HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.

ROSAT Guest Observer Facility

A Quick Example of using PIMMS for ROSAT HRI count rate estimations


pimms

*** PIMMS Version 1.2 (1993 May 26 release) ***
    Reading mission directory, please wait
*   PIMMS simulation product is COUNT
    count rates for various instruments or intrinsic fluxes can be estimated
    Use 'PRODUCT' to simulate images
*   Current model is BREMSSTRAHLUNG, kT=  10.0000 keV; NH =  1.000E+21
    Use 'MODEL' command to change
*   By default, input rate is taken to be
    Flux (  2.000- 10.000 keV) in ergs/cm/cm/s
    Use 'FROM' command to change the default
*   Simulation product will be
    Count rate in ASCA SIS
    Use 'INSTRUMENT' command to switch to another instrument

PIMMS > instrument rosat hri

PIMMS > model

PIMMS knows about the following
     Blackbody (BB)
     Powerlaw (PL)
     (Thermal) Bremsstrahlung (TB)
     RaymondSmith (RS)
For the above, enter name, temperature/slope and Nh
                 e.g., model bb 2.4 2e21
PIMMS also knows about following precalculated models:
  Name          Short explanation
  RSQ60         Raymond-Smith, logT=6.0 (kT=0.086 keV), abundance 0.25 Solar
  RSQ62         Raymond-Smith, logT=6.2 (kT=0.137 keV), abundance 0.25 Solar
[Many others follow]
  For these, type MODEL  []
PIMMS can also use any Ascii files containing:
        energy (kev), flux (photons/cm/cm/s) pairs as model
  For this, type  []

Enter model name > PL

Enter photon index > 2

Enter Nh > 3E20

PIMMS > go 2E-11

* For power law model with photon index = 2.0000; NH =  3.000E+20
   and a flux (  2.000- 10.000keV) of  2.000E-11 ergs/cm/cm/s
  (Model normalization =  7.779E-03)
* PIMMS predicts  6.618E-01 cps with ROSAT HRI

[or, to estimate rosat counts based on another mission]

PIMMS > from einstein hri

PIMMS > go 1

* For power law model with photon index = 2.0000; NH =  3.000E+20
  and  1.000E+00 cps in EINSTEIN HRI
  (Model normalization =  2.282E-02)
* PIMMS predicts  1.941E+00 cps with ROSAT HRI

[or change the assumed input flux energy range]

PIMMS > from flux erg 0.1-2

PIMMS > go 1e-11

* For power law model with photon index = 2.0000; NH =  3.000E+20
   and a flux (  0.100-  2.000keV) of  1.000E-11 ergs/cm/cm/s
  (Model normalization =  3.708E-03)
* PIMMS predicts  3.155E-01 cps with ROSAT HRI

Last Update: Feb 14, 1995 Curator: Michael Arida (ADNET)
HEASARC Guest Observer Facility
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This file was last modified on Monday, 13-Sep-1999 15:47:29 EDT

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