Data processing pipeline for Herschel HIFI
Artikel i vetenskaplig tidskrift, 2017
Context. The HIFI instrument on the Herschel Space Observatory performed over 9100 astronomical observations, almost 900 of which were calibration observations in the course of the nearly four-year Herschel mission. The data from each observation had to be converted from raw telemetry into calibrated products and were included in the Herschel Science Archive. Aims. The HIFI pipeline was designed to provide robust conversion from raw telemetry into calibrated data throughout all phases of the HIFI missions. Pre-launch laboratory testing was supported as were routine mission operations. Methods. A modular software design allowed components to be easily added, removed, amended and / or extended as the understanding of the HIFI data developed during and after mission operations. Results. The HIFI pipeline processed data from all HIFI observing modes within the Herschel automated processing environment as well as within an interactive environment. The same software can be used by the general astronomical community to reprocess any standard HIFI observation. The pipeline also recorded the consistency of processing results and provided automated quality reports. Many pipeline modules were in use since the HIFI pre-launch instrument level testing. Conclusions. Processing in steps facilitated data analysis to discover and address instrument artefacts and uncertainties. The availability of the same pipeline components from pre-launch throughout the mission made for well-understood, tested, and stable processing. A smooth transition from one phase to the next significantly enhanced processing reliability and robustness.
methods: data analysis
instrumentation: spectrographs
Författare
R. Shipman
Netherlands Institute for Space Research (SRON)
Rijksuniversiteit Groningen
S. F. Beaulieu
University of Waterloo
D. Teyssier
Europeiska rymdorganisationen (ESA)
P. Morris
California Institute of Technology (Caltech)
M. Rengel
Max-Planck-Gesellschaft
Europeiska rymdorganisationen (ESA)
C. McCoey
University of Waterloo
K. Edwards
University of Waterloo
D. Kester
Netherlands Institute for Space Research (SRON)
A. Lorenzani
Osservatorio Astrofisico di Arcetri
O. Coeur-Joly
Universite Paul Sabatier Toulouse III
M. Melchior
Fachhochschule Nordwestschweiz
J. Xie
Europeiska rymdorganisationen (ESA)
E. Sanchez
Europeiska rymdorganisationen (ESA)
P. Zaal
Netherlands Institute for Space Research (SRON)
I. M. Avruch
Netherlands Institute for Space Research (SRON)
C. Borys
California Institute of Technology (Caltech)
J. Braine
Laboratoire d'Astrophysique de Bordeaux
C. Comito
Universität zu Köln
B. Delforge
Rijksuniversiteit Groningen
F. Herpin
Laboratoire d'Astrophysique de Bordeaux
A. Hoac
California Institute of Technology (Caltech)
W. Kwon
Netherlands Institute for Space Research (SRON)
Korea Astronomy and Space Science Institute
S. D. Lord
California Institute of Technology (Caltech)
A. P. Marston
Space Telescope Science Institute (STScI)
M. Mueller
Netherlands Institute for Space Research (SRON)
Rijksuniversiteit Groningen
Michael Olberg
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
V. Ossenkopf
Universität zu Köln
E. Puga
Europeiska rymdorganisationen (ESA)
M. Akyilmaz-Yabaci
Universität zu Köln
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 608 A49- A49Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Infrastruktur
Onsala rymdobservatorium
DOI
10.1051/0004-6361/201731385