skip to content
 
ASCA Guest Observer Facility


FTOOLS V3.6 RELEASED


We are pleased to announce the release of FTOOLS v3.6. In this message, we summarize:

  1. How to obtain FTOOLS v3.6
  2. Impact on ASCA users
    • 2a. Differences between v3.5.2 and v3.6
    • 2b. Differences between v3.5 and v3.6
  3. Known bugs/deficiencies of FTOOLS v3.6

1. How to obtain FTOOLS v3.6


FTOOLS v3.6 has been released, and can be obtained from the FTOOLS web-page at:

http://heasarc.gsfc.nasa.gov/docs/software/ftools/ftools_menu.html

Notices of the FTOOLS Releases, online HTML versions of FTOOLS documentation (like this document), the official FAQ, and other goodies are available on the World Wide Web at:

http://heasarc.gsfc.nasa.gov/docs/software/ftools/ftools_menu.html

This is where the most up to date FTOOLS information is available, including the continually updated FAQ. Users should always check here first for answers to questions.

Any problems installing FTOOLS should be reported to:

Feedback form.

Any problems using FTOOLS for ASCA data analysis should be reported to the ftoolshelp address above or to:

Feedback form.

If the problem relates to the scientific contents of the FTOOLS, the latter address is more appropriate.


2. Impact on ASCA users


There are relatively few changes in the contents of ASCA FTOOLS since ASCA patch 3.5.2; changes since the original v3.5 release are quite substantial. These are listed separately below.


2a. New since v3.5.2

  • We now support stand-alone FTOOLS under Linux, and IRAF version of FTOOLS under Solaris.

  • We have dramatically improved our testing of FTOOLS on different architectures; previous releases were extensively tested only under Alpha/OSF and Sun/SunOS. With increased testing under Sun/Solaris, SGI and other types of machines, we have flushed out many architecture or compiler dependent bugs (e.g., non-standard extensions supported on most, but not all, machines). Consequently, we believe this version of FTOOLS are far more robust, particularly on Solaris machines.

Changes to individual software:

  • We have been notified of an error in the treatment of area discrimination for SIS Fast mode data ('select fast inside' 'select fast outside' commands). We have fixed this problem in xselect.

  • We have fixed a bug in extractor which resulted in incorrect wmaps when the extraction region was specified in sky coordinates. However, see

    http://heasarc.gsfc.nasa.gov/docs/asca/soft_skycoord.html for the limitations of the current algorithm.

  • Sisrmg has been converted to use native C version of fitsio.

  • Ghkcurve has been updated to treat combined medium and high bit rate data correctly.

2b. Changes since original v3.5 release

ascaarf    - uses new XRT calibration files (xrt_ea_v2_0.fits,
             xrt_psf_v2_0.fits) and new "filter" modification
             to the effective area curve that provides power-law
             fit to GIS Crab spectra consistent with Toor & Seward
             (1979; AJ 79, 995). This filter can be switched off using
             the 'filter=no' option. All calibration files can be read
             from either the CALDB or the refdata area. The default is
             the AUTO setting which first checks for CALDB files and if
             they are not found then looks in the refdata area. If CALDB
             is given as the value of the input RMF parameter then ascaarf
             checks the CALDB for an appropriate RMF to use to set the
             energies on which the ARF is calculated.

             Note that the "filter" modification is applied to both GIS
             and SIS data however it has only been calibrated against the
             GIS Crab data.

ascaeffmap - uses new XRT calibration files and AUTO argument for all calibration files.

ascalin - now can redetermine GIS/SIS PI values using manually input new gain and/or offset numbers. To use this option, use the 'gain fit' command in XSPEC and use the resultant gain and offset numbers on the command line (gainnorm=0.98, gainoff=0.03 etc.) Note, however, the parameter file will remember the values supplied; it is recommended to reset these to 1.0 and 0.0 respectively, after use. Please note that this update is to enable manual adjustment of the gain, specifically to allow for the GIS gain mis-correction announced recently (see GIS team memo Apr 12, 1996). The update corresponding to the July 10th announcement by the GIS team will be available in a future release.

fastwmap - bug fix of the FTOOLS v3.5 release version (this fix was made available shortly after the v3.5 release)

ldeadtime - carry out deadtime correction for GIS light curves

sisrmg - several user interface bugs have been fixed. It should now default to grade 0234 for BRIGHT/BRIGHT2 mode data, unless the 'grades' hidden parameter is used to override the default. For fast mode data, it is recommended that you specify the grade explicitly (normally grades=0) on the command line; without this line, sisrmg will still crash on Alpha/OSF machines for fast mode data (this version does run on Alpha/OSF machines, provided that you supply the grades=0 option on the command line). However, this is believed to be the last (minor) remaining user-interface bug.


3. Known bugs and defficiencies of FTOOLS v3.6


  • The current scheme used for spectral extractions in sky coordinates has limitations. See http://heasarc.gsfc.nasa.gov/docs/asca/soft_skycoord.html for details.

  • When running on PI spectral files, sisrmg does not treat the event threshold/lower level discrimination correctly (PHA vs PI inconsistency). This may result in slight inaccuracy for the lowest channels.

  • The formula to correct for the GIS-3 gain problem (apparently caused by a change in the gain map, as detailed in the 1996 July 10th announcement by the GIS team) is not yet available in ascalin.

  • The current version of SISPI does not record the nominal gain value. For the usual case of 3.65 eV per channel, the FITS header will have:

    GAIN_NOM= 0.00365000 / Nominal gain value (ev/channel) for PI column

  • The standard region selection (to exclude the calibration source) for GIS 64x64 spatial resolution mode fails. However, a point source near the center can be extracted without problems.

This file was last modified on Wednesday, 07-Apr-2004 11:02:48 EDT
Curator: Michael Arida (SP Sys); arida@milkyway.gsfc.nasa.gov
HEASARC Guest Observer Facility
If you have any questions concerning ASCA, visit our Feedback form.

This file was last modified on Wednesday, 07-Apr-2004 11:02:48 EDT

NASA Astrophysics

  • FAQ/Comments/Feedback
  • Education Resources
  • Download Adobe Acrobat
  • A service of the Astrophysics Science Division (ASD) at NASA/ GSFC

    ASCA Project Scientist: Dr. Nicholas E. White

    Responsible NASA Official: Phil Newman

    Privacy Policy and Important Notices.