname PYG@tok@nc\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 24 | \expandafter\def\csname PYG@tok@nn\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 25 | \expandafter\def\csname PYG@tok@ne\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.82,0.25,0.23}{##1}}} 26 | \expandafter\def\csname PYG@tok@nv\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 27 | \expandafter\def\csname PYG@tok@no\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.53,0.00,0.00}{##1}}} 28 | \expandafter\def\csname PYG@tok@nl\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.63,0.63,0.00}{##1}}} 29 | \expandafter\def\csname PYG@tok@ni\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.60,0.60,0.60}{##1}}} 30 | \expandafter\def\csname PYG@tok@na\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.49,0.56,0.16}{##1}}} 31 | \expandafter\def\csname PYG@tok@nt\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 32 | \expandafter\def\csname PYG@tok@nd\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 33 | \expandafter\def\csname PYG@tok@s\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 34 | \expandafter\def\csname PYG@tok@sd\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 35 | \expandafter\def\csname PYG@tok@si\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 36 | \expandafter\def\csname PYG@tok@se\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.13}{##1}}} 37 | \expandafter\def\csname PYG@tok@sr\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 38 | \expandafter\def\csname PYG@tok@ss\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 39 | \expandafter\def\csname PYG@tok@sx\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 40 | \expandafter\def\csname PYG@tok@m\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 41 | \expandafter\def\csname PYG@tok@gh\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 42 | \expandafter\def\csname PYG@tok@gu\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.50,0.00,0.50}{##1}}} 43 | \expandafter\def\csname PYG@tok@gd\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.63,0.00,0.00}{##1}}} 44 | \expandafter\def\csname PYG@tok@gi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.63,0.00}{##1}}} 45 | \expandafter\def\csname PYG@tok@gr\endcsname{\def\PYG@tc##1{\textcolor[rgb]{1.00,0.00,0.00}{##1}}} 46 | \expandafter\def\csname PYG@tok@ge\endcsname{\let\PYG@it=\textit} 47 | \expandafter\def\csname PYG@tok@gs\endcsname{\let\PYG@bf=\textbf} 48 | \expandafter\def\csname PYG@tok@gp\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 49 | \expandafter\def\csname PYG@tok@go\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.53,0.53,0.53}{##1}}} 50 | \expandafter\def\csname PYG@tok@gt\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.27,0.87}{##1}}} 51 | \expandafter\def\csname PYG@tok@err\endcsname{\def\PYG@bc##1{\setlength{\fboxsep}{0pt}\fcolorbox[rgb]{1.00,0.00,0.00}{1,1,1}{\strut ##1}}} 52 | \expandafter\def\csname PYG@tok@kc\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 53 | \expandafter\def\csname PYG@tok@kd\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 54 | \expandafter\def\csname PYG@tok@kn\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 55 | \expandafter\def\csname PYG@tok@kr\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 56 | \expandafter\def\csname PYG@tok@bp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 57 | \expandafter\def\csname PYG@tok@fm\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 58 | \expandafter\def\csname PYG@tok@vc\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 59 | \expandafter\def\csname PYG@tok@vg\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 60 | \expandafter\def\csname PYG@tok@vi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 61 | \expandafter\def\csname PYG@tok@vm\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 62 | \expandafter\def\csname PYG@tok@sa\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 63 | \expandafter\def\csname PYG@tok@sb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 64 | \expandafter\def\csname PYG@tok@sc\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 65 | \expandafter\def\csname PYG@tok@dl\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 66 | \expandafter\def\csname PYG@tok@s2\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 67 | \expandafter\def\csname PYG@tok@sh\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 68 | \expandafter\def\csname PYG@tok@s1\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 69 | \expandafter\def\csname PYG@tok@mb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 70 | \expandafter\def\csname PYG@tok@mf\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 71 | \expandafter\def\csname PYG@tok@mh\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 72 | \expandafter\def\csname PYG@tok@mi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 73 | \expandafter\def\csname PYG@tok@il\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 74 | \expandafter\def\csname PYG@tok@mo\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 75 | \expandafter\def\csname PYG@tok@ch\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 76 | \expandafter\def\csname PYG@tok@cm\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 77 | \expandafter\def\csname PYG@tok@cpf\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 78 | \expandafter\def\csname PYG@tok@c1\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 79 | \expandafter\def\csname PYG@tok@cs\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 80 | 81 | \def\PYGZbs{\char`\\} 82 | \def\PYGZus{\char`\_} 83 | \def\PYGZob{\char`\{} 84 | \def\PYGZcb{\char`\}} 85 | \def\PYGZca{\char`\^} 86 | \def\PYGZam{\char`\&} 87 | \def\PYGZlt{\char`\<} 88 | \def\PYGZgt{\char`\>} 89 | \def\PYGZsh{\char`\#} 90 | \def\PYGZpc{\char`\%} 91 | \def\PYGZdl{\char`\$} 92 | \def\PYGZhy{\char`\-} 93 | \def\PYGZsq{\char`\'} 94 | \def\PYGZdq{\char`\"} 95 | \def\PYGZti{\char`\~} 96 | % for compatibility with earlier versions 97 | \def\PYGZat{@} 98 | \def\PYGZlb{[} 99 | \def\PYGZrb{]} 100 | \makeatother 101 | 102 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_tutorial/default.pygstyle: -------------------------------------------------------------------------------- 1 | 2 | \makeatletter 3 | \def\PYGdefault@reset{\let\PYGdefault@it=\relax \let\PYGdefault@bf=\relax% 4 | \let\PYGdefault@ul=\relax \let\PYGdefault@tc=\relax% 5 | \let\PYGdefault@bc=\relax \let\PYGdefault@ff=\relax} 6 | \def\PYGdefault@tok#1{\csname PYGdefault@tok@#1\endcsname} 7 | \def\PYGdefault@toks#1+{\ifx\relax#1\empty\else% 8 | \PYGdefault@tok{#1}\expandafter\PYGdefault@toks\fi} 9 | \def\PYGdefault@do#1{\PYGdefault@bc{\PYGdefault@tc{\PYGdefault@ul{% 10 | \PYGdefault@it{\PYGdefault@bf{\PYGdefault@ff{#1}}}}}}} 11 | \def\PYGdefault#1#2{\PYGdefault@reset\PYGdefault@toks#1+\relax+\PYGdefault@do{#2}} 12 | 13 | \expandafter\def\csname PYGdefault@tok@w\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.73,0.73}{##1}}} 14 | \expandafter\def\csname PYGdefault@tok@c\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 15 | \expandafter\def\csname PYGdefault@tok@cp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.74,0.48,0.00}{##1}}} 16 | \expandafter\def\csname PYGdefault@tok@k\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 17 | \expandafter\def\csname PYGdefault@tok@kp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 18 | \expandafter\def\csname PYGdefault@tok@kt\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.69,0.00,0.25}{##1}}} 19 | \expandafter\def\csname PYGdefault@tok@o\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 20 | \expandafter\def\csname PYGdefault@tok@ow\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 21 | \expandafter\def\csname PYGdefault@tok@nb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 22 | \expandafter\def\csname PYGdefault@tok@nf\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 23 | \expandafter\def\csname PYGdefault@tok@nc\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 24 | \expandafter\def\csname PYGdefault@tok@nn\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 25 | \expandafter\def\csname PYGdefault@tok@ne\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.82,0.25,0.23}{##1}}} 26 | \expandafter\def\csname PYGdefault@tok@nv\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 27 | \expandafter\def\csname PYGdefault@tok@no\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.53,0.00,0.00}{##1}}} 28 | \expandafter\def\csname PYGdefault@tok@nl\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.63,0.63,0.00}{##1}}} 29 | \expandafter\def\csname PYGdefault@tok@ni\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.60,0.60,0.60}{##1}}} 30 | \expandafter\def\csname