What ’ s New in HIPE 10.0 (SPIRE FTS). Nanyao Lu NHSC/IPAC (on behalf of the SPIRE ICC). Calibration Improvements in HIPE 10.0.
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What’s New in HIPE 10.0(SPIRE FTS)
(on behalf of the SPIRE ICC)
Fit a polynomial to the “drift” of normalized dark observations as a function
of observational days (OD) per detector, and incorporate the result into
The telescope model as an additional multiplicative factor.
More consistent per-detector
results from dark observations
(of the telescope)
Overall standard dev. (in units of Jy) reduced
for the dark observations for most detectors.
Red: HIPE 9
Bright green: HIPE 10
Red: HIPE 9
Dark green: HIPE 10
User input in the script:
Integrated line maps
Initial fit on the selected spaxel
Residual for all spaxels
A Satisfactory Bright-source Pipeline in HIPE 11
Gray: HIPE 10 spectrum (bright-mode pipeline);
Red: HIPE 11 spectrum (bright-mode pipeline);
Blue crosses: Mars model fluxes.
Red: HIPE 10 spectrum (nominal-mode data);
Blue: HIPE 11 spectrum (bright-mode pipeline).