The MIRI Medium Resolution Spectrometer calibration pipeline
Paper i proceeding, 2016
The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer (MRS) is the only mid-IR Integral Field Spectrometer on board James Webb Space Telescope. The complexity of the MRS requires a very specialized pipeline, with some specific steps not present in other pipelines of JWST instruments, such as fringe corrections and wavelength offsets, with different algorithms for point source or extended source data. The MRS pipeline has also two different variants: the baseline pipeline, optimized for most foreseen science cases, and the optimal pipeline, where extra steps will be needed for specific science cases. This paper provides a comprehensive description of the MRS Calibration Pipeline from uncalibrated slope images to final scientific products, with brief descriptions of its algorithms, input and output data, and the accessory data and calibration data products necessary to run the pipeline.
Pipeline
MIRI
Data
MRS
JWST
Calibration
Författare
A. Labiano
Eidgenössische Technische Hochschule Zürich (ETH)
R. Azzollini
Dublin Institute for Advanced Studies
J. Bailey
Universiteit Leiden
S. Beard
UK Astronomy Technology Centre
D. Dicken
Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA)
M. Garcia-Marin
Europeiska rymdorganisationen (ESA)
Space Telescope Science Institute (STScI)
V. C. Geers
UK Astronomy Technology Centre
A. Glasse
UK Astronomy Technology Centre
A. M. Glauser
Eidgenössische Technische Hochschule Zürich (ETH)
K. Gordon
Space Telescope Science Institute (STScI)
Kay Justtanont
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
P. Klaassen
UK Astronomy Technology Centre
F. Lahuis
Netherlands Institute for Space Research (SRON)
D. Law
Space Telescope Science Institute (STScI)
J. E. Morrison
Space Telescope Science Institute (STScI)
University of Arizona
M. Müller
Rijksuniversiteit Groningen
G. H. Rieke
University of Arizona
B. Vandenbussche
KU Leuven
G. Wright
UK Astronomy Technology Centre
Proceedings of SPIE - The International Society for Optical Engineering
0277786X (ISSN) 1996756X (eISSN)
Vol. 9910 99102W- 99102I978-1-5106-0199-4 (ISBN)
Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1117/12.2232554
ISBN
978-1-5106-0199-4