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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 448028.0, MPI für Astronomie / Publikationen_mpia
The HERSCHEL/PACS Spectrometer Pipeline
Authors:Schreiber, J.; Wieprecht, E.; de Jong, J.; Wetzstein, M.; Jacobson, J.; Huygen, R.; Appleton, P.; Bouwman, J.; Contursi, A.; Fadda, D.; Jean, C.; Klaas, U.; Royer, P.; Vandenbussche, B.
Place of Publication:San Francisco
Date of Publication (YYYY-MM-DD):2009
Title of Proceedings:Astronomical Data Analysis Software and Systems XVIII
Start Page:478
End Page:481
Title of Series:ASP Conf. Ser.
Volume (in Series):411
Review Status:not specified
Audience:Experts Only
Abstract / Description:ESA's Herschel Space Observatory, to be launched in 2009, is the first space observatory covering the full far-infrared and sub-millimeter wavelength range (60 - 670 micron). The Photodetector Array Camera & Spectrometer (PACS) is one of the three science instruments. It employs two Ge:Ga photoconductor arrays and two bolometer arrays to perform integral field spectroscopy and imaging photometry in the 60 - 210 micron wavelength band. The interactive PACS Spectrometer and Photometer \citep{wieprecht09} Data Reduction Pipeline is integrated in the Herschel Data Processing System. The DP is implemented using Java technology and written in a common effort by the HERSCHEL Science Center (HSC) and the three instrument teams. We overview the concept and status of the PACS Spectrometer Data Reduction Pipeline. Additionally, we address the instrument mode-dependent data processing and the definition of the products of the different processing levels. Finally, we show first results by applying the pipeline on flight model instrument level test data.
Comment of the Author/Creator:Date: 2009, September 1, 2009
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2009ASPC..411..478S [ID No:1]
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