3 | #include "cblas.h"
4 | #include "error_cblas_l3.h"
5 |
6 | #include "hypot.c"
7 |
8 | void
9 | cblas_ztrsm (const enum CBLAS_ORDER Order, const enum CBLAS_SIDE Side,
10 | const enum CBLAS_UPLO Uplo, const enum CBLAS_TRANSPOSE TransA,
11 | const enum CBLAS_DIAG Diag, const int M, const int N,
12 | const void *alpha, const void *A, const int lda, void *B,
13 | const int ldb)
14 | {
15 | #define BASE double
16 | #include "source_trsm_c.h"
17 | #undef BASE
18 | }
19 |
--------------------------------------------------------------------------------
/bin/removelines:
--------------------------------------------------------------------------------
1 | #! /usr/bin/env python3
2 | from __future__ import print_function
3 | from __future__ import absolute_import
4 | import sys
5 | # Assume this script is in $(INSTALL_DIR)/bin/ and the
6 | # python base directory is in $(INSTALL_DIR)/lib/python/ .
7 | try:
8 | # If the PYTHONPATH is already set up, don't mess with it.
9 | import astrometry.util.removelines
10 | except:
11 | import os
12 | sys.path.insert(1, os.path.normpath(os.path.join(os.path.dirname(__file__), '..', 'lib', 'python')))
13 |
14 | from astrometry.util.removelines import main
15 | sys.exit(main())
16 |
--------------------------------------------------------------------------------
/include/astrometry/dualtree_nearestneighbour.h:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | #ifndef DUALTREE_NEAREST_NEIGHBOUR_H
7 | #define DUALTREE_NEAREST_NEIGHBOUR_H
8 |
9 | #include "astrometry/kdtree.h"
10 |
11 | void dualtree_nearestneighbour(kdtree_t* xtree, kdtree_t* ytree, double maxdist2,
12 | double** nearest_d2, int** nearest_ind,
13 | int** count_within_range,
14 | int notself);
15 |
16 | #endif
17 |
18 |
--------------------------------------------------------------------------------
/man/wcsinfo.1:
--------------------------------------------------------------------------------
1 | .TH WCSINFO "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | wcsinfo \- print simple properties of WCS headers (scale, rotation, etc)
4 | .SH SYNOPSIS
5 | .B wcsinfo
6 | [options]
7 | \fIwcs-file\fR
8 | .SH OPTIONS
9 | .TP
10 | \fB\-e\fR \fIextension\fR
11 | Read from given HDU (default 0 = primary)
12 | .TP
13 | \fB\-W\fR \fIwidth\fR
14 | Set/override IMAGEW
15 | .TP
16 | \fB\-H\fR \fIheight\fR
17 | Set/override IMAGEH
18 | .SH AUTHOR
19 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
20 | Dustin Lang (CMU).
