Astronomical Software

AIPS

​AIPS, the NRAO Astronomical Image Processing System is used primarily for reducing data from synthesis radio telescopes. General information is given in the ​AIPS FAQ. We currently have version 31DEC06 installed.

CIAO

​CIAO, is a data analysis system written for the needs of users of the Chandra X-ray Observatory. Because Chandra is the first mission with 4-dimensional data (2 spatial, time, energy) in which each dimension has many independent elements, CIAO was built to handle N-dimensional data without concern about which particular axes were being analyzed. Also, apart from a few Chandra instrument tools, CIAO is mission independent.

IRAF

​IRAF is a heterogeneous collection of routines and packages for all sorts of tasks, but it is first of all a data reduction environment, for which there is extensive ​on-line documentation.

PYRAF

​PyRAF is a new command language for IRAF based on the Python scripting language. It is useful both for interactive data analysis and for writing analysis scripts. PyRAF coexists with the current IRAF CL. We currently have version v1.2.1 installed, which includes a number new PyRAF packages for the HST instruments e.g. ​Pydrizzle and ​Multidrizzle.

FFTW

​FFTW is a C subroutine library for computing the discrete Fourier transform (DFT) in one or more dimensions, of arbitrary input size, and of both real and complex data (as well as of even/odd data, i.e. the discrete cosine/sine transforms or DCT/DST). The FFTW package was developed at MIT by Matteo Frigo and Steven G. Johnson. Our workstation have version 3 installed.

GNU scientific library

GNU Scientific Library (GSL)

HEASOFT

​HEASOFT is a unified release of the FTOOLS and XANADU Software Packages

XANADU High-level, multi-mission tasks for X-ray astronomical spectral, timing, and imaging data analysis FTOOLS General and mission-specific tools to manipulate FITS files FITSIO Core library responsible for reading and writing FITS files (distributed with FTOOLS) fv General FITS file browser/editor/plotter with a graphical user interface (distributed with FTOOLS) XSTAR Tool for calculating the physical conditions and emission spectra of photoionized gases. The current version of HEAsoft is 6.0.4 (November 28 2005)

IDL

​IDL, the Interactive Data Language, or IDL, is a product of Research Systems Inc (RSI). It is a package designed to reduce, analyse and display scientific data and images. IDL can be used for tasks such as: Line drawing and fitting, contour and surface plotting, animation. Matrix operations, solving nonlinear equations, ffts etc. Writing functions and procedures. and much more. More extensive information is given in the IDL FAQ. We currently have IDL 6.2 installed.

TeXtoIDL

​TeXtoIDL: The purpose of the TeXtoIDL routines is to make it simple to use Greek letters, subscripts and superscripts in making labels for plots in IDL. This is accomplished by allowing the user to use TeX control sequences for Greek letters and special symbols and for sub/superscripts. The TeX control sequences are simple and easy to remember, especially if you already use TeX for writing papers (for those unfamiliar with TeX, an explanation of that notation is below). The translation is done for either vector or PostScript fonts.

IDLWAVE

​IDLWAVE: This package has been installed as part of Emacs to enable it to understand IDL syntax, which is very useful when writing IDL scripts. IDLWAVE also enables running an IDL shell within emacs - type:

M-X idlwave-shell

which runs your settup defined by the environment variable IDL_STARTUP.

KARMA

​KARMA is a toolkit for interprocess communications, authentication, encryption, graphics display, user interface and manipulating the Karma network data structure. It contains KarmaLib (the structured libraries and API) and a large number of modules (applications) to perform many standard tasks. A suite of visualisation tools are distributed with the library.

LApack

​LAPACK is written in Fortran77 and provides routines for solving systems of simultaneous linear equations, least-squares solutions of linear systems of equations, eigenvalue problems, and singular value problems. The associated matrix factorizations (LU, Cholesky, QR, SVD, Schur, generalized Schur) are also provided, as are related computations such as reordering of the Schur factorizations and estimating condition numbers. Dense and banded matrices are handled, but not general sparse matrices. In all areas, similar functionality is provided for real and complex matrices, in both single and double precision.

MIRIAD

​MIRIAD is radio interferometry data reduction package. It has particular emphasis on aspects of interest to users of the Australia Telescope Compact Array (ATCA). Miriad can be used for the reduction of continuum and spectral line experiments. Miriad, in particular, supports a number of niche areas. These include calibration and analysis of polarimetric data from the ATCA, multi-frequency synthesis imaging, mosaicing, ATCA pulsar bin mode, and some spectral line observing applications (e.g. Zeeman experiments).

PHYSICA

​PHYSICA is a high level, interactive programming environment with user friendly graphics and sophisticated mathematical analysis capabilities. Version 2.77

SAS

​SAS is the XMM-Newton Science Analysis System. We currently have version 6.5.0 installed.

STSDAS

​STSDAS is the software for reducing and analyzing data from the Hubble Space Telescope. It is layered on top of IRAF and provides general purpose tools for astronomical data analysis as well as routines specifically designed for HST analysis. We currently have version 3.4 installed.

SCILAB

​Scilab is a scientific software package for numerical computations providing a powerful open computing environment for engineering and scientific applications. Scilab includes hundreds of mathematical functions with the possibility to add interactively programs from various languages (C, Fortran...). It has sophisticated data structures (including lists, polynomials, rational functions, linear systems...), an interpreter and a high level programming language.

Spitzer tools

​Spitzer telescope observation preparation tool (SPOT). SPOT is the observation preparation tool for the Spitzer telescope. Leopard is the software package used to download data. A ​SPOT User Guide and ​Leopard User Guide are available. We currently have version Spitzer-pride13_0_3 installed.

TEMPO

​Tempo is a program for the analysis of pulsar timing data. Pulsar rotation, astrometric, and binary parameters are deduced by fitting models to pulse times of arrival measured at one or more terrestrial observatories. Tempo is maintained and distributed by Princeton University and the Australia Telescope National Facility. The code is freely available, and others are encouraged to extend, modify, and improve it as they see fit.

Image Display Programs

ds9

SAOImage ​DS9 is an astronomical imaging and data visualization application. DS9 supports FITS images and binary tables, multiple frame buffers, region manipulation, and many scale algorithms and colormaps. It provides for easy communication with external analysis tasks and is highly configurable and extensible. The currently installed version is 4.0b8.

PGPLOT

​PGPLOT is a large subroutine library for plotting scientific data. The PGPLOT Graphics Subroutine Library is a Fortran- or C-callable, device-independent graphics package for making simple scientific graphs. It is intended for making graphical images of publication quality with minimum effort on the part of the user. For most applications, the program can be device-independent, and the output can be directed to the appropriate device at run time.

Language Compilers

perl

PerlDL

awk

gcc

c++

g77 (fortran)

cvs

python

tcl/tk

g95

gfortran

R