PYGdefault@tok@na\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.49,0.56,0.16}{##1}}} 31 | \expandafter\def\csname PYGdefault@tok@nt\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 32 | \expandafter\def\csname PYGdefault@tok@nd\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 33 | \expandafter\def\csname PYGdefault@tok@s\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 34 | \expandafter\def\csname PYGdefault@tok@sd\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 35 | \expandafter\def\csname PYGdefault@tok@si\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 36 | \expandafter\def\csname PYGdefault@tok@se\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.13}{##1}}} 37 | \expandafter\def\csname PYGdefault@tok@sr\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 38 | \expandafter\def\csname PYGdefault@tok@ss\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 39 | \expandafter\def\csname PYGdefault@tok@sx\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 40 | \expandafter\def\csname PYGdefault@tok@m\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 41 | \expandafter\def\csname PYGdefault@tok@gh\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 42 | \expandafter\def\csname PYGdefault@tok@gu\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.50,0.00,0.50}{##1}}} 43 | \expandafter\def\csname PYGdefault@tok@gd\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.63,0.00,0.00}{##1}}} 44 | \expandafter\def\csname PYGdefault@tok@gi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.63,0.00}{##1}}} 45 | \expandafter\def\csname PYGdefault@tok@gr\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{1.00,0.00,0.00}{##1}}} 46 | \expandafter\def\csname PYGdefault@tok@ge\endcsname{\let\PYGdefault@it=\textit} 47 | \expandafter\def\csname PYGdefault@tok@gs\endcsname{\let\PYGdefault@bf=\textbf} 48 | \expandafter\def\csname PYGdefault@tok@gp\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 49 | \expandafter\def\csname PYGdefault@tok@go\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.53,0.53,0.53}{##1}}} 50 | \expandafter\def\csname PYGdefault@tok@gt\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.27,0.87}{##1}}} 51 | \expandafter\def\csname PYGdefault@tok@err\endcsname{\def\PYGdefault@bc##1{\setlength{\fboxsep}{0pt}\fcolorbox[rgb]{1.00,0.00,0.00}{1,1,1}{\strut ##1}}} 52 | \expandafter\def\csname PYGdefault@tok@kc\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 53 | \expandafter\def\csname PYGdefault@tok@kd\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 54 | \expandafter\def\csname PYGdefault@tok@kn\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 55 | \expandafter\def\csname PYGdefault@tok@kr\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 56 | \expandafter\def\csname PYGdefault@tok@bp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 57 | \expandafter\def\csname PYGdefault@tok@fm\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 58 | \expandafter\def\csname PYGdefault@tok@vc\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 59 | \expandafter\def\csname PYGdefault@tok@vg\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 60 | \expandafter\def\csname PYGdefault@tok@vi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 61 | \expandafter\def\csname PYGdefault@tok@vm\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 62 | \expandafter\def\csname PYGdefault@tok@sa\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 63 | \expandafter\def\csname PYGdefault@tok@sb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 64 | \expandafter\def\csname PYGdefault@tok@sc\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 65 | \expandafter\def\csname PYGdefault@tok@dl\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 66 | \expandafter\def\csname PYGdefault@tok@s2\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 67 | \expandafter\def\csname PYGdefault@tok@sh\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 68 | \expandafter\def\csname PYGdefault@tok@s1\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 69 | \expandafter\def\csname PYGdefault@tok@mb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 70 | \expandafter\def\csname PYGdefault@tok@mf\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 71 | \expandafter\def\csname PYGdefault@tok@mh\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 72 | \expandafter\def\csname PYGdefault@tok@mi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 73 | \expandafter\def\csname PYGdefault@tok@il\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 74 | \expandafter\def\csname PYGdefault@tok@mo\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 75 | \expandafter\def\csname PYGdefault@tok@ch\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 76 | \expandafter\def\csname PYGdefault@tok@cm\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 77 | \expandafter\def\csname PYGdefault@tok@cpf\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 78 | \expandafter\def\csname PYGdefault@tok@c1\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 79 | \expandafter\def\csname PYGdefault@tok@cs\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 80 | 81 | \def\PYGdefaultZbs{\char`\\} 82 | \def\PYGdefaultZus{\char`\_} 83 | \def\PYGdefaultZob{\char`\{} 84 | \def\PYGdefaultZcb{\char`\}} 85 | \def\PYGdefaultZca{\char`\^} 86 | \def\PYGdefaultZam{\char`\&} 87 | \def\PYGdefaultZlt{\char`\<} 88 | \def\PYGdefaultZgt{\char`\>} 89 | \def\PYGdefaultZsh{\char`\#} 90 | \def\PYGdefaultZpc{\char`\%} 91 | \def\PYGdefaultZdl{\char`\$} 92 | \def\PYGdefaultZhy{\char`\-} 93 | \def\PYGdefaultZsq{\char`\'} 94 | \def\PYGdefaultZdq{\char`\"} 95 | \def\PYGdefaultZti{\char`\~} 96 | % for compatibility with earlier versions 97 | \def\PYGdefaultZat{@} 98 | \def\PYGdefaultZlb{[} 99 | \def\PYGdefaultZrb{]} 100 | \makeatother 101 | 102 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/08A2B04D709025F9E47DCD217156ACB0C45D995AE810B8705B9F959AF97E5C0D.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | \PYG{k}{\PYGZbs{}\PYGZus{}} 3 | \end{Verbatim} 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-------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | The net force is 3 | \PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}align*\PYG{n+nb}{\PYGZcb{}} 4 | F\PYG{n+nb}{\PYGZus{}\PYGZob{}}net\PYG{n+nb}{\PYGZcb{}} \PYG{n+nb}{\PYGZam{}}= \PYG{k}{\PYGZbs{}sum}\PYG{n+nb}{\PYGZus{}}i F\PYG{n+nb}{\PYGZus{}}i \PYG{k}{\PYGZbs{}\PYGZbs{}} 5 | \PYG{n+nb}{\PYGZam{}}= F \PYGZhy{} F\PYG{n+nb}{\PYGZus{}}f \PYG{k}{\PYGZbs{}\PYGZbs{}} 6 | \PYG{n+nb}{\PYGZam{}}= m a 7 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}align*\PYG{n+nb}{\PYGZcb{}} 8 | \end{Verbatim} 9 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/18B68DED28B3B7DA233821C5F7DFFD7AC45D995AE810B8705B9F959AF97E5C0D.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | \PYG{k}{\PYGZbs{}newpage} 3 | \end{Verbatim} 4 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/1B6305911B86D1951F4AA91AC6422B5FC45D995AE810B8705B9F959AF97E5C0D.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | Partl\PYGZti{}\PYG{k}{\PYGZbs{}cite}\PYG{n+nb}{\PYGZob{}}pa\PYG{n+nb}{\PYGZcb{}} has 3 | proposed that \PYG{k}{\PYGZbs{}ldots} 4 | \PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}thebibliography\PYG{n+nb}{\PYGZcb{}\PYGZob{}}99\PYG{n+nb}{\PYGZcb{}} 5 | \PYG{k}{\PYGZbs{}bibitem}\PYG{n+nb}{\PYGZob{}}pa\PYG{n+nb}{\PYGZcb{}} H.\PYGZti{}Partl: 6 | \PYG{k}{\PYGZbs{}emph}\PYG{n+nb}{\PYGZob{}}German \PYG{k}{\PYGZbs{}TeX}\PYG{n+nb}{\PYGZcb{}}, 7 | TUGboat Volume\PYGZti{}9, Issue\PYGZti{}1 (1988) 8 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}thebibliography\PYG{n+nb}{\PYGZcb{}} 9 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}document\PYG{n+nb}{\PYGZcb{}} 10 | \end{Verbatim} 11 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/1DDEE85B3A44D145B01F57FCA1C2B2ECC45D995AE810B8705B9F959AF97E5C0D.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | \PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}figure\PYG{n+nb}{\PYGZcb{}} 3 | \PYG{k}{\PYGZbs{}centering} 4 | \PYG{k}{\PYGZbs{}includegraphics}\PYG{n+na}{[width=0.2\PYGZbs{}textwidth]}\PYG{n+nb}{\PYGZob{}}./Figures/cat.png\PYG{n+nb}{\PYGZcb{}} 5 | \PYG{k}{\PYGZbs{}caption}\PYG{n+nb}{\PYGZob{}}An image of a cat.\PYG{n+nb}{\PYGZcb{}} 6 | \PYG{k}{\PYGZbs{}label}\PYG{n+nb}{\PYGZob{}}img:cat image\PYG{n+nb}{\PYGZcb{}} 7 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}figure\PYG{n+nb}{\PYGZcb{}} 8 | \end{Verbatim} 9 | 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\PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}physics\PYG{n+nb}{\PYGZcb{}} 8 | \PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}amssymb, amsmath\PYG{n+nb}{\PYGZcb{}} 9 | \PYG{k}{\PYGZbs{}usepackage}\PYG{n+nb}{\PYGZob{}}cancel\PYG{n+nb}{\PYGZcb{}} 10 | 11 | \PYG{k}{\PYGZbs{}begin}\PYG{n+nb}{\PYGZob{}}document\PYG{n+nb}{\PYGZcb{}} 12 | ... 