IRFLUX-Flux calibrates an IR spectrum using a black-body model

Description:

Flux calibrates an IR spectrum using a black body model for a standard star.

Parameters:

SPECTRUM

Name of Star spectrum.

STANDARD

Name of Standard spectrum.

TEMP

Temperature of standard.

CALTYPE

Type of calibration data.

MAG

Magnitude of standard star.

FLUX

Flux of standard star at calib wavelength (mJy).

WAVE

Calibration wavelength (microns).

OUTPUT

Name of resulting spectrum.

Source comments:

 I R F L U X

 Flux calibrates an IR spectrum using a black body model for a
 standard star

 Command parameters -

 SPECTRUM  The name of the structure containing the first image.

 STANDARD  The name of the structure containing the second
           image data.

 TEMP      The temperature of the black body to be used.

 CALTYPE   The type of calibration data. A single character as follows:
              'J','H','K','L','M' - magnitude in a standard band
              'F' - Flux at specified wavelength

 MAG       The magnitude of the standard used.

 FLUX      The flux in mJy of the standard.

 WAVE      The wavelength at which the flux is specified.

 OUTPUT    The name of the result of the operation.  This can
           be the same as for SPECTRUM.  If not, a new structure
           is created, with everything but the data a direct
           copy of the input.

                                      JAB / JAC  19th Sep 1990