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JWST/MIRI Data Reduction and Products

Bright, SN; Gordon, KD; Chen, CH; Lajoie, R; Azzollini, R; Bergeron, L; Bouchet, P; ... Wright, GS; + view all (2016) JWST/MIRI Data Reduction and Products. In: Lorente, NPF and Shortridge, K and Wayth, R, (eds.) Astronomical Data Analysis Software and Systems XXV. (pp. pp. 371-374). Astronomical Society of the Pacific: Sydney, NSW, Australia. Green open access

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Abstract

The Mid-Infrared Instrument (MIRI) is one of four science instruments to be flown aboard the James Webb Space Telescope (JWST). MIRI operates from 5 to 28.5 microns and provides a suite of versatile capabilities including imaging, low-resolution spectroscopy (LRS), medium-resolution spectroscopy (MRS) via an integral field unit, and coronagraphy. The MIRI pipeline consists of three stages: 1) Raw to Slope Images, 2) Calibrated Slope Images, and 3) Multiple Exposures Combined. The pipeline is designed to provide well-calibrated, high level data products that maximize the scientific return from the instrument.

Type: Proceedings paper
Title: JWST/MIRI Data Reduction and Products
Event: Twenty-fifth annual conference on Astronomical Data Analysis Software and Systems (ADASS XXV)
Location: Sydney, NSW, Australia
Dates: 25 October 2015 - 29 October 2015
ISBN-13: 978-1-58381-908-1
Open access status: An open access version is available from UCL Discovery
Publisher version: http://aspbooks.org/custom/publications/paper/512-...
Language: English
Additional information: This version is the author version of record. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10085193
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