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The MIRI Medium Resolution Spectrometer calibration pipeline

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arxiv 1608.05312 v1 pith:DT3NESY2 submitted 2016-08-18 astro-ph.IM

A. Labiano , R. Azzollini , J. I. Bailey III , S. Beard , D. Dicken , M. García-Marín , V. Geers , A. Glasse
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A. Glauser K. Gordon K. Justtanont P. Klaassen F. Lahuis D. Law J. Morrison M. Müller G. Rieke B. Vandenbussche G. Wright
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 12 citations worldwide. Full citation record

  1. MICONIC: The multiphase circumnuclear region of Centaurus A as seen with JWST/MIRI MRS observations. I. Spectral inventory and properties of the warm molecular disk

    astro-ph.GA 2026-05 conditional novelty 7.0 of 10

    New JWST observations of Centaurus A detect H2 lines up to S(8) and map a warm molecular disk with a 20-pc cavity aligned to the jet, filamentary high-excitation structures, S-shaped kinematics, and an inward streamer...

  2. JWST MIRI/MRS observations of hot molecular gas in an AGN host galaxy at Cosmic Noon

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    First detection of hot molecular gas via H2 2.12 micrometer emission in an AGN host at z~2.2, with a hot-to-cold gas mass ratio near one millionth.

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