!
!                     THE NuSTAR SSDC SIMULATOR
!      EXAMPLE of input file for the simulation of pointlike sources
!
! The first non-blank or uncommented line,(i.e. without a "!" at the beginning)
! must include the EQUINOX to be used for the coordinates and the ENERGY RANGE
! in units of keV, where the X-ray flux is calculated.
! The following uncommented lines (one line per source, up to 10,000 lines)
! must include the RA and DEC, the source X-RAY FLUX
! the SPECTRAL MODEL to be used for the simulation and the SPECTRAL PARAMETERS
! for the chosen models. (Please use the same format as in the examples)
!
! PLEASE note that the FIELD CENTER will be set to the position of 
! of the FIRST source in the list which will therefore become the TARGET of the
! simulated field  
!
!  The simulator supports the XSPEC models described below
!  See the XSPEC manual for more detailed models description
!
! -----------------------------------------------------------------------
!  model name:       wabs
!
!  description:  Photoelectric absorption using Morrison and McCammon
!                                                       cross-sections
!  always used in conjunction (multiplied) with one of the allowed models
!                                                        described below)
!  parameters    NH in units of atoms*cm-2 , e.g. 3.e20
! -----------------------------------------------------------------------
!  model name:       powerlaw
!
!  description: Simple photon power law. [A(E) = K (E/1 keV)**(-par1)]
!  parameters : par1 (photon index)
!  example (absorbed power law)
!                                                     NH   par1 unused unused
!100.000   -20.0000    1.00e-13   wabs   powerlaw   3.0e20 1.5   0.    0.
!
! -----------------------------------------------------------------------
! model name:        bkn
!
!  description: Broken powerlaw
!      A(E) = K * (E/1 keV)**-par1                         for E < par2
!           = K * par2**(par3-par1) * (E/1 keV)**-par3     for E > par2
!  parameters : par1, par2, par3
!  example (absorbed broken power law)
!                                                    NH     par1 ener  par3
!                                                                break
!100.000   -20.0000    2.00e-13   wabs   bkn        1.63e21 1.8   3.   2.4 
!
! -----------------------------------------------------------------------
! model name:        bremss
!
! description: Thermal bremsstrahlung spectrum
! parameters : par1=plasma temperature in keV
! example (absorbed  bremss)
!100.000   -20.0000    1.00e-13   wabs   bremss      4.0e20  5.0  0.   0.
! ---------------------------------------------------------------------------
!
!       ---------- PART USED BY SIMULATOR STARTS HERE ----------
!
! equinox energy range for fluxes 
  2000.         5.   10.
!
!   ra        dec        flux       models            parameters
! degrees   degrees    erg/cm2/s
!
 356.770    51.7050    2.00e-13   wabs   bkn        1.63e21 1.8   3.   2.4 
 356.680    51.7030    8.12e-12   wabs   powerlaw   3.90e20 1.7   0.   0.
 356.800    51.7100    1.83e-13   wabs   bremss     3.90e20 5.0   0.   0.
! other sources (up to a total of 10,000) may be added