Published 2015
| Version Published
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The Herschel/SPIRE Spectrometer Useful Scripts
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Abstract
In most cases, the Standard Product Generation (SPG) processing pipelines for the Herschel SPIRE Fourier Transform Spectrometer (FTS) produce well-calibrated spectra of high quality. However, some Astronomical sources, such as those with a faint continuum, require additional processing to achieve more meaningful spectra. In consultation with the astronomical community, a set of scripts were developed to assist in the post-pipeline analysis of the spectra.
Additional Information
© 2015 Astronomical Society of the Pacific. The funding for the Canadian contribution to SPIRE is provided by the Canadian Space Agency and NSERC.Attached Files
Published - 495-0339.pdf
Files
495-0339.pdf
Additional details
Identifiers
- Eprint ID
- 65649
- Resolver ID
- CaltechAUTHORS:20160324-084636797
Funding
- Canadian Space Agency (CSA)
- Natural Sciences and Engineering Research Council of Canada (NSERC)
Dates
- Created
-
2016-03-30Created from EPrint's datestamp field
- Updated
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2019-10-03Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- Astronomical Society of the Pacific conference series
- Series Volume or Issue Number
- 495