JWST MIRI flight performance: Imaging

Dan Dicken; Macarena García Marín; Irene Shivaei; Pierre Guillard; Mattia Libralato; Alistair Glasse; Karl D. Gordon; Christophe Cossou; Patrick Kavanagh; Tea Temim; Nicolas Flagey; Pamela Klaassen; George H. Rieke; Gillian Wright; Stacey Alberts; Ruyman Azzollini; Javier Álvarez-Márquez; Patrice Bouchet; Stacey Bright; Misty Cracraft; Alain Coulais; Ors Hunor Detre; Mike Engesser; Ori D. Fox; Andras Gaspar; René Gastaud; Adrian M. Glauser; Dean C. Hines; Sarah Kendrew; Alvaro Labiano; Pierre Oliver Lagage; David Lee; David R. Law; Jane E. Morrison; Alberto Noriega-Crespo; Olivia Jones; Polychronis Patapis; Silvia Scheithauer; G. C. Sloan; Laszlo Tamas

doi:10.1051/0004-6361/202449451

JWST MIRI flight performance: Imaging

Dan Dicken, Macarena García Marín, Irene Shivaei, Pierre Guillard, Mattia Libralato, Alistair Glasse, Karl D. Gordon, Christophe Cossou, Patrick Kavanagh, Tea Temim, Nicolas Flagey, Pamela Klaassen, George H. Rieke, Gillian Wright, Stacey Alberts, Ruyman Azzollini, Javier Álvarez-Márquez, Patrice Bouchet, Stacey Bright, Misty CracraftAlain Coulais, Ors Hunor Detre, Mike Engesser, Ori D. Fox, Andras Gaspar, René Gastaud, Adrian M. Glauser, Dean C. Hines, Sarah Kendrew, Alvaro Labiano, Pierre Oliver Lagage, David Lee, David R. Law, Jane E. Morrison, Alberto Noriega-Crespo, Olivia Jones, Polychronis Patapis, Silvia Scheithauer, G. C. Sloan, Laszlo Tamas

Astrophysical Sciences

Research output: Contribution to journal › Article › peer-review

8 Scopus citations

Abstract

The Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope (JWST) provides the observatory with a huge advance in mid-infrared imaging and spectroscopy covering the wavelength range of 5a 28 μm. This paper describes the performance and characteristics of the MIRI imager as understood during observatory commissioning activities, and through its first year of science operations. We discuss the measurements and results of the imagera-s point spread function, flux calibration, background, distortion and flat fields as well as results pertaining to best observing practices for MIRI imaging, and discuss known imaging artefacts that may be seen during or after data processing. Overall, we show that the MIRI imager has met or exceeded all its pre-flight requirements, and we expect it to make a significant contribution to mid-infrared science for the astronomy community for years to come.

Original language	English (US)
Article number	A5
Journal	Astronomy and Astrophysics
Volume	689
DOIs	https://doi.org/10.1051/0004-6361/202449451
State	Published - Sep 1 2024

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Instrumentation: photometers
Techniques: photometric
Telescopes

Access to Document

10.1051/0004-6361/202449451

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Dicken, D., Marín, M. G., Shivaei, I., Guillard, P., Libralato, M., Glasse, A., Gordon, K. D., Cossou, C., Kavanagh, P., Temim, T., Flagey, N., Klaassen, P., Rieke, G. H., Wright, G., Alberts, S., Azzollini, R., Álvarez-Márquez, J., Bouchet, P., Bright, S., ... Tamas, L. (2024). JWST MIRI flight performance: Imaging. Astronomