Abstract
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.
Herschel was an ESA space observatory with science instruments provided
by European-led Principal Investigator consortia and with important
participation from NASA.
Original language | English |
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Journal | Astronomy & Astrophysics |
Volume | 608 |
DOIs | |
Publication status | Published - 1-Dec-2017 |
Keywords
- instrumentation: spectrographs
- methods: data analysis