Difference: SpireCalibrationWeb (20 vs. 21)

Revision 212011-05-18 - IvanV

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META TOPICPARENT name="WebHome"

SPIRE instrument and calibration web pages

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FTS data processing

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  • Telescope RSRFs (daily dark sky observation) are available here for HIPE 5.x and here for HIPE 6.x. These can be used directly in the user processing script. For best results, one should use the telescope RSRF derived from a daily dark taken in the day of the observation.
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  • Telescope RSRFs (daily dark sky observation) are available here for different versions of HIPE. These can be used directly in the user processing script. For best results, one should use the telescope RSRF derived from a daily dark taken in the day of the observation. The RSRF file must match the spectral resolution of the observations, the links with "aH, aM, and aL" are for the apodized case.
 
META FILEATTACHMENT attr="" autoattached="1" comment="" date="1304680364" name="SPIRE-BSS-DOC-002966_SPIRE_Spectrometer_pipeline_description_Draft_3_1.pdf" path="SPIRE-BSS-DOC-002966_SPIRE_Spectrometer_pipeline_description_Draft_3_1.pdf" size="774644" user="Main.LucaConversi" version="1"
META FILEATTACHMENT attr="" autoattached="1" comment="" date="1305107081" name="beam_release_note_v1-1.pdf" path="beam_release_note_v1-1.pdf" size="4141606" user="Main.LucaConversi" version="1"
 
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