The Mid-Infrared Instrument for the James Webb Space Telescope, I: Introduction

By G. Rieke, G. Wright, T. Böker, J. Bouwman, L. Colina, A. Glasse, K. Gordon, T. Greene, M. Gudel, Th. Henning and 8 more. 2015

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CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results (2022, background): “…et al. 2003, 2005; Beichman et al. 2012) short and long-wavelength channels in ten pointings, observed as coordinated parallels to primary observations with the Near Infrared Spectrograph (NIRSpec; Jakobsen et al. 2022) and the MidInfrared Instrument (MIRI; Rieke et al. 2015; Wright et al. 2015).”
The James Webb Space Telescope Mission (2023, methodology): “MIRI (Rieke et al. 2015a; Wright et al. 2015, 2023, this issue) provides both imaging in broad-band filters and IFU spectroscopy from 5.0 to 28.0 μm.”
Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure (2022, unknown): “The infrared instruments aboard the James Webb Space Telescope (Gardner et al. 2006; Beichman et al. 2012; Artigau et al. 2014; 3 Rieke et al. 2015; Labiano et al. 2021) will search for confirmation and spectral classification of this distant star to define its place on the Hertzsprung–Russell…”
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging (2022, methodology): “Such confirmation should be possible in modest exposure times with the NIRSpec and/or MIRI spectrographs on board JWST.”