13 | \PYG{k}{\PYGZbs{}end}\PYG{n+nb}{\PYGZob{}}document\PYG{n+nb}{\PYGZcb{}} 14 | \end{Verbatim} 15 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/527C556828BFAC0C5EF39774F3494B57C45D995AE810B8705B9F959AF97E5C0D.pygtex: -------------------------------------------------------------------------------- 1 | \begin{Verbatim}[commandchars=\\\{\}] 2 | documentclass 3 | \end{Verbatim} 4 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX 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Tutorial/_minted-LaTeX_workshop/default-pyg-prefix.pygstyle: -------------------------------------------------------------------------------- 1 | 2 | \makeatletter 3 | \def\PYG@reset{\let\PYG@it=\relax \let\PYG@bf=\relax% 4 | \let\PYG@ul=\relax \let\PYG@tc=\relax% 5 | \let\PYG@bc=\relax \let\PYG@ff=\relax} 6 | \def\PYG@tok#1{\csname PYG@tok@#1\endcsname} 7 | \def\PYG@toks#1+{\ifx\relax#1\empty\else% 8 | \PYG@tok{#1}\expandafter\PYG@toks\fi} 9 | \def\PYG@do#1{\PYG@bc{\PYG@tc{\PYG@ul{% 10 | \PYG@it{\PYG@bf{\PYG@ff{#1}}}}}}} 11 | \def\PYG#1#2{\PYG@reset\PYG@toks#1+\relax+\PYG@do{#2}} 12 | 13 | \expandafter\def\csname PYG@tok@gd\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.63,0.00,0.00}{##1}}} 14 | \expandafter\def\csname PYG@tok@gu\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.50,0.00,0.50}{##1}}} 15 | \expandafter\def\csname PYG@tok@gt\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.27,0.87}{##1}}} 16 | \expandafter\def\csname PYG@tok@gs\endcsname{\let\PYG@bf=\textbf} 17 | \expandafter\def\csname PYG@tok@gr\endcsname{\def\PYG@tc##1{\textcolor[rgb]{1.00,0.00,0.00}{##1}}} 18 | \expandafter\def\csname PYG@tok@cm\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 19 | \expandafter\def\csname PYG@tok@vg\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 20 | \expandafter\def\csname PYG@tok@vi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 21 | \expandafter\def\csname PYG@tok@vm\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 22 | \expandafter\def\csname PYG@tok@mh\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 23 | \expandafter\def\csname PYG@tok@cs\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 24 | \expandafter\def\csname PYG@tok@ge\endcsname{\let\PYG@it=\textit} 25 | \expandafter\def\csname PYG@tok@vc\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 26 | \expandafter\def\csname PYG@tok@il\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 27 | \expandafter\def\csname PYG@tok@go\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.53,0.53,0.53}{##1}}} 28 | \expandafter\def\csname PYG@tok@cp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.74,0.48,0.00}{##1}}} 29 | \expandafter\def\csname PYG@tok@gi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.63,0.00}{##1}}} 30 | \expandafter\def\csname PYG@tok@gh\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 31 | \expandafter\def\csname PYG@tok@ni\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.60,0.60,0.60}{##1}}} 32 | \expandafter\def\csname PYG@tok@nl\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.63,0.63,0.00}{##1}}} 33 | \expandafter\def\csname PYG@tok@nn\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 34 | \expandafter\def\csname PYG@tok@no\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.53,0.00,0.00}{##1}}} 35 | \expandafter\def\csname PYG@tok@na\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.49,0.56,0.16}{##1}}} 36 | \expandafter\def\csname PYG@tok@nb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 37 | \expandafter\def\csname PYG@tok@nc\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 38 | \expandafter\def\csname PYG@tok@nd\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 39 | \expandafter\def\csname PYG@tok@ne\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.82,0.25,0.23}{##1}}} 40 | \expandafter\def\csname PYG@tok@nf\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 41 | \expandafter\def\csname PYG@tok@si\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 42 | \expandafter\def\csname PYG@tok@s2\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 43 | \expandafter\def\csname PYG@tok@nt\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 44 | \expandafter\def\csname PYG@tok@nv\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 45 | \expandafter\def\csname PYG@tok@s1\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 46 | \expandafter\def\csname PYG@tok@dl\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 47 | \expandafter\def\csname PYG@tok@ch\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 48 | \expandafter\def\csname PYG@tok@m\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 49 | \expandafter\def\csname PYG@tok@gp\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 50 | \expandafter\def\csname PYG@tok@sh\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 51 | \expandafter\def\csname PYG@tok@ow\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 52 | \expandafter\def\csname PYG@tok@sx\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 53 | \expandafter\def\csname PYG@tok@bp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 54 | \expandafter\def\csname PYG@tok@c1\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 55 | \expandafter\def\csname PYG@tok@fm\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 56 | \expandafter\def\csname PYG@tok@o\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 57 | \expandafter\def\csname PYG@tok@kc\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 58 | \expandafter\def\csname PYG@tok@c\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 59 | \expandafter\def\csname PYG@tok@mf\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 60 | \expandafter\def\csname PYG@tok@err\endcsname{\def\PYG@bc##1{\setlength{\fboxsep}{0pt}\fcolorbox[rgb]{1.00,0.00,0.00}{1,1,1}{\strut ##1}}} 61 | \expandafter\def\csname PYG@tok@mb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 62 | \expandafter\def\csname PYG@tok@ss\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 63 | \expandafter\def\csname PYG@tok@sr\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 64 | \expandafter\def\csname PYG@tok@mo\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 65 | \expandafter\def\csname PYG@tok@kd\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 66 | \expandafter\def\csname PYG@tok@mi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 67 | \expandafter\def\csname PYG@tok@kn\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 68 | \expandafter\def\csname PYG@tok@cpf\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 69 | \expandafter\def\csname PYG@tok@kr\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 70 | \expandafter\def\csname PYG@tok@s\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 71 | \expandafter\def\csname PYG@tok@kp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 72 | \expandafter\def\csname PYG@tok@w\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.73,0.73}{##1}}} 73 | \expandafter\def\csname PYG@tok@kt\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.69,0.00,0.25}{##1}}} 74 | \expandafter\def\csname PYG@tok@sc\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 75 | \expandafter\def\csname PYG@tok@sb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 76 | \expandafter\def\csname PYG@tok@sa\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 77 | \expandafter\def\csname PYG@tok@k\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 78 | \expandafter\def\csname PYG@tok@se\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.73,0.40,0.13}{##1}}} 79 | \expandafter\def\csname PYG@tok@sd\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 80 | 81 | \def\PYGZbs{\char`\\} 82 | \def\PYGZus{\char`\_} 83 | \def\PYGZob{\char`\{} 84 | \def\PYGZcb{\char`\}} 85 | \def\PYGZca{\char`\^} 86 | \def\PYGZam{\char`\&} 87 | \def\PYGZlt{\char`\<} 88 | \def\PYGZgt{\char`\>} 89 | \def\PYGZsh{\char`\#} 90 | \def\PYGZpc{\char`\%} 91 | \def\PYGZdl{\char`\$} 92 | \def\PYGZhy{\char`\-} 93 | \def\PYGZsq{\char`\'} 94 | \def\PYGZdq{\char`\"} 95 | \def\PYGZti{\char`\~} 96 | % for compatibility with earlier versions 97 | \def\PYGZat{@} 98 | \def\PYGZlb{[} 99 | \def\PYGZrb{]} 100 | \makeatother 101 | 102 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/_minted-LaTeX_workshop/default.pygstyle: -------------------------------------------------------------------------------- 1 | 2 | \makeatletter 3 | \def\PYGdefault@reset{\let\PYGdefault@it=\relax \let\PYGdefault@bf=\relax% 4 | \let\PYGdefault@ul=\relax \let\PYGdefault@tc=\relax% 5 | \let\PYGdefault@bc=\relax \let\PYGdefault@ff=\relax} 6 | \def\PYGdefault@tok#1{\csname PYGdefault@tok@#1\endcsname} 7 | \def\PYGdefault@toks#1+{\ifx\relax#1\empty\else% 8 | \PYGdefault@tok{#1}\expandafter\PYGdefault@toks\fi} 9 | \def\PYGdefault@do#1{\PYGdefault@bc{\PYGdefault@tc{\PYGdefault@ul{% 10 | \PYGdefault@it{\PYGdefault@bf{\PYGdefault@ff{#1}}}}}}} 11 | \def\PYGdefault#1#2{\PYGdefault@reset\PYGdefault@toks#1+\relax+\PYGdefault@do{#2}} 12 | 13 | \expandafter\def\csname PYGdefault@tok@gd\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.63,0.00,0.00}{##1}}} 14 | \expandafter\def\csname PYGdefault@tok@gu\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.50,0.00,0.50}{##1}}} 15 | \expandafter\def\csname PYGdefault@tok@gt\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.27,0.87}{##1}}} 16 | \expandafter\def\csname PYGdefault@tok@gs\endcsname{\let\PYGdefault@bf=\textbf} 17 | \expandafter\def\csname PYGdefault@tok@gr\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{1.00,0.00,0.00}{##1}}} 18 | \expandafter\def\csname PYGdefault@tok@cm\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 19 | \expandafter\def\csname PYGdefault@tok@vg\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 20 | \expandafter\def\csname PYGdefault@tok@vi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 21 | \expandafter\def\csname PYGdefault@tok@vm\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 22 | \expandafter\def\csname PYGdefault@tok@mh\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 23 | \expandafter\def\csname PYGdefault@tok@cs\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 24 | \expandafter\def\csname PYGdefault@tok@ge\endcsname{\let\PYGdefault@it=\textit} 25 | \expandafter\def\csname PYGdefault@tok@vc\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 26 | \expandafter\def\csname PYGdefault@tok@il\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 27 | \expandafter\def\csname PYGdefault@tok@go\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.53,0.53,0.53}{##1}}} 28 | \expandafter\def\csname PYGdefault@tok@cp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.74,0.48,0.00}{##1}}} 29 | \expandafter\def\csname PYGdefault@tok@gi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.63,0.00}{##1}}} 30 | \expandafter\def\csname PYGdefault@tok@gh\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 31 | \expandafter\def\csname PYGdefault@tok@ni\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.60,0.60,0.60}{##1}}} 32 | \expandafter\def\csname PYGdefault@tok@nl\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.63,0.63,0.00}{##1}}} 33 | \expandafter\def\csname PYGdefault@tok@nn\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 34 | \expandafter\def\csname PYGdefault@tok@no\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.53,0.00,0.00}{##1}}} 35 | \expandafter\def\csname PYGdefault@tok@na\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.49,0.56,0.16}{##1}}} 36 | \expandafter\def\csname PYGdefault@tok@nb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 37 | \expandafter\def\csname PYGdefault@tok@nc\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 38 | \expandafter\def\csname PYGdefault@tok@nd\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 39 | \expandafter\def\csname PYGdefault@tok@ne\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.82,0.25,0.23}{##1}}} 40 | \expandafter\def\csname PYGdefault@tok@nf\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 41 | \expandafter\def\csname PYGdefault@tok@si\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 42 | \expandafter\def\csname PYGdefault@tok@s2\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 43 | \expandafter\def\csname PYGdefault@tok@nt\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 44 | \expandafter\def\csname PYGdefault@tok@nv\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 45 | \expandafter\def\csname PYGdefault@tok@s1\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 46 | \expandafter\def\csname PYGdefault@tok@dl\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 47 | \expandafter\def\csname PYGdefault@tok@ch\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 48 | \expandafter\def\csname PYGdefault@tok@m\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 49 | \expandafter\def\csname PYGdefault@tok@gp\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,0.50}{##1}}} 50 | \expandafter\def\csname PYGdefault@tok@sh\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 51 | \expandafter\def\csname PYGdefault@tok@ow\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.67,0.13,1.00}{##1}}} 52 | \expandafter\def\csname PYGdefault@tok@sx\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 53 | \expandafter\def\csname PYGdefault@tok@bp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 54 | \expandafter\def\csname PYGdefault@tok@c1\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 55 | \expandafter\def\csname PYGdefault@tok@fm\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.00,1.00}{##1}}} 56 | \expandafter\def\csname PYGdefault@tok@o\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 57 | \expandafter\def\csname PYGdefault@tok@kc\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 58 | \expandafter\def\csname PYGdefault@tok@c\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 59 | \expandafter\def\csname PYGdefault@tok@mf\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 60 | \expandafter\def\csname PYGdefault@tok@err\endcsname{\def\PYGdefault@bc##1{\setlength{\fboxsep}{0pt}\fcolorbox[rgb]{1.00,0.00,0.00}{1,1,1}{\strut ##1}}} 61 | \expandafter\def\csname PYGdefault@tok@mb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 62 | \expandafter\def\csname PYGdefault@tok@ss\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.10,0.09,0.49}{##1}}} 63 | \expandafter\def\csname PYGdefault@tok@sr\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.53}{##1}}} 64 | \expandafter\def\csname PYGdefault@tok@mo\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 65 | \expandafter\def\csname PYGdefault@tok@kd\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 66 | \expandafter\def\csname PYGdefault@tok@mi\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}} 67 | \expandafter\def\csname PYGdefault@tok@kn\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 68 | \expandafter\def\csname PYGdefault@tok@cpf\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.25,0.50,0.50}{##1}}} 69 | \expandafter\def\csname PYGdefault@tok@kr\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 70 | \expandafter\def\csname PYGdefault@tok@s\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 71 | \expandafter\def\csname PYGdefault@tok@kp\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 72 | \expandafter\def\csname PYGdefault@tok@w\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.73,0.73}{##1}}} 73 | \expandafter\def\csname PYGdefault@tok@kt\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.69,0.00,0.25}{##1}}} 74 | \expandafter\def\csname PYGdefault@tok@sc\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 75 | \expandafter\def\csname PYGdefault@tok@sb\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 76 | \expandafter\def\csname PYGdefault@tok@sa\endcsname{\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 77 | \expandafter\def\csname PYGdefault@tok@k\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.00,0.50,0.00}{##1}}} 78 | \expandafter\def\csname PYGdefault@tok@se\endcsname{\let\PYGdefault@bf=\textbf\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.40,0.13}{##1}}} 79 | \expandafter\def\csname PYGdefault@tok@sd\endcsname{\let\PYGdefault@it=\textit\def\PYGdefault@tc##1{\textcolor[rgb]{0.73,0.13,0.13}{##1}}} 80 | 81 | \def\PYGdefaultZbs{\char`\\} 82 | \def\PYGdefaultZus{\char`\_} 83 | \def\PYGdefaultZob{\char`\{} 84 | \def\PYGdefaultZcb{\char`\}} 85 | \def\PYGdefaultZca{\char`\^} 86 | \def\PYGdefaultZam{\char`\&} 87 | \def\PYGdefaultZlt{\char`\<} 88 | \def\PYGdefaultZgt{\char`\>} 89 | \def\PYGdefaultZsh{\char`\#} 90 | \def\PYGdefaultZpc{\char`\%} 91 | \def\PYGdefaultZdl{\char`\$} 92 | \def\PYGdefaultZhy{\char`\-} 93 | \def\PYGdefaultZsq{\char`\'} 94 | \def\PYGdefaultZdq{\char`\"} 95 | \def\PYGdefaultZti{\char`\~} 96 | % for compatibility with earlier versions 97 | \def\PYGdefaultZat{@} 98 | \def\PYGdefaultZlb{[} 99 | \def\PYGdefaultZrb{]} 100 | \makeatother 101 | 102 | 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https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/figures/programming-comic.jpg -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/figures/sps-logo.jpg: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/figures/sps-logo.jpg -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/figures/texstackexchange.