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.
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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-pp.ucl.ac.uk/id/eprint/10085193 |
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