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.

MRS

JWST

Pipeline

Data

Calibration

MIRI

Författare

A. Labiano

ETH Zurich

R. Azzollini

Dublin Institute for Advanced Studies

J. Bailey

Leiden Observatory Research Institute

S. Beard

UK Astronomy Technology Centre

D. Dicken

CEA Saclay

M. Garcia-Marin

STScI

European Space Agency - ESA

V. C. Geers

UK Astronomy Technology Centre

A. Glasse

UK Astronomy Technology Centre

A. M. Glauser

ETH Zurich

K. Gordon

STScI

Kay Justtanont

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

P. Klaassen

UK Astronomy Technology Centre

F. Lahuis

SRON Netherlands Institute for Space Research

D. Law

STScI

J. E. Morrison

STScI

University of Arizona

M. Müller

University of Groningen, Kapteyn Astronomical Institute

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- 99102I

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1117/12.2232554

ISBN

978-1-5106-0199-4