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/figures/texstackexchange.png -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/LaTeX Tutorial/references.bib: -------------------------------------------------------------------------------- 1 | @unpublished{notsoshort, 2 | title = "{The Not So Short Introduction to LaTeX}", 3 | author = {Tobias Oetiker}, 4 | note={https://tobi.oetiker.ch/lshort/lshort.pdf}, 5 | year = {2015}, 6 | url={https://tobi.oetiker.ch/lshort/lshort.pdf} 7 | } -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/README.md: -------------------------------------------------------------------------------- 1 | README: 2 | # Agenda: 3 | 4 | ### Intro 5 | - Intro, Check-in. 6 | 7 | ### Tutorial: 8 | 1. Creating a Curriculum Vitae (CV) 9 | 2. Creating a website 10 | 3. Latex and Overleaf for writing papers 11 | 12 | # Assignments: 13 | 1. Look up the personal websites (NOT university faculty page!) of at least five different astronomers. Explore them in detail. Write an entry in your notebook describing what you like and what you don't like. Remember, a website is often times many people's first impression of you, what do you want them to know? Remember to consider content as well as aesthetics. Use this in planning a design for your personal website. 14 | 15 | 2. Review these astronomers' CVs which are always posted somewhere on their websites. Record trends in your notebook. What aspects of their CVs do you want to emulate? Do they have sections of their CV that we did not cover or bring up? 16 | 17 | 3. Read this article on building a website: https://researcheracademy.elsevier.com/uploads/2017-11/ECR_Building_personal_website_210912.pdf 18 | 19 | 4. Create a website using the platform of your choice. You may use a template or create a site from scratch. 20 | 21 | 5. Create an account on overleaf (https://www.overleaf.com/) and make a draft of a CV. See the "CV Guidelines" for more information. 22 | 23 | 6. Check your work from last week against the tutorial answer key (posted in week 4 folder) 24 | 25 | 7. Overleaf/Latex 26 | - Creating and saving a document. 27 | - Choice of template 28 | - Equations, Figures, Tables 29 | 30 | 31 | ### Resources: 32 | Here are some examples of websites from various undergrads, grad students/post docs, and faculty. Feel free to browse them for inspiration! 33 | 34 | *undergrad websites:* 35 | 36 | https://arjunsavel.github.io/ (Arjun Savel, undergrad) 37 | 38 | *grad student/post doc websites:* 39 | 40 | https://sites.psu.edu/szs714/ (Sofia Sheikh, grad student) 41 | 42 | https://rrubenza.github.io/ (Ryan Rubenzahl, grad student) 43 | 44 | 45 | *faculty websites:* 46 | 47 | https://exoplanets.caltech.edu/(Andrew Howard, Professor) 48 | 49 | http://w.astro.berkeley.edu/~dressing/ (Courtney Dressing, professor) 50 | 51 | https://www.erikpetigura.com/ (Erik Petigura, professor) 52 | 53 | Weekly Reading: 54 | [Direct Imaging of Exoplanets](https://arxiv.org/pdf/1810.02031.pdf) 55 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Homework Assignment/RR_PHYXXX_HWX.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/Templates/Homework Assignment/RR_PHYXXX_HWX.pdf -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Homework Assignment/RR_PHYXXX_HWX.tex: -------------------------------------------------------------------------------- 1 | \documentclass[11pt, oneside]{article} 2 | \usepackage[top=2.2cm, bottom=2cm, left=1cm, right=2cm]{geometry} 3 | \geometry{letterpaper} 4 | 5 | \usepackage{fancyhdr} 6 | \usepackage{graphicx} 7 | \usepackage{tikz} 8 | \usepackage{float} 9 | 10 | \usepackage{physics} 11 | \usepackage{amssymb} 12 | \usepackage{amsmath} 13 | \usepackage{cancel} 14 | 15 | \usepackage{verbatim} 16 | \usepackage[shortlabels]{enumitem} 17 | 18 | \setlength\parindent{22pt} 19 | \pagestyle{fancy} 20 | \fancyhf{} 21 | \lhead{Ryan Rubenzahl} 22 | \chead{PHY XXX} 23 | \rhead{HW X} 24 | 25 | \rfoot{\thepage} 26 | 27 | \begin{document} 28 | 29 | \begin{enumerate} 30 | 31 | \item 32 | 33 | 34 | 35 | 36 | 37 | 38 | 39 | 40 | \end{enumerate} 41 | 42 | \end{document} 43 | 44 | -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Physics Lab Report/PhysicsLabTemplate.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/Templates/Physics Lab Report/PhysicsLabTemplate.pdf -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Physics Lab Report/PhysicsLabTemplate.tex: -------------------------------------------------------------------------------- 1 | \documentclass[11pt, oneside]{article} % <-- Could change the font size up here 2 | \usepackage{geometry} % Packages and things to be imported that may be used 3 | \geometry{letterpaper} % Later on in tables, figures, etc. 4 | \usepackage{graphicx} 5 | 6 | \usepackage{amssymb} 7 | \usepackage{float} 8 | \usepackage{array} 9 | 10 | 11 | 12 | \title{Physics Lab Template} 13 | \author{\underline{Your Name}, Partner Name} 14 | \date{Tuesday, February 9th, 2015} 15 | 16 | \begin{document} % Starts the Document 17 | \maketitle % Makes the Title 18 | 19 | 20 | \abstract % Latex has its own abstract heading! 21 | Abstract section where you discuss what you found, if you wish to type a math equation inside text, use dollar signs on either side of your equation: $g = 9.81m/s^2$ 22 | 23 | 24 | 25 | 26 | \section{Theory} 27 | Theory section 28 | 29 | \subsection{Part 1} 30 | Some specific part of the theory behind the experiment 31 | \newline % Go to the next line 32 | % The next commented section gives the layout to make a figure at the location in the document where it is typed 33 | 34 | % \begin{figure}[H] 35 | % \centering 36 | % \includegraphics[scale=0.3]{Folder/diagramname.jpg} 37 | % \caption{This is what figure 1 is} 38 | % \label{Figure 1} 39 | % \end{figure} 40 | \par Might use equations to to describe something, like % \par does paragraph indentation 41 | \begin{equation} \vec{L} = I \vec{\omega} \end{equation} 42 | 43 | 44 | \section{Experiment} 45 | Experiment section 46 | 47 | 48 | 49 | \section{Data Analysis} 50 | Might want a table to present data: 51 | 52 | \begin{table}[h] 53 | \centering 54 | \begin{tabular}{|c|c|c|} 55 | \hline 56 | Trial & 1 & 2 \\ \hline 57 | $\theta_1$ & 1 & 2 \\ \hline 58 | $\theta_2$ & 1 & 2 \\ \hline 59 | \end{tabular} 60 | \caption{caption about table 1} 61 | \label{Table 1} 62 | \end{table} 63 | 64 | Of course, error propagation will be in here: 65 | \begin{equation} \sigma = \sqrt{\left(\frac{\partial}{\partial x}\right)^2\sigma _x^2+\left(\frac{\partial}{\partial y}\right)^2\sigma _y^2 + \left(\frac{\partial}{\partial z}\right)^2\sigma _z^2...} \end{equation} 66 | 67 | Maybe some weighted mean: 68 | \begin{equation} w_i = \frac{1}{\sigma_i^2} \end{equation} 69 | \begin{equation} x_{mean} = \frac{\sum\limits_{i=1}^N{w_ix_i}}{\sum\limits_{i=1}^N{w_i}} \end{equation} 70 | \begin{equation} \sigma_{mean} = \frac{1}{\sqrt{\sum\limits_{i=1}^N{w_i}}} \end{equation} 71 | 72 | 73 | \section{Conclusion} 74 | Summary 75 | 76 | 77 | 78 | \section{Remarks} 79 | remarks 80 | 81 | 82 | 83 | 84 | \end{document} % Ends the masterpiece -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project1.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project1.pdf -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project1.tex: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project1.tex -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project2.pdf: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project2.pdf -------------------------------------------------------------------------------- /Week5_CV_Latex_Overleaf_website/Templates/Project Report/RR_PHYXXX_Project2.tex: 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-17.581042654028437 5 | 3.799999999999999, -10.948815165876766 6 | 3.9499999999999993, -3.368720379146936 7 | 4.65, 51.59431279620851 8 | 4.799999999999999, 60.59620853080567 9 | 4.949999999999999, 65.80663507109001 10 | 5.649999999999999, 47.78388625592413 11 | 5.950000000000001, 20.2900473933649 12 | 11.7, -43.326066350710875 13 | 11.849999999999998, -36.69383886255923 14 | 12.649999999999999, 29.641706161137407 15 | 12.899999999999999, 34.850236966824625 16 | 13.649999999999999, 65.6417061611374 17 | 13.849999999999998, 57.107109004739314 18 | 14.699999999999996, 0.6928909952606546 19 | 14.749999999999996, -3.573459715639842 20 | 14.849999999999998, -8.788625592417077 21 | 14.899999999999999, -23.95545023696681 22 | 15.649999999999999, -48.61421800947869 23 | 15.799999999999997, -43.40379146919429 24 | 15.899999999999999, -55.254028436018956 25 | 16.65, 12.030331753554492 26 | 16.799999999999997, 14.871090047393352 27 | 16.9, 18.66066350710898 28 | 17.75, 65.56398104265399 29 | 17.849999999999998, 62.24454976303315 30 | 18.649999999999995, 28.106161137440736 31 | 18.8, 8.198104265402833 32 | 18.85, -5.546919431279633 33 | 19.65, -41.58104265402844 34 | 19.749999999999996, -57.22274881516586 