Changes between Version 39 and Version 40 of Astronomical Tools/Software
- Timestamp:
- 04/03/06 12:52:15 (20 years ago)
Legend:
- Unmodified
- Added
- Removed
- Modified
-
Astronomical Tools/Software
v39 v40 25 25 packages for the HST instruments e.g. [http://stsdas.stsci.edu/pydrizzle/ Pydrizzle] and [http://stsdas.stsci.edu/multidrizzle/ Multidrizzle]. 26 26 27 28 27 == FFTW == 29 28 [http://www.fftw.org/ 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). 30 29 The FFTW package was developed at MIT by Matteo Frigo and Steven G. Johnson. 31 30 Our workstation have version 3 installed. 31 32 == GNU scientific library == 33 GNU Scientific Library (GSL) 32 34 33 35 == HEASOFT == … … 75 77 [http://www.atnf.csiro.au/computing/software/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. 76 78 79 == LApack == 80 81 [http://www.netlib.org/lapack/index.html 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. 82 77 83 == MIRIAD == 78 84 [http://www.atnf.csiro.au/computing/software/miriad/ MIRIAD] is radio interferometry data reduction package. … … 82 88 synthesis imaging, mosaicing, ATCA pulsar bin mode, and some spectral line observing applications (e.g. Zeeman experiments). 83 89 90 == PHYSICA == 91 92 [http://www.triumf.ca/compserv.html PHYSICA] is a high level, interactive programming environment with user friendly graphics and sophisticated mathematical analysis capabilities. 93 Version 2.77 94 95 84 96 == SAS == 85 97 [http://xmm.vilspa.esa.es/sas/new/ SAS] is the XMM-Newton Science Analysis System. … … 93 105 We currently have version 3.4 installed. 94 106 95 == TEMPO ==96 [http://pulsar.princeton.edu/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.97 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.98 99 107 == SCILAB == 100 108 [http://www.scilab.org/ Scilab] is a scientific software package for numerical computations … … 105 113 interpreter and a high level programming language. 106 114 107 * [wiki:XSPEC]108 115 == Spitzer tools == 109 116 [http://ssc.spitzer.caltech.edu/propkit/spot/ Spitzer telescope observation preparation tool (SPOT)]. … … 113 120 We currently have version Spitzer-pride13_0_3 installed. 114 121 115 * [wiki:"GNU scientific library"] 116 * [wiki:physica] 117 122 == TEMPO == 123 [http://pulsar.princeton.edu/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. 124 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. 118 125 119 126 == Image Display Programs == … … 131 138 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. 132 139 133 === ximtool ===134 135 136 140 === ImageMagick === 137 141 138 ImageMagick®, is a free software suite to create, edit, and compose bitmap images. It can read, convert and write images in a large variety of formats. Images can be cropped, colors can be changed, various effects can be applied, images can be rotated and combined, and text, lines, polygons, ellipses and Bézier curves can be added to images and stretched and rotated.142 [http://www.imagemagick.org/script/index.php ImageMagick®], is a free software suite to create, edit, and compose bitmap images. It can read, convert and write images in a large variety of formats. Images can be cropped, colors can be changed, various effects can be applied, images can be rotated and combined, and text, lines, polygons, ellipses and Bézier curves can be added to images and stretched and rotated. 139 143 version 140 144 141 * [wiki:LApack]142 143 144 145 = Display/documents = 145 * LaTex (and all related packages, e.g., pdflatex, ps2pdf??, etc) 146 147 == LaTeX == 146 148 147 149 == Supermongo (sm) == … … 180 182 181 183 == EDITORS == 184 182 185 === emacs === 183 186 To start Emacs,
