Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node960.html
Дата изменения: Tue Sep 20 19:45:21 2011
Дата индексирования: Mon Apr 11 03:39:47 2016
Кодировка:
Description

Calibration Access and Data Handbook


next up previous contents
Next: Generation from Ground Calibration Up: DIFFUSEGALA Previous: DIFFUSEGALA   Contents

Description

A copy of this CCF component is used by the PHS tools.

The DiffuseGala file consists of three extensions:
DGL_MAP The mapping of the diffuse galactic emission in galactic coordinates. The map is in S10 units. When reading the Image extension DGL_MAP, the keywords CRVALn, CRPIXn and CDELTn have to be interpreted.
DGL_SPEC The assumed spectrum of the DGL.
DGL_COUNTS The expected count rates (cts/s/subpixel) in the different filter elements.

The format of the DiffuseGala CCF component is described in detail below.

Image: DGL_MAP
keyword name keyword type keyword unit keyword value comment
BITPIX   not applicable -32  
NAXIS I not applicable 2  
NAXIS1 I not applicable varies  
NAXIS2 I not applicable varies  
CTYPE1 S not applicable gal. longitude  
CRVAL1 E degree varies reference longitude
CDELT1 E degree varies increment of longitude
CRPIX1 I not applicable varies address of reference pixel
CTYPE2 S not applicable gal. latitude  
CRVAL2 E degree   reference latitude
CDELT2 E degree   increment of latitude
CRPIX2 I not applicable varies address of reference pixel
BUNIT S S10(B) may vary Units of image

Binary table: DGL_SPEC
keyword keyword type keyword unit keyword value
REF_INTENS E S10(B) may vary
column name column type column unit comment
LAMBDA E nm wavelength
FLUX E $W/m^2/nm/deg^2$ DGL flux for reference intensity

Binary table: DGL_COUNTS
keyword keyword type keyword unit keyword value
REF_INTENS E S10(B) may vary
column name column type column unit comment
FILTER_ID 9A not applicable filter ID
COUNTS E cts/sec/subpixel expected flux per pixel
      at the reference intensity


next up previous contents
Next: Generation from Ground Calibration Up: DIFFUSEGALA Previous: DIFFUSEGALA   Contents
Michael Smith 2011-09-20