35 | 19.9, -56.2777251184834 36 | 20.599999999999998, -18.37630331753556 37 | 20.75, -6.056872037914701 38 | 20.849999999999998, 7.685308056872032 39 | 21.599999999999998, 58.38199052132697 40 | 21.65, 61.22464454976301 41 | 21.7, 68.80663507109001 42 | 23.599999999999998, -33.125118483412336 43 | 23.65, -35.96966824644551 44 | 23.699999999999996, -29.33554502369671 45 | 23.749999999999996, -40.710900473933634 46 | 24.65, -31.723222748815175 47 | 24.75, -25.563981042654007 48 | 24.849999999999998, -20.826540284360192 49 | 25.65, 47.40473933649285 50 | 25.699999999999996, 49.29952606635068 51 | 25.75, 57.82938388625588 52 | 26.65, 71.55639810426537 53 | 26.65, 66.81706161137438 54 | 26.75, 63.97156398104262 55 | 26.75, 52.59715639810425 56 | 27.699999999999996, -20.40663507109005 57 | 27.799999999999997, -29.887203791469204 58 | 28.599999999999994, -42.22464454976301 59 | 28.749999999999993, -37.48815165876778 60 | 28.64999999999999, -31.325118483412325 61 | 28.849999999999994, -33.22464454976304 62 | 29.65, 26.94976303317533 63 | 29.700000000000003, 36.90142180094783 64 | 29.75, 43.06161137440756 65 | 30.699999999999996, 64.84454976303314 66 | 30.75, 58.68246445497627 67 | 30.599999999999994, 61.52890995260661 68 | 30.849999999999994, 52.51943127962083 69 | 31.699999999999996, 2.7402843601895484 70 | 31.749999999999993, -1.52606635071092 71 | -------------------------------------------------------------------------------- /Week6_RV_Summer_Research/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT (UT-7), Monday July 5th, 2024. 2 | Connection details will be sent via email 3 | 4 | Instructors: 5 | Mentor Profiles: 6 | 7 | ### Agenda: 8 | * Intro 9 | * Fitting Methods + Radvel tutorial 10 | * Summer Research 11 | 12 | 13 | ### Tutorials: 14 | 1. Fitting methods + Radvel Tutorial 15 | 2. Summer Research 16 | 17 | ### Assignments for this Week 18 | 19 | 1. Complete the remaining `#TODO` items in the RadVel tutorial 20 | 2. Complete the remaining `#TODO` items in the Bayesian Fitting tutorial 21 | 3. Figure out a list of summer research positions you would like to apply to next summer. Note the deadlines and required materials 22 | 23 | ### Paper for this Week 24 | One of the very first results from the James Webb Space Telescope 25 | https://arxiv.org/abs/2211.10487 26 | -------------------------------------------------------------------------------- /Week6_RV_Summer_Research/Radial Velocities Assignment -- Finding the Orbital Parameters of ___.ipynb: -------------------------------------------------------------------------------- 1 | { 2 | "cells": [ 3 | { 4 | "cell_type": "markdown", 5 | "id": "c2cfa925", 6 | "metadata": {}, 7 | "source": [ 8 | "*Quick note: make sure you have the following packages installed before using this notebook!*" 9 | ] 10 | }, 11 | { 12 | "cell_type": "code", 13 | "execution_count": 1, 14 | "id": "2cf681cb", 15 | "metadata": {}, 16 | "outputs": [], 17 | "source": [ 18 | "from astropy.stats import LombScargle # for periodograms\n", 19 | "import corner # for visualizing parameter distributions\n", 20 | "import numpy as np # for math and data storage\n", 21 | "import pandas as pd # for math and data storage\n", 22 | "import matplotlib.pyplot as plt # for plot making\n", 23 | "import radvel # for fitting RVs\n", 24 | "from radvel.plot import orbit_plots, mcmc_plots # for visualizing RVs\n", 25 | "from scipy import optimize # for fitting RVs\n", 26 | "\n", 27 | "# this bit below is just to fix an issue with radvel that appears if you're using numpy versions 1.22.0 or later!\n", 28 | "try:\n", 29 | " np.__config__.blas_opt_info = np.__config__.blas_ilp64_opt_info\n", 30 | "except Exception:\n", 31 | " pass" 32 | ] 33 | }, 34 | { 35 | "cell_type": "markdown", 36 | "id": "570f4671", 37 | "metadata": {}, 38 | "source": [ 39 | "# Finding the Orbital Parameters of ???\n", 40 | "\n", 41 | "Welcome to the Radial Velocities assignment! In this assignment, you're going to be finding the mass (or minimum mass) of a planet from radial velocity measurements from scratch, all on your own.\n", 42 | "\n", 43 | "This is a very open-ended assignment, and I'd like you to code it all on your own! You pick the planet, you code it up. That said, I will give some steps (that you don't have to follow but may be helpful):\n", 44 | "\n", 45 | "1. Figure out which planet you want to find the orbital parameters of! Not all RV data is good to work with, especially for people still getting used to RVs. Ideally, you find a planet that:\n", 46 | "- is the only planet in its system (otherwise you'll have two signals! You can model them both if you want a challenge, but you don't need to here.)\n", 47 | "- is a very massive planet! If you have Earthike planets, the signals start getting too small for RV methods to detect without also having to model things like stellar variability (and trust me -- as someone who struggles to do that as a job, it's tough!)\n", 48 | "- Around a Sun-like star (really small stars have very high signal semi-amplitudes but have a lot of stellar variability, while really big stars have very small RV semi-amplitudes!\n", 49 | "- Has RVs from only one instrument, as each instrument may have different offsets or quirks that make them more difficult to model together\n", 50 | "- Has RVs you can easily download and access yourself!\n", 51 | "\n", 52 | " Here are a few papers containing RVs that satisfy those bullet points! You don't need to use them, but they're here if you'd rather not find a system yourself.\n", 53 | "- TrES-2 b, with its paper [here](https://iopscience.iop.org/article/10.1086/509123/pdf)\n", 54 | "- HAT-P-15 b, with its paper [here](https://iopscience.iop.org/article/10.1088/0004-637X/724/2/866)\n", 55 | "- HD 22532 b, with its paper [here](https://www.aanda.org/articles/aa/full_html/2022/01/aa40078-20/aa40078-20.html)\n", 56 | "\n", 57 | "2. Download and read in the data! In some papers (like the HAT-P-15 b paper or the HD 22532 paper), the RVs are available in a downloadable table in the paper. Sometimes, the data is linked through data centers like CDS, or maybe Simbad or Vizier; sometimes, like in the TrES-2 b paper, you just need to copy and paste the table into a .txt file :/ In any case, get the data and read it in. To make sure you know it works, maybe try plotting your RVs as a function of time, with error bars if you can!\n", 58 | "\n", 59 | "3. Figure out your priors! Some of these are going to be informed by realistic numbers (e.g. informing that your jitter cannot be negative), while some of these are going to be informed by previous studies. For example, if the paper you're getting your RV data from notes that this planet is transiting, use priors informed by the transits for $P$ and $t_0$! (RVs can figure out those two values to the tune of hours or minutes, but transits can get so much more precise values for those -- down to a fraction of a second in some cases -- that it's worth just using the values of $P$ and $t_0$ from transit fits for your priors.)\n", 60 | "\n", 61 | "4. Figure out what values to initialize your parameters to. It's okay to just do this by eye if you don't have better options, but if you have better options use them! For example, it might be worth making your own peridogram to figure out what value to initialize your planet's period to if you don't have transit data.\n", 62 | "\n", 63 | "5. Run a simple optimization fit!\n", 64 | "\n", 65 | "6. Do an MCMC fit.\n", 66 | "\n", 67 | "7. Look at your results! Do they look reasonable? Are they consistent with the results found in the papers you got data from?" 68 | ] 69 | }, 70 | { 71 | "cell_type": "code", 72 | "execution_count": null, 73 | "id": "5f31b07d", 74 | "metadata": {}, 75 | "outputs": [], 76 | "source": [ 77 | "# TODO: find planet masses!" 