21 | .SH SEE ALSO
22 | http://astrometry.net
23 |
--------------------------------------------------------------------------------
/util/makefile.qfits:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 |
4 | QFITS_DIR := $(BASEDIR)/qfits-an
5 | QFITS_LIB_FILE := $(QFITS_DIR)/libqfits.a
6 | QFITS_SRCDIR := $(QFITS_DIR)
7 |
8 | QFITS_CFLAGS :=
9 | QFITS_INC :=
10 | QFITS_LIB :=
11 | QFITS_SLIB := $(QFITS_LIB_FILE)
12 |
13 | # $(QFITS_LIB_FILE):
14 | # $(MAKE) -C $(QFITS_DIR) libqfits.a
15 |
16 | include $(COMMON)/makefile.anbase
17 |
18 | QFITS_INC += $(ANBASE_INC)
19 | QFITS_LIB += $(ANBASE_LIB)
20 | QFITS_SLIB += $(ANBASE_SLIB)
21 | QFITS_CFLAGS += $(ANBASE_CFLAGS)
22 |
--------------------------------------------------------------------------------
/blind/tst.plot:
--------------------------------------------------------------------------------
1 | plot_wcs tst.wcs
2 | plot_wcs_setsize
3 |
4 | plot_color 0.5 0.5 0.5
5 | grid_rastep 1
6 | grid_decstep 1
7 | grid_ralabelstep 1
8 | grid_declabelstep 1
9 | grid
10 |
11 | plot_color green
12 | plot_lw 3
13 |
14 | annotations_fontsize 20
15 | annotations_target 350 0 350,0
16 | annotations_target 20 0 20,0
17 | annotations_target 0 10 0,10
18 | annotations_target 0 -10 0,-10
19 | annotations_target 10 10 10,10
20 | annotations_target -10 10 -10,10
21 | annotations_target 10 -10 10,-10
22 | annotations_target -10 -10 -10,-10
23 |
24 | annotations_target 180 0 180,0
25 |
26 | annotations
27 |
28 |
--------------------------------------------------------------------------------
/include/astrometry/brightstars.h:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | #ifndef BRIGHTSTARS_H
7 | #define BRIGHTSTARS_H
8 |
9 | struct brightstar {
10 | // Don't change the order of these fields - the included datafile depends on this order!
11 | char* name;
12 | char* common_name;
13 | double ra;
14 | double dec;
15 | double Vmag;
16 | };
17 | typedef struct brightstar brightstar_t;
18 |
19 | int bright_stars_n();
20 | const brightstar_t* bright_stars_get(int starindex);
21 |
22 | #endif
23 |
--------------------------------------------------------------------------------
/doc/changelog.rst:
--------------------------------------------------------------------------------
1 |
2 | Change Log:
3 | ===========
4 |
5 | Version 0.46:
6 | -------------
7 |
8 | * Makefile revamp. Now possible to use system GSL rather than our
9 | shipped subset, by defining SYSTEM_GSL=yes::
10 |
11 | make SYSTEM_GSL=yes
12 |
13 | * Move away from *qfits*, toward *an-qfits*; reorganize *qfits-an*
14 | directory to be more like the other source directories.
15 |
16 | * Web api: add *invert* option
17 |
18 | * Add more Intermediate World Coords options to WCS classes
19 |
20 | Version 0.47:
21 | -------------
22 |
23 | * *solve-field*: add "focalmm" as a supported image scale type.
24 |
25 |
--------------------------------------------------------------------------------
/net/templates/tag/user_image_tag_list.html:
--------------------------------------------------------------------------------
1 |
2 | {% for user_image_tag in tags %}
3 | - {{ user_image_tag.text }}
4 | {% if user == user_image_tag.tagger or user == tagged_object_owner %}
5 | [remove]
8 | {% endif %}
9 | {% endfor %}
10 |
11 |
--------------------------------------------------------------------------------
/net/templates/dashboard/index.html:
--------------------------------------------------------------------------------
1 | {% extends 'dashboard/base.html' %}
2 |
3 | {% block dashboard_content %}
4 |
5 | We had to change our login system, so logins after March 16, 2016 appear as new accounts. If you want all of the images you have uploaded previously to appear in this new account, please Email us with the old and new account names (eg, "I used to use google account bobwob@gmail.com and now I'm using Twitter account @bobwob") and we'll connect it up. Thanks!
6 |
7 | {% endblock %}
8 |
--------------------------------------------------------------------------------
/util/shell.py:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 | def shell_escape(s):
4 | repl = ('\\', '|', '&', ';', '(', ')', '<', '>', ' ', '\t',
5 | '\n', '$', "'", '"', "`")
6 | # (note, \\ must be first!)
7 | for x in repl:
8 | s = s.replace(x, '\\'+x)
9 | return s
10 |
11 | # escape a string that will appear inside double-quotes.
12 | def shell_escape_inside_quotes(s):
13 | repl = ('\\', '\t', '`', '"', '$')
14 | # (note, \\ must be first!)
