QUESTION AND ANSWERAn Interrogative Introduction to HEAsoft 5.3.1Q1: What is HEASOFT? A1: HEASOFT is a software suite consisting of the union of FTOOLS/FV, XIMAGE, XRONOS, XSPEC and XSTAR. Q2: What is XANADU? A2: The packages XIMAGE, XRONOS and XSPEC were originally distributed together as the XANADU package. Over the years, while the three continued to complement each others' function, they ceased to be fully integrated, and were distributed separately. As of the release of HEASOFT 5.0, the three packages are once again fully integrated. XANADU is the union of XIMAGE, XRONOS, and XSPEC. XANADU is thus a subset of HEASOFT. Q3: What is FTOOLS / FV? A3: FTOOLS / FV is a suite of several hundred tools, each of which has a fairly specific, narrow function for the analysis of FITS format files. Some of these tools are specific to particular missions, like ASCA, ROSAT and XTE. Other tools are more general, or support specific mission-independent functions, such as accessing the LHEA Calibration Database (CALDB). FV is a GUI-based tool for examining and manipulating FITS format files. Q4: What is XSTAR? A4: XSTAR is a command-driven computer program for calculating the physical conditions and emission spectra of photoionized gases. The XSTAR package was originally distributed separately, but is now fully integrated into the HEASOFT framework. Q5: Is there a binary distribution available for my machine? A5: There are binary distributions available for SUN/Solaris, Intel/Linux, Macintosh OS X/Darwin, DEC/OSF, Macintosh/LinuxPPC, SGI/IRIX, and x86/Cygwin. These include binaries for all the subsets of HEASOFT. Q6: Why should I build my own copy of HEASOFT, if pre-built binaries are available for my machine? A6: There are several reasons to build the software instead of installing pre-built binaries. First, binaries generally run better on the system where they were built. Second, the source code is considerably smaller, hence easier to download. Third, the pre-built binaries are statically linked, which typically makes them much larger. Q7: How is the HEASOFT source code packaged? A7: For convenience, the HEASOFT source code is bundled in the following gzipped tarfiles: lheasoft5.3.1src.tar.gz -- HEASOFT 5.3.1 complete (see question 1 above for detailed list of contents) ftools5.3.1src.tar.gz -- FTOOLS 5.3.1 / FV 4.1.2 only xanadu5.3.1src.tar.gz -- XANADU 5.3.1 only (see question 2 above for detailed list of contents) xstar2.1ksrc.tar.gz -- XSTAR 2.1k only Q8: What is the gzipped tarfile xspec11.3.1data.tar.gz, and why and when is it needed? A8: This file contains the XSPEC data files, which are required for XSPEC to run. These data files are excluded from lheasoft5.3.1src.tar.gz and xanadu5.3.1src.tar.gz for a purely practical reason: the data files would add about 230 MB to the size of these files! This file is needed if and only if XSPEC is installed. Q9: Is it possible to build just parts of FTOOLS, or parts of XANADU? A9: Yes. Although the source code is only available in the groups described above, it is possible to build just a portion of the source code, for example, just the XTE FTOOLS, or just XIMAGE. Q10: What if I want to install FTOOLS / FV separately from some other package(s), like XSPEC? A10: Nothing prevents installing two disjoint gzipped tarfiles, like ftools5.3.1src.tar.gz and xanadu5.3.1src.tar.gz, in two separate areas. After installation, either one or both of these areas may be used by running the standard initialization described below for each package in sequence. HEASoft / FTOOLS Help Desk If FTOOLS has been useful in your research, please reference this site (https://heasarc.gsfc.nasa.gov/ftools) and use the ASCL reference for HEASoft [ascl:1408.004] or the ASCL reference for the original FTOOLs paper [ascl:9912.002]: Blackburn, J. K. 1995, in ASP Conf. Ser., Vol. 77, Astronomical Data Analysis Software and Systems IV, ed. R. A. Shaw, H. E. Payne, and J. J. E. Hayes (San Francisco: ASP), 367. Web page maintained by: Bryan K. Irby HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public Last modified: Thursday, 20-May-2004 15:33:54 EDT |