78 | ] 79 | } 80 | ], 81 | "metadata": { 82 | "kernelspec": { 83 | "display_name": "Python 3 (ipykernel)", 84 | "language": "python", 85 | "name": "python3" 86 | }, 87 | "language_info": { 88 | "codemirror_mode": { 89 | "name": "ipython", 90 | "version": 3 91 | }, 92 | "file_extension": ".py", 93 | "mimetype": "text/x-python", 94 | "name": "python", 95 | "nbconvert_exporter": "python", 96 | "pygments_lexer": "ipython3", 97 | "version": "3.10.14" 98 | } 99 | }, 100 | "nbformat": 4, 101 | "nbformat_minor": 5 102 | } 103 | -------------------------------------------------------------------------------- /Week6_RV_Summer_Research/Summer_research_opportunities.pptx: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week6_RV_Summer_Research/Summer_research_opportunities.pptx -------------------------------------------------------------------------------- /Week6_RV_Summer_Research/WASP-12_ETD_clean.txt: -------------------------------------------------------------------------------- 1 | 1 0 2454508.976854460 0.0002 1 Hebb et al 2008 2 | 2 300 2454836.4033931005 0.0006 2 Hentunen 3 | 5 304 2454840.7686030436 0.00047 1 Tucker et al. 2011 4 | 6 304 2454840.771193043 0.001 3 Gary 5 | 11 366 2454908.437992057 0.001 3 Naves 6 | 13 387 2454931.3581816694 0.00098 3 Brát L. 7 | 16 601 2455164.923956134 0.00149 3 Shadick S. 8 | 17 601 2455164.9243161334 0.00129 3 Stan Shadick 9 | 18 608 2455172.561815919 0.00044 1 Tucker et al. 2011 10 | 19 608 2455172.562785919 0.00014 1 Ingemyr M. 11 | 21 632 2455198.756735166 0.00141 3 Tieman B. 12 | 23 661 2455230.4067300046 0.00011 1 Maciejewski et al. 2011 13 | 25 683 2455254.418869997 0.00014 1 Maciejewski et al. 2011 14 | 26 685 2455256.596033418 0.00059 3 Latham C., Schwieterman E. 15 | 28 693 2455265.3340531443 0.00129 3 Kučáková H. 16 | 31 914 2455506.533284860 0.00112 3 Naves R. 17 | 32 917 2455509.808914742 0.00087 3 Dvorak S. 18 | 33 926 2455519.632074388 0.0007 2 Naves R. 19 | 34 938 2455532.729963918 0.00035 1 Irwin S. 20 | 36 946 2455541.461083606 0.0005 2 Zambelli R. 21 | 38 978 2455576.387242368 0.00135 3 Ayiomamitis A. 22 | 39 979 2455577.4751723297 0.00038 2 Garcia R. 23 | 40 979 2455577.4767823294 0.00069 2 Naves R. 24 | 41 979 2455577.4771123296 0.00085 3 Salvaggio F., Marino G. 25 | 42 980 2455578.5684222914 0.00082 3 Poddaný S. 26 | 44 994 2455593.850191754 0.00047 2 Stan Shadick and Hao He 27 | 48 1000 2455600.398281524 0.00042 1 Cagas P. 28 | 50 1001 2455601.4892114857 0.00109 3 Brát L. 29 | 51 1003 2455603.671161409 0.00094 3 Griffith J., Condon I. 30 | 53 1011 2455612.4008011026 0.00083 3 Karashevich S. V., Sokov E. N. 31 | 54 1011 2455612.4013211024 0.00078 3 Sokov E. N. 32 | 55 1014 2455615.675910987 0.00054 2 E.Rich, S.Irwin 33 | 56 1043 2455647.3287598747 0.00173 3 Zinoviev S. , Sokov E. 34 | 58 1236 2455857.9737826996 0.00071 2 Shadic S. 35 | 59 1236 2455857.9737826996 0.00071 2 Shadic S. 36 | 61 1245 2455867.7978323917 0.00075 3 Shadic S. 37 | 63 1250 2455873.2536122217 0.00126 3 Ivanov K. 38 | 64 1254 2455877.618482087 0.00092 3 Hoeven A. 39 | 65 1254 2455877.6191620864 0.00129 3 Hoeven A. 40 | 67 1265 2455889.623301718 0.00073 3 Naves R. 41 | 68 1274 2455899.4484414198 0.00063 2 Ayiomamitis A. 42 | 69 1274 2455899.4512514197 0.00057 3 Romas E., Sokov E. 43 | 70 1275 2455900.539781387 0.00038 2 Romas E., Sokov E. 44 | 72 1279 2455904.9052712554 0.00103 3 Stan Shadick 45 | 73 1280 2455905.995241223 0.00135 3 Shadic S. 46 | 75 1286 2455912.5445610285 0.00057 2 Romas E., Sokov E. 47 | 76 1286 2455912.5445610285 0.00057 2 Romas E., Sokov E. 48 | 77 1287 2455913.636130995 0.00078 2 Lopesino J. 49 | 78 1288 2455914.7267409633 0.00047 2 Shadic S. 50 | 80 1295 2455922.370120738 0.0009 3 Sokov E. N. 51 | 82 1301 2455928.913320548 0.00073 3 Shadic S. 52 | 83 1308 2455936.5525603276 0.00091 3 Naves R. 53 | 84 1308 2455936.561520327 0.00123 3 Lopesino J. 54 | 85 1309 2455937.6454302957 0.00119 3 Naves R. 55 | 86 1310 2455938.738730265 0.00072 3 Shadic S. 56 | 87 1317 2455946.383030047 0.00077 2 Ruben Garcia 57 | 88 1318 2455947.4684800166 0.00102 3 Naves R. 58 | 89 1320 2455949.650899955 0.00059 3 Shadic S. 59 | 90 1320 2455949.650899955 0.00059 3 Shadic S. 60 | 91 1321 2455950.7425099243 0.00066 2 Stan Shadick 61 | 92 1327 2455957.2875997415 0.0011 3 Lomoz F. 62 | 93 1327 2455957.294399741 0.00104 3 Lomoz F. 63 | 94 1327 2455957.296779741 0.00057 2 Eugene Sokov 64 | 95 1327 2455957.296779741 0.00057 2 Sokov E. N. 65 | 97 1331 2455961.659129620 0.00107 3 Shadic S. 66 | 98 1332 2455962.749929590 0.00132 3 Shadic S. 67 | 100 1339 2455970.392369380 0.00086 3 Ivanov A. V., Sokov E. N. 68 | 102 1350 2455982.394919057 0.00116 3 Aceti P. 69 | 103 1360 2455993.3098687683 0.0006 2 Rusov S., Sokov E. 70 | 104 1360 2455993.3131187684 0.00076 3 Kouprianov V.V., Sokov E. N. 71 | 105 1361 2455994.3987187403 0.00068 2 Marchini A. 72 | 106 1361 2455994.399358740 0.00076 3 Sokov E. N. 73 | 107 1369 2456003.129688514 0.00063 2 Ivanov K. 74 | 108 1369 2456003.130168514 0.0006 2 Ivanov K. 75 | 110 1371 2456005.3153284574 0.00044 2 Romas E., Sokov E. 76 | 114 1570 2456222.5096953874 0.00081 3 Rusov S., Sokov E. 77 | 115 1592 2456246.516835025 0.00074 3 Ivanov A. V., Sokov E. N. 78 | 116 1595 2456249.793844979 0.00067 3 Shadic S. 79 | 118 1613 2456269.4251947156 0.0009 3 Horta F. G. 80 | 119 1615 2456271.6232646876 0.00055 2 Salisbury M. 81 | 123 1638 2456296.724384389 0.00052 2 Shadic S. 82 | 125 1645 2456304.3645343054 0.00146 3 Bourdanov A. 83 | 126 1645 2456304.3658043053 0.00089 3 Salisbury M. 84 | 127 1645 2456304.3674543053 0.00156 3 Bourdanov A. 85 | 128 1645 2456304.367784305 0.00058 2 Naumov K. N., Sokov E. N. 86 | 129 1668 2456329.4692940502 0.00164 3 Gudmundsson S. 87 | 130 1700 2456364.392543749 0.00117 3 Horta F. G. 88 | 132 1902 2456584.8601733795 0.00051 2 Benni P. 89 | 133 1912 2456595.7728134315 0.00096 3 Shadick S. 90 | 134 1913 2456596.8663834375 0.00051 2 Benni P. 91 | 135 1920 2456604.503073479 0.00092 3 Albiréo 78 92 | 136 1924 2456608.8695635046 0.00071 3 Shadic S. 93 | 137 1931 2456616.511353553 0.0009 3 Salisbury M. 94 | 138 1940 2456626.3333236203 0.00051 2 Karavaev Y., Loginovskaj A. 95 | 139 1941 2456627.4290336287 0.00105 3 Scaggiante F., Zardin D. 96 | 140 1942 2456628.515003636 0.00097 3 René R. 97 | 141 1942 2456628.5170736364 0.00088 3 Bachschmidt M. 98 | 142 1944 2456630.6997536523 0.00044 2 Benni P. 99 | 143 1952 2456639.430343721 0.00074 2 Nicolas E. 100 | 144 1952 2456639.4328937214 0.00068 3 Dittler U. 101 | 146 1953 2456640.5225537303 0.00082 3 Sokov E. N., Naumov K. 102 | 147 1954 2456641.610273739 0.0008 3 CAAT 103 | 148 1962 2456650.3415838145 0.00104 3 Gaitan J. 104 | 150 1974 2456663.4436139367 0.00076 3 René R. 105 | 152 1997 2456688.544734204 0.00054 2 Benni P. 106 | 156 2028 2456722.3725346276 0.00089 3 Gaitan J. 107 | 158 2028 2456722.3826146275 0.00108 3 René R. 108 | 159 2039 2456734.3835047917 0.00112 3 Carreñ 109 | 160 2039 2456734.388674792 0.00073 2 Horta F. G. 110 | 161 2050 2456746.3855149634 0.00139 3 Bachschmidt M. 111 | 162 2050 2456746.391884963 0.00141 3 Trnka J. 112 | 163 2216 2456927.546138298 0.00164 3 Bachschmidt M. 113 | 164 2237 2456950.4851188404 0.00074 2 Zibar M. 114 | 165 2246 2456960.3068690808 0.00057 2 Karavaev Y. 115 | 166 2249 2456963.578439162 0.00093 3 Francesco Scaggiante, Danilo Zardin 116 | 167 2249 2456963.578959162 0.00089 3 Francesco Scaggiante, Danilo Zardin,Marco Fiaschi 117 | 168 2249 2456963.582479162 0.00061 2 Matthieu BACHSCHMIDT 118 | 169 2270 2456986.501139745 0.00051 2 Mark Salisbury 119 | 170 2281 2456998.508180060 0.00145 3 Marc Bretton 120 | 171 2281 2456998.508180060 0.00145 3 Marc Bretton 121 | 173 2312 2457032.3333109776 0.00113 3 JOSEP GAITAN 122 | 174 2313 2457033.433561009 0.00046 1 Marc Bretton 123 | 175 2346 2457069.448912041 0.00051 2 Veli-Pekka Hentunen 124 | 176 2356 2457080.3675723644 0.00119 3 Jaroslav Trnka 125 | 177 2356 2457080.3675723644 0.00119 3 Jaroslav Trnka 126 | 178 2367 2457092.3683527256 0.0006 2 Mark Salisbury 127 | 179 2598 2457344.486722873 0.00065 2 Luis Tremosa 128 | 180 2598 2457344.4886928727 0.00107 3 Fran Campos 129 | 181 2599 2457345.578812914 0.00109 3 Miroslav Smolka 130 | 182 2599 2457345.5798329143 0.00049 2 David Molina 131 | 183 2609 2457356.4937333274 0.00061 2 David Molina 132 | 184 2610 2457357.5850133696 0.00052 2 David Molina 133 | 185 2610 2457357.586493369 0.00043 1 Marc Bretton 134 | 186 2620 2457368.4989637877 0.00058 2 Enrique Díez Alonso 135 | 187 2620 2457368.499653788 0.00046 1 Marc Bretton 136 | 188 2621 2457369.5894738296 0.00034 1 ESSEIVA Nicolas 137 | 189 2630 2457379.414424210 0.00089 3 David Molina 138 | 190 2630 2457379.414424210 0.00089 3 David Molina 139 | 191 2662 2457414.334725580 0.00131 3 Francesco Scaggiante, Danilo Zardin 140 | 192 2673 2457426.343356056 0.00065 2 Marc Bretton 141 | 193 2696 2457451.4472370553 0.00086 2 David Molina 142 | 194 2717 2457474.3640779685 0.00077 2 Marc Bretton 143 | 195 2717 2457474.3643479683 0.00055 2 Marc Bretton 144 | 196 2728 2457486.371248447 0.00135 3 Marc Bretton 145 | 197 2895 2457668.6377857854 0.00082 2 David Molina 146 | 198 2948 2457726.484138119 0.00055 2 Vrašťák M 147 | 199 2969 2457749.405049043 0.00084 3 Claudio Arena 148 | 200 2970 2457750.494949087 0.00053 2 Matthieu BACHSCHMIDT 149 | 201 2971 2457751.585649131 0.00094 3 Matthieu BACHSCHMIDT 150 | 202 2971 2457751.586939131 0.00072 2 David Molina 151 | 203 2976 2457757.043280925 0.00037 1 Wonseok Kang 152 | 204 2977 2457758.134850969 0.00052 1 Wonseok Kang 153 | 206 2979 2457760.3174710576 0.00067 2 Marc Bretton 154 | 207 2979 2457760.318171058 0.00103 3 Marc Bretton 155 | 208 2980 2457761.4089511014 0.00063 2 David Molina 156 | 209 2988 2457770.1403614543 0.00033 1 Wonseok Kang 