15 | for x in repl:
16 | s = s.replace(x, '\\'+x)
17 | return s
18 |
--------------------------------------------------------------------------------
/include/astrometry/bl.ph:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | /// Private header file shared between bl.inc and bl.c
7 |
8 | InlineDeclare
9 | bl_node* find_node(const bl* list, size_t n, size_t* rtn_nskipped);
10 |
11 | // data follows the bl_node*.
12 | #define NODE_DATA(node) ((void*)(((bl_node*)(node)) + 1))
13 | #define NODE_CHARDATA(node) ((char*)(((bl_node*)(node)) + 1))
14 | #define NODE_INTDATA(node) ((int*)(((bl_node*)(node)) + 1))
15 | #define NODE_DOUBLEDATA(node) ((double*)(((bl_node*)(node)) + 1))
16 |
17 | #define bl_free_node free
18 |
--------------------------------------------------------------------------------
/man/pad-file.1:
--------------------------------------------------------------------------------
1 | .TH PAD-FILE "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | pad-file \- Pad a FITS file out to the correct size
4 | .SH SYNOPSIS
5 | .B pad-file
6 | \fIdesired-length input-file\fR [\fIinput-file\fR ...]
7 | .SH DESCRIPTION
8 | The file will be padded in\-place. By default, the file is padded with zeros.
9 | .SH OPTIONS
10 | .TP
11 | \fB\-v\fR \fIn\fR
12 | Numerical value of character to pad with
13 | .TP
14 | \fB\-c\fR \fIc\fR
15 | Character to pad with
16 | .SH AUTHOR
17 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
18 | Dustin Lang (CMU).
19 | .SH SEE ALSO
20 | http://astrometry.net
21 |
--------------------------------------------------------------------------------
/man/subtable.1:
--------------------------------------------------------------------------------
1 | .TH SUBTABLE "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | subtable \- Pull out a set of columns from a many-column FITS binary table.
4 | .SH SYNOPSIS
5 | .B
6 | subtable
7 | \fB\-i\fR \fIinput-file\fR \fB\-o\fR \fIoutput-file\fR
8 | \fB\-c\fR \fIcol-name\fR [\fB\-c\fR \fIcol-name\fR ...]
9 | .SH OPTIONS
10 | .TP
11 | \fB\-i\fR \fIfile\fR
12 | Input file
13 | .TP
14 | \fB\-o\fR \fIfile\fR
15 | Output file
16 | .TP
17 | \fB\-c\fR \fIname\fR
18 | Column name
19 | .SH AUTHOR
20 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
21 | Dustin Lang (CMU).
22 | .SH SEE ALSO
23 | http://astrometry.net
24 |
--------------------------------------------------------------------------------
/net/templates/radio-horizontal.html:
--------------------------------------------------------------------------------
1 | {% with id=widget.attrs.id %}
2 |
21 | {% endwith %}
22 |
--------------------------------------------------------------------------------
/qfits-an/NOTE-Astrometry.net:
--------------------------------------------------------------------------------
1 | This distribution of the qfits library is a modified version of
2 | qfits-6.2.0.
3 |
4 | We have submitted our patches upstream but have not heard back from
5 | the original author.
6 |
7 | All modified files contain a note at the top of the file (as required
8 | by the GPL):
9 |
10 | /* Note: this file has been modified from its original form by the
11 | Astrometry.net team. For details see http://astrometry.net */
12 |
13 | In turn, we hereby claim all our modifications:
14 | Copyright 2006, 2007 Dustin Lang, Keir Mierle and Sam Roweis
15 | and release our modifications under the GPL v2 or later.
16 |
17 |
18 |
19 |
--------------------------------------------------------------------------------
/include/astrometry/tic.h:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | #ifndef TIC_H
7 | #define TIC_H
8 |
9 | #include
10 | #include
11 |
12 | void tic();
13 | int get_resource_stats(double* p_usertime, double* p_systime, long* p_maxrss);
14 | void toc();
15 |
16 | double millis_between(struct timeval* tv1, struct timeval* tv2);
17 |
18 | // Returns the number of seconds since (approximately) Jan 1, 2000 UTC.
