Next: A Instrument Tables
Up: 13 Calibration G Products
Previous: 13.18 Effective solid angles
Description Parameter: Appendix C
Processing Level: none
Usage in processing: N/A
File Type: Binary FITS Table
File Names: PCCBB, PCCMBBONE, PCCMBBTWO, PCCPOWER
The colour correction tables are not used in OLP. Since the colour
corrections depend on source specific assumptions, no efforts were made
for implementation in OLP. The Cal G products give
the observer the possibility to apply colour corrections.
Colour corrections are provided for 4 different
models of the infrared continuum: blackbody , modified
blackbodies with 1 and 2,
and power law continua . A description of the derivation
of the colour corrections is given in Appendix C.
The flux density value in OLP which refers to a source spectrum has to be divided by the colour correction factor associated to the assumed source spectrum.
Binary FITS table with record length 104. The record fields are:
Field Offset Number Type Description TEMP 0 1 R*4 Temperature in K P1_3.29 4 1 R*4 P1 3.3 m correction P1_3.60 8 1 R*4 P1 3.6 m correction P1_4.85 12 1 R*4 P1 4.8 m correction P1_7.30 16 1 R*4 P1 7.3 m correction P1_7.70 20 1 R*4 P1 7.7 m correction P1_10.0 24 1 R*4 P1 10 m correction P1_11.3 28 1 R*4 P1 11.3 m correction P1_11.5 32 1 R*4 P1 12 m correction P1_12.8 36 1 R*4 P1 12.8 m correction P1_16.0 40 1 R*4 P1 15 m correction P2_20 44 1 R*4 P2 20 m correction P2_25 48 1 R*4 P2 25 m correction P3_60 52 1 R*4 P3 60 m correction P3_100 56 1 R*4 P3 100 m correction C1_50 60 1 R*4 C100 70 m correction C1_60 64 1 R*4 C100 60 m correction C1_70 68 1 R*4 C100 80 m correction C1_90 72 1 R*4 C100 90 m correction C1_100 76 1 R*4 C100 100 m correction C1_105 80 1 R*4 C100 105 m correction C2_120 84 1 R*4 C200 120 m correction C2_135 86 1 R*4 C200 150 m correction C2_160 92 1 R*4 C200 170 m correction C2_180 96 1 R*4 C200 180 m correction C2_200 100 1 R*4 C200 200 m correction
Same file structure as in section 13.19.1
Same file structure as in section 13.19.1
Same file structure as in section 13.19.1, but instead of temperature in field 1, the exponent of the power law is given.
ISOPHOT Data Users Manual, Version 4.1, SAI/95-220/Dc