157 | 210 2990 2457772.327371543 0.00099 3 David Molina 158 | 211 2991 2457773.4151615873 0.00055 2 Franky Dubois 159 | 212 2992 2457774.506521631 0.00062 2 ESSEIVA Nicolas 160 | 214 3024 2457809.4312730418 0.00072 2 David Molina 161 | 215 3024 2457809.435043042 0.00094 3 Marc Bretton 162 | 216 3045 2457832.3508739625 0.00058 2 Marc Bretton 163 | 218 3279 2458087.7458433444 0.00035 1 O. Cooper, E. Helou, J. Lowenthal, R. O’Connor, E. Papineau, A. Peck, L. Stephens, K. Walker 164 | 219 3287 2458096.474133639 0.00057 2 Claudio Arena 165 | 220 3299 2458109.571734078 0.00138 3 Mattia Spagnol 166 | 221 3319 2458131.4003147967 0.00064 2 Mario Morales 167 | 226 3562 2458396.6151619162 0.00118 3 ESSEIVA nicolas 168 | 227 3562 2458396.617561916 0.0007 2 Yves Jongen 169 | 228 3576 2458411.8960522227 0.0007 3 Riley Larochelle 170 | 229 3616 2458455.5545930467 0.00071 3 Ferran Grau Horta 171 | 230 3618 2458457.734253086 0.00055 2 James Mazur 172 | 233 3638 2458479.568743471 0.00058 2 Yves Jongen 173 | 234 3647 2458489.383453638 0.00068 2 Fran Campos 174 | 235 3647 2458489.387803638 0.00103 3 Snaevarr Gudmundsson 175 | 236 3648 2458490.477903656 0.00086 2 Ramon Naves 176 | 237 3648 2458490.4828236564 0.00085 3 Yves Jongen 177 | 238 3658 2458501.391673836 0.0003 1 Marc Bretton 178 | 239 3658 2458501.392013836 0.00076 2 Anael Wunsche 179 | 240 3658 2458501.396543836 0.00068 2 Yves Jongen 180 | 241 3669 2458513.402254027 0.00082 3 Francesco Scaggiante, Danilo Zardin 181 | 244 3691 2458537.407634385 0.00061 2 Anael Wunsche 182 | 246 3692 2458538.5077344007 0.00145 3 Jean plazas 183 | 248 3966 2458837.5501557584 0.00073 2 Manfred Raetz 184 | 249 3976 2458848.4616857045 0.0007 2 Yves Jongen 185 | 250 3986 2458859.375955644 0.00135 3 Veli-Pekka Hentunen 186 | 251 3987 2458860.4658756377 0.00082 3 Yves Jongen 187 | 252 3987 2458860.4696156373 0.00067 2 Ferran Grau Horta 188 | 253 3997 2458871.379135569 0.00094 3 Anaël Wünsche 189 | 254 3997 2458871.382555569 0.00049 2 Veli-Pekka Hentunen 190 | 255 3998 2458872.470795562 0.00113 3 Valè 191 | 256 4008 2458883.3871654863 0.00054 2 Yves Jongen 192 | 257 4008 2458883.3895554864 0.00054 2 Anaël Wünsche 193 | 258 4009 2458884.478175478 0.0007 2 Pere Guerra 194 | 259 4009 2458884.478425478 0.00079 3 SIBIL·LA LLORET GÓMEZ 195 | 260 4009 2458884.479455478 0.00084 3 Sibil·la Lloret Gómez 196 | 262 4029 2458906.3069253047 0.0006 2 Veli-Pekka Hentunen 197 | 263 4051 2458930.332215082 0.00052 1 Veli-Pekka Hentunen 198 | 265 4250 2459147.5102512357 0.00073 3 Veli-Pekka Hentunen 199 | 266 4272 2459171.5229206374 0.00064 2 Vicenç Ferrando (AAS) 200 | 267 4273 2459172.6087406105 0.00102 3 F. Lomoz 201 | 268 4273 2459172.617850610 0.00078 3 F. Lomoz 202 | 269 4283 2459183.5319103287 0.00061 2 Jordi Lopesino 203 | 270 4292 2459193.3524800707 0.00133 3 Yves Jongen 204 | 272 4293 2459194.4423400415 0.00077 2 Anaël Wünsche 205 | 273 4293 2459194.4436100414 0.00061 2 Thomas MOLLIER 206 | 274 4295 2459196.6239499836 0.00052 2 Yves Jongen 207 | 275 4296 2459197.719249954 0.00113 3 Yves Jongen 208 | 276 4317 2459220.632699325 0.00113 3 Yves Jongen 209 | 277 4337 2459242.461498697 0.00053 2 Snaevarr Gudmundsson 210 | 279 4358 2459265.384258006 0.00078 2 FERRATFIAT STEPHANE 211 | 280 4358 2459265.3843180058 0.00042 1 Ferran Grau Horta 212 | 285 4578 2459505.4956089947 0.00125 3 Giuseppe Conzo 213 | 287 4622 2459553.5146268737 0.00038 1 Snaevarr Gudmundsson 214 | 288 4622 2459553.5151368733 0.00072 3 Veli-Pekka Hentunen 215 | 289 4632 2459564.4277463825 0.00086 2 Fabio Salvaggio 216 | 290 4633 2459565.520376333 0.00047 1 Yves Jongen 217 | 291 4634 2459566.615006284 0.00095 3 Alessandro Marchini 218 | 294 4643 2459576.438095839 0.00054 2 Snaevarr Gudmundsson 219 | -------------------------------------------------------------------------------- /Week7_AO_JWST/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT (UT-7), Monday Aug 12th, 2024. 2 | 3 | ### Agenda: 4 | * Adaptive Optics 5 | * JWST! 6 | 7 | 8 | ### Tutorials: 9 | Please go through the excellent tutorial on retrieving and fitting JWST data by 10 | https://github.com/Kappibw/JWST 11 | 12 | ### Writing a Proposal 13 | ## Written by Sarah Blunt (Updated by Howard Isaacson) 14 | 15 | ## Motivation: 16 | Many undergraduate research internships do not have dedicated time for students to do literature reviews and come up with their own ideas. This project is an opportunity to do just that. We believe this project will compliment your future research experiences, and help to complete your understanding of the research process. 17 | 18 | ## Assignment: 19 | Select and read at least 3 scientific papers on a particular topic in astronomy using [SAO/NASA ADS](https://ui.adsabs.harvard.edu/). At least one of these should be a review paper. You may choose your own topic or choose from the list we’ve compiled below. As you read, come up with an idea for an original research project that could contribute to the field you’ve chosen. Your idea doesn’t have to be doable, but it must by original and advance knowledge in your chosen field. 20 | 21 | Write a proposal convincing the reader that your idea should be funded based on the results of your reading. You may assume your reader has infinite money, but must decide between your proposal and many others. 22 | 23 | ### Proposal Requirements: 24 | - 2 or more pages (double spaced, 12-pt font) 25 | - Must propose to carry out an original idea (i.e. something nobody else has done, to the best of your knowledge) 26 | - Must contribute knowledge to chosen field in astronomy. 27 | ### Proposal Guidelines: 28 | - The first ~75% of your proposal should summarize the papers you’ve read and set the stage for your idea. The remaining 25% should describe your idea and convince the reader that this project would advance knowledge in your chosen field. 29 | ### Possible Topics: 30 | - exoplanet atmospheres 31 | - exoplanet formation 32 | - exoplanet dynamics & interactions 33 | - astrobiology 34 | - Search for Extraterrestrial Intelligence (SETI) 35 | - exoplanet transits 36 | - exoplanet radial velocities 37 | - exoplanet imaging 38 | - exoplanet microlensing 39 | - asteroseismology 40 | - exoplanet population statistics 41 | 42 | 43 | * Select and read the 3 papers you will include in your report. You can use Discord to discuss your ideas and receive advice about your project. 44 | * Outline and write your proposal. You can meet virtually with an instructor to discuss your progress once this week. 45 | * You can also send your final proposal to the organinzers to receive comments. You are encouraged but not required to make these changes. We encourage you to share this proposal with potential research advisers and include it on research internship applications. 46 | 47 | ## Example Projects and Resources: 48 | 49 | This assignment is modeled after the [NSF Graduate Research Fellowship](https://www.nsfgrfp.org/) proposal application essays. For many excellent example NSF essays, see [Alex Lang’s website](http://www.alexhunterlang.com/nsf-fellowship#TOC-Examples-of-Successful-Essays) (click on any “proposal” link in the table). Your proposals should be shorter than the NSF proposals, but other than that, you can model yours exactly after the NSF ones. 50 | 51 | Isabel has compiled a list of advice for writing an effective proposal [here](https://github.com/howardisaacson/Intro-to-Astro2023/blob/main/Week8_REU_Opportunities_Proposals/Writing%20a%20Proposal.md). 52 | 53 | There are many other excellent proposal-writing resources online. I like [this one](https://www.mhc.ab.ca/services/academicsupport/~/media/a6c5e5b4dc184e8d8c72d72ec7032a2c.ashx) in particular. Please read through as many of them as is helpful! 54 | -------------------------------------------------------------------------------- /Week8_Grad_school_ML/Classification_Clustering.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week8_Grad_school_ML/Classification_Clustering.png -------------------------------------------------------------------------------- /Week8_Grad_school_ML/README.md: -------------------------------------------------------------------------------- 1 | ## Meeting Time: 5:00pm PDT (UT-7), Monday Aug 19th, 2024. 2 | 3 | 4 | ### Agenda: 5 | * Grad School Application 6 | * Machine Learning, deep learning 7 | 8 | ### Tutorials: 9 | Please go through the tutorials in Categorical_Classification.ipynb 10 | -------------------------------------------------------------------------------- /Week8_Grad_school_ML/true_distrib.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/howardisaacson/Intro-to-Astro2024/1fb4f81d275e83bc8ed7440feaff4fd23b351ab3/Week8_Grad_school_ML/true_distrib.png --------------------------------------------------------------------------------