19 | // You probably only want to look at differences in the values returned by this function.
20 | double timenow();
21 |
22 | #endif
23 |
--------------------------------------------------------------------------------
/util/makefile.cfitsio:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 |
4 | # if CFITS_INC environment variable is set, assume CFITS_EXISTS.
5 | # Note also that CFITS_EXISTS can be overridden by the environment.
6 | ifeq ($(origin CFITS_INC), environment)
7 | CFITS_EXISTS := 1
8 | else
9 | X := $(shell pkg-config --exists cfitsio && echo yes || echo no)
10 | ifeq ($(X), yes)
11 | CFITS_EXISTS ?= 1
12 | endif
13 | endif
14 |
15 | CFITS_INC ?= $(shell pkg-config --cflags cfitsio 2>/dev/null)
16 | CFITS_LIB ?= $(shell pkg-config --libs cfitsio 2>/dev/null)
17 | CFITS_SLIB :=
18 |
19 |
--------------------------------------------------------------------------------
/net/client/README:
--------------------------------------------------------------------------------
1 |
2 | simplejson is no longer needed. client.py uses the python builtin json libs coming with version >=2.6
3 |
4 | Supernova API is at:
5 | http://supernova.astrometry.net/api
6 |
7 | Nova API is at:
8 | http://nova.astrometry.net/api
9 |
10 |
11 | Note on supernova:
12 | Since supernova is undergoing continuous development, consider your API
13 | key for it short lived and volatile.
14 |
15 | That said:
16 | If you find that the client is no longer able to connect to the
17 | (experimental) supernova API, please check that your API key hasn't
18 | changed by visiting http://supernova.astrometry.net/dashboard/profile/
19 |
--------------------------------------------------------------------------------
/blind/pquad.h:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | #ifndef PQUAD_H
7 | #define PQUAD_H
8 |
9 | /**
10 | This file is just required for testing purposes (of solver.c)
11 | */
12 |
13 | struct potential_quad
14 | {
15 | anbool scale_ok;
16 | int fieldA, fieldB;
17 | // distance-squared between A and B, in pixels^2.
18 | double scale;
19 | double costheta, sintheta;
20 | // (field pixel noise / quad scale in pixels)^2
21 | double rel_field_noise2;
22 | anbool* inbox;
23 | int ninbox;
24 | double* xy;
25 | };
26 | typedef struct potential_quad pquad;
27 |
28 | #endif
29 |
--------------------------------------------------------------------------------
/man/downsample-fits.1:
--------------------------------------------------------------------------------
1 | .TH DOWNSAMPLE-FITS "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | downsample-fits \- Scale down a FITS image
4 | .SH SYNOPSIS
5 | .B
6 | downsample-fits
7 | [options] \fIinput-file\fR \fIoutput-file\fR
8 | .SH DESCRIPTION
9 | Scale down a FITS image. Use "\-" to write to stdout.
10 | .SH OPTIONS
11 | .TP
12 | \fB\-s\fR \fIscale\fR
13 | Downsample scale (default: 2): integer
14 | .TP
15 | \fB\-e\fR \fIextension\fR
16 | Read extension (default: 0)
17 | .TP
18 | \fB\-v\fR
19 | Verbose
20 | .SH AUTHOR
21 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
22 | Dustin Lang (CMU).
23 | .SH SEE ALSO
24 | http://astrometry.net
25 |
--------------------------------------------------------------------------------
/util/makefile.libkd:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 |
4 | LIBKD_DIR := $(BASEDIR)/libkd
5 | LIBKD_LIB_FILE := $(LIBKD_DIR)/libkd.a
6 | LIBKD_NOIO_LIB_FILE := $(LIBKD_DIR)/libkd-noio.a
7 |
8 | LIBKD_INC :=
9 | LIBKD_SLIB := $(LIBKD_LIB_FILE)
10 | LIBKD_LIB :=
11 |
12 | # $(LIBKD_LIB_FILE):
13 | # $(MAKE) -C $(LIBKD_DIR) libkd.a
14 | #
15 | # $(LIBKD_NOIO_LIB_FILE):
16 | # $(MAKE) -C $(LIBKD_DIR) libkd-noio.a
17 |
18 | include $(COMMON)/makefile.anutils
19 |
20 | LIBKD_INC += $(ANUTILS_INC)
21 | LIBKD_CFLAGS += $(ANUTILS_CFLAGS)
22 | LIBKD_SLIB += $(ANUTILS_SLIB)
23 | LIBKD_LIB += $(ANUTILS_LIB)
24 |
--------------------------------------------------------------------------------
/man/an-pnmtofits.1:
--------------------------------------------------------------------------------
1 | .TH AN-PNMTOFITS "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | an\-pnmtofits \- Convert PNM file to FITS.
4 | .SH SYNOPSIS
5 | .B
6 | an\-pnmtofits
7 | [options] [\fIinput-file\fR [\fIoutput-file\fR]]
8 | .SH DESCRIPTION
9 | Convert a PNM file to a FITS file. If no input file is given, stdin is used.
10 | If no output file is given, stdout is used.
11 | .TP
12 | \fB\-o\fR \fIfile\fR
13 | Output file (default stdout)
14 | .TP
15 | \fB\-v\fR
16 | Verbose mode
17 | .TP
18 | \fB\-q\fR
19 | Quiet mode
20 | .SH AUTHOR
21 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
22 | Dustin Lang (CMU).
23 | .SH SEE ALSO
24 | http://astrometry.net
25 |
--------------------------------------------------------------------------------
/qfits-an/md5.h:
--------------------------------------------------------------------------------
1 | #ifndef MD5_H
2 | #define MD5_H
3 |
4 | typedef unsigned int word32;
5 |
6 | struct MD5Context {
7 | word32 buf[4];
8 | word32 bits[2];
9 | union {
10 | unsigned char in[64];
11 | word32 in32[16];
12 | };
13 | };
14 |
15 | void MD5Init(struct MD5Context *context);
16 | void MD5Update(struct MD5Context *context, unsigned char const *buf,
17 | unsigned len);
18 | void MD5Final(unsigned char digest[16], struct MD5Context *context);
19 | void MD5Transform(word32 buf[4], word32 const in[16]);
20 |
21 | /*
22 | * This is needed to make RSAREF happy on some MS-DOS compilers.
23 | */
24 | typedef struct MD5Context MD5_CTX;
25 |
26 | #endif
27 |
--------------------------------------------------------------------------------
/gsl-an/gsl/gsl_block.h:
--------------------------------------------------------------------------------
1 | #ifndef __GSL_BLOCK_H__
2 | #define __GSL_BLOCK_H__
3 |
4 | #include
5 | #include
6 | #include
7 |
8 | #include
9 | #include
10 | #include
11 |
12 | #include
13 | #include
14 |
15 | #include
16 | #include
17 |
18 | #include
19 | #include
20 |
21 | #include
22 | #include
23 |
24 | #endif /* __GSL_BLOCK_H__ */
25 |
--------------------------------------------------------------------------------
/sdss/setup.py:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 | from distutils.core import setup, Extension
4 | import os
5 | import sys
6 |
7 | sys.path.append(os.path.join(os.path.dirname(os.path.dirname(os.path.abspath(__file__))), 'util'))
8 | from an_build_ext import an_build_ext
9 |
10 | setup(cmdclass={'build_ext': an_build_ext},
11 | name='C utils for Astrometry.net SDSS routines',
12 | version = '1.0',
13 | author = 'Lang & Hogg',
14 | author_email = 'dstndstn@gmail.com',
15 | url = 'http://astrometry.net',
16 | ext_modules = [Extension('_cutils', ['cutils.i'], libraries=['m'])],
17 | )
18 |
--------------------------------------------------------------------------------
/man/fits-flip-endian.1:
--------------------------------------------------------------------------------
1 | .TH FITS-FLIP-ENDIAN "1" "July 2015" "0.56" "astrometry.net"
2 | .SH NAME
3 | fits-flip-endian \- Endian swapping of FITS binary tables.
