SXG icin PIMMS Ornegi

An Example of a Simple PIMMS Session


To run PIMMS, one executes a number of commands to set up the desired parameters for the run, and then the 'go' command. The basic PIMMS commands are:

In the following example, PIMMS is used to predict the count rate in the XSPECT LEPC detector for a source with a thermal Bremsstrahlung spectrum with kT = 1 keV and NH = 1.0e21, and a rate in the ASCA SIS of 1 cps.

> 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-12> product count		# Specify Count Rate product
 PIMMS-12> instrument sxg lepc		# Desired instrument is SXG LEPC
 PIMMS-12> from asca sis		# Normalization obtained from ASCA SIS
 PIMMS-12> model tb 1.0 1.0e21		# Thermal Bremsstrahlung, kT = 1.0 keV,
					# NH = 1.0e21 cm**-2
 PIMMS-12> go 1.0			# Execute, with a normalization of 
					# 1 ASCA SIS cps

  * For thermal Bremsstrahlung model with kT=  1.0000 keV; NH =  1.000E+21
    and  1.000E+00 cps in ASCA SIS
    (Model normalization =  2.894E-02)
  * PIMMS predicts  9.841E+00 cps with SXG LEPC
 PIMMS-12> quit
>
For additional examples and a fuller description of the above and other PIMMS commands, click here (external postscript viewer required, ~100 kbytes).


Problem ve sorulariniz icin lutfen umk@astroa.physics.metu.edu.tr ile temas kurun.