PIMMS v4.8b now available
The new Japanese observatory is recognized as Hitomi starting with
Version 4.8b; the support for IXO project has been discontinued.
Version 4.8a contains a minor update of Chandra effective area curve files,
suitable for use for Cycle 18 proposals. If you already have version 4.8
installed, you can simply download
and unpack its content on the data subdirectory of your PIMMS
installation - the existing executable will automatically pick up the new
Version 4.8 contains a revised pile-up formula for XMM-Newton EPIC
instruments; it also contains an updated EPIC effective area curves
and updated ASTRO-H HXI effective area curves.
If you would like to be informed whenever
a new version of PIMMS is released, please contact
PIMMS - Portable, Interactive Multi-Mission Simulator
Command-line tool and the Web interface
PIMMS was originally written as a stand-alone,
interactive program (the "command line PIMMS").
implements a subset of the functionalities of the command line
PIMMS. While allowing easy access, without the need to
install the software, it does not have all the functionality
of the command line version.
PIMMS, as described here, is software for high-energy
astrophysicists, and has nothing to do with
the Project to Increase Mastery of Mathematics and Science.
The program was named quite independently of this
worthwhile project at Wesleyan University.
Time-Variable Instrumental Response
PIMMS currently does not support time-variable calibration
of instruments. Because it is primarily intended as a planning tool
for future observations, the responses in PIMMS is often
applicable for upcoming observations.
For example, if you are a Chandra user who wishes
to convert count rates in a past observation to flux, please see
PIMMS is currently supported on several flavors of UNIX
workstations, on Linux PCs, Macs running OS X/Darwin.
It requires a Fortran compiler, and make on UNIX machines.
Please consult the Installation Guide
for details, then
the latest version.
New in Version 3.8/3.8a/3.8a2 (Released 2006 May 1 - 2006 May 24)
New in Version 3.7/3.7a (Released 2005 Sep 13 - 2005 Dec 23)
New in Version 3.6/3.6a/3.6b/3.6c5 (Released 2004 Sep 15 - 2005 Feb 10).
New in Version 3.5 (Released 2004 Jul 9).
New in Version 3.4/3.4a (Released 2003 Sep - 2004 Jan 12).
New in Version 3.3/3.3a (Released 2002 Dec 16 - 2003 Mar 27).
New in version 3.2-3.2d (Released 2001 Sep 10 - 2002 Jan 29).
New in version 3.1 a-c (Released 2001 January 29 - May 03).
New in version 3.0 (Released 2000 April 28).
New in version 2.7 (Released 1999 July 9).
New in version 2.6 a-c (Released 1999 February 2 - May 4).
New in version 2.5 (Released 1997 December 15).
New in version 2.4/2.4b
(Released 1996 June 03).
New in version 2.3 (Released 1996 June 03).
New in version 2.2 (Released 1995 August 07).
New in version s2.1a (Released 1995 April 03).
- New in Version 4.8/4.8a/4.8b (Released 2015 Aug 17/Dec 16/2016 Feb 29)
- The former ASTRO-H mission is now recognized as Hitomi,
starting with Version 4.8b. The support for the IXO project has
- Version 4.8a contains a minor update of Chandra effective area curves,
suitable for use for Cycle 18 proposals.
- The pile-up formulae for the XMM-Newton EPIC instruments have been revised
using the latest information from the instrument teams. This brings PIMMS
in line with tools used at the XMM SOC.
- Version 4.7 contains new XMM-Newton EPIC effective area curves suyitable
for AO-15 proposal preparation, although any differences with the previous
version is exteremely minor.
- Version 4.7 also contains new ASTRO-H HXI effective area curves.
- New in Version 4.7/4.7a/4.7b/4.7c/4.7d (Released 2014 Mar 5/Jul 24/Aug 20/Dec 22/Dec 23)
- New in Version 4.6/4.6a/4.6b (Released May 25/Sep 28/2013 Jan 25)
- New in Version 4.5 (Released 2012 Jan 30)
- New in Version 4.4 (Released 2011 Sep 19)
- New in Version 4.3 (Released 2011 Feb 15)
- New in Version 4.2/4.21 (Released 2010 Dec 20/Oct 27)
- New in Version 4.1/4.1a/4.1b (Released 2010 Jun 1 - Sep 21)
- New in Version 4.0 (Released 2010 Feb 17)
- New in Version 3.9 through 3.9k (Released 2006 Sep 6 - 2009 Oct 6)
- Sample Sessions
- Using Multi-component Models
- Extended Sources
- The User Interface
- PIMMS commands
version of the Guide.
Adding new missions and other future plans
At a very basic level, new missions can be added simply by
creating a set of effective area curve files: they need to
be two-column ASCII files, containing pairs of photon energy
in keV and effective area in cm2.
PIMMS source code and data files are distributed
freely, without restrictions. If you decide to add new
missions to PIMMS, we would like to be able to distribute
it from HEASARC.
We hope to have a programmers' guide some day to make it easier
to add mission-specific information.
Credits and Feedback
PIMMS is mostly written and maintained by Koji Mukai.
Effective area curves for current and future missions have been supplied
by the respective projects. XTE specific subroutines have been written
by Koji Mukai, with the help of Jim Lochner and Phil Blanco. The SAX
specific subroutine has been written by the SAX Data Center and
Lorella Angelini. Snowden R-band effective area curves for ROSAT
PSPC have been created by Richard West of Leicester.
The only published article on PIMMS is in the HEASARC journal:
Mukai, K. 1993, Legacy 3, 21-31.
Questions and comments on PIMMS can be sent to
HEASARC Home |
This file was last modified on Monday, 29-Feb-2016 12:03:05 EST