4 | .SH SYNOPSIS
5 | .B
6 | fits\-flip\-endian
7 | \fB\-i\fR \fIinput-file\fR
8 | \fB\-o\fR \fIoutput-file\fR
9 | [ \fB\-e\fR \fIext\fR \fB\-s\fR \fIsize\fR ] ...
10 | .SH OPTIONS
11 | .TP
12 | \fB\-i\fR \fIfile\fR
13 | Input file
14 | .TP
15 | \fB\-o\fR \fIfile\fR
16 | Output file
17 | .TP
18 | \fB\-e\fR \fIext\fR
19 | Extension number
20 | .TP
21 | \fB\-s\fR \fIsize\fR
22 | Data size in bytes
23 | .SH AUTHOR
24 | The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
25 | Dustin Lang (CMU).
26 | .SH SEE ALSO
27 | http://astrometry.net
28 |
--------------------------------------------------------------------------------
/include/astrometry/bl-nl.inc:
--------------------------------------------------------------------------------
1 | /*
2 | # This file is part of the Astrometry.net suite.
3 | # Licensed under a 3-clause BSD style license - see LICENSE
4 | */
5 |
6 | #include "astrometry/bl-nl.ph"
7 |
8 | InlineDefine
9 | number NLF(get)(nl* list, size_t n) {
10 | number* ptr = (number*)bl_access(list, n);
11 | return *ptr;
12 | }
13 |
14 | InlineDefine
15 | number NLF(get_const)(const nl* list, size_t n) {
16 | number* ptr = (number*)bl_access_const(list, n);
17 | return *ptr;
18 | }
19 |
20 | InlineDefine
21 | size_t NLF(size)(const nl* list) {
22 | return bl_size(list);
23 | }
24 |
25 | InlineDefine
26 | number* NLF(access)(nl* list, size_t j) {
27 | return (number*)bl_access(list, j);
28 | }
29 |
30 |
--------------------------------------------------------------------------------
/catalogs/openngc-names-csv.awk:
--------------------------------------------------------------------------------
1 | # This file is part of the Astrometry.net suite.
2 | # Licensed under a 3-clause BSD style license - see LICENSE
3 |
4 | function printName(name) {
5 | print isngc ";" id ";" name;
6 | }
7 |
8 | # Skip header line.
9 | NR==1 { next }
10 |
11 | {
12 | if ($1 !~ /^(IC|NGC)[0-9]*$/) next;
13 |
14 | # Is it part of NGC or IC?
15 | isngc = ($1 ~ /^NGC/);
16 |
17 | # ID number.
18 | id = $1;
19 | gsub(/[A-Z]/, "", id);
20 | id = int(id);
21 |
22 | # Common names (comma separated).
23 | split($24, names, ",");
24 | for (i in names) {
25 | printName(names[i]);
26 | }
27 |
28 | # Add Messier number as a common name.
29 | if ($19 != "") {
30 | printName("M " int($19));
31 | }
32 | }
33 |
--------------------------------------------------------------------------------
/gsl-an/gsl/gsl_matrix.h:
--------------------------------------------------------------------------------
1 | #ifndef __GSL_MATRIX_H__
2 | #define __GSL_MATRIX_H__
3 |
4 | #include
5 | #include
6 | #include
7 |
8 | #include
9 | #include
10 | #include
11 |
12 | #include
13 | #include
14 |
15 | #include
16 | #include
17 |
18 | #include
19 | #include
20 |
21 | #include
22 | #include