source: trunk/README @ 151

Last change on this file since 151 was 146, checked in by Matthew Whiting, 18 years ago

A few new things:

  • Made a mycpgplot.hh file, to keep PGPlot-related constants (enum types)

in a standard namespace (so one can do cpgsci(RED) rather than cpgsci(2)...).
Incorporated this into all code that uses pgplot.

  • Improved the outputting of the number of detected objects in the search

functions. Now shows how many have been detected, before they are merged
into the list.

  • Fixed a bug in columns.cc that was incorrectly updating the precision for

negative velocities.

  • Additional text in the Guide, and general clean up of code.
File size: 4.6 KB
Line 
1-----------------------------------------------------------------------
2               The Duchamp Source Finder
3-----------------------------------------------------------------------
4Duchamp 1.0 -- an object finder for spectral-line data cubes
5Copyright (C) 2006, Matthew Whiting, ATNF
6
7Duchamp is free software; you can redistribute it and/or modify it
8under the terms of the GNU General Public License as published by the
9Free Software Foundation; either version 2 of the License, or (at your
10option) any later version.
11
12Duchamp is distributed in the hope that it will be useful, but WITHOUT
13ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
14FITNESS FOR A PARTICULAR PURPOSE.  See the GNU General Public License
15for more details.
16
17You should have received a copy of the GNU General Public License
18along with Duchamp; if not, write to the Free Software Foundation,
19Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307, USA
20
21Correspondence concerning Duchamp may be directed to:
22   Internet email: matthew.whiting@atnf.csiro.au
23   Postal address: Dr. Matthew Whiting
24                   Australia Telescope National Facility, CSIRO
25                   PO Box 76
26                   Epping NSW 1710
27                   AUSTRALIA
28-----------------------------------------------------------------------
29
30Introduction
31------------
32
33Duchamp is a stand-alone program designed to find objects in
34astronomical data cubes, particularly spectral-line observations. Its
35features include a wavelet-based reconstruction technique for reducing
36the noise in the cube (and thereby enhancing detectability of
37sources), easy-to-use text-based interface, flexibility to control all
38relevant parameters such as detection thresholds, and a useful range
39of text- and graphics-based output.
40
41Duchamp works on any FITS image using the CFITSIO package, and uses
42Mark Calabretta's WCSLIB library to provide accurate position and
43velocity information for all detected sources.
44
45
46Obtaining and Building Duchamp
47------------------------------
48
49The Duchamp web page is at
50http://www.atnf.csiro.au/people/Matthew.Whiting/Duchamp
51where you can download a gzipped tar archive of the source code.
52
53Duchamp uses three main external libraries: pgplot, cfitsio and
54wcslib. If you do not have the libraries, they can be downloaded from
55the following locations:
56PGPlot -- http://www.astro.caltech.edu/~tjp/pgplot/
57cfitsio -- http://heasarc.gsfc.nasa.gov/docs/software/fitsio/fitsio.html
58wcslib -- http://www.atnf.csiro.au/people/Mark.Calabretta/WCS/index.html
59
60Duchamp can be built on Unix systems by typing:
61 >  ./configure
62 >  make
63 >  make clean (optional -- to remove the object files from the src
64                directory)
65
66This way, configure should find all the necessary libraries, but if
67the above-mentioned libraries have been installed in non-standard
68locations, you can specify additional directories to look in. There
69are separate options for library files (eg. libcpgplot.a) and header
70files (eg. cpgplot.h).
71
72For example, if wcslib had been installed in /home/mduchamp/wcslib,
73there are two libraries that are likely to be in separate
74subdirectories: C/ and pgsbox/. Each subdirectory needs to be searched
75for library and header files, so one could build Duchamp by typing:
76 >  ./configure LIBDIRS="/home/mduchamp/wcslib/C
77/home/mduchamp/wcslib/pgsbox" INCDIRS="/home/mduchamp/wcslib/C
78/home/mduchamp/wcslib/pgsbox"
79And then just run make in the usual fashion:
80 >  make
81
82
83Using Duchamp
84---------------
85
86There are two possible ways to run Duchamp. The first is:
87
88 >  Duchamp -f image.fits
89
90where image.fits is the data cube to be searched. This method simply
91uses the default values of all parameters.
92
93The second method allows some determination of the parameter values by
94the user. Type:
95
96 >  Duchamp -p parameterFile
97
98where parameterFile is a file with the input parameters, including the
99name of the cube you want to search. There are two example input files
100included with the distribution. The smaller one, InputExample, shows
101the typical parameters one might want to set. The large one,
102InputComplete, lists all possible parameters that can be entered, and
103a brief description of them. To get going quickly, just replace the
104"your-file-here" in InputExample with your image name, and type
105
106 >  Duchamp -p InputExample
107
108A User's Guide in the docs/ directory provides complete
109documentation. It comes in both postscript and portable document
110format (pdf -- note that this contains hyperlinks). This guide will
111provide full descriptions of all parameters, and of all steps in the
112execution of Duchamp.
113
114Any questions, please contact me!
115
116Author:
117  Matthew Whiting, Australia Telescope National Facility, June 2006
118  Matthew.Whiting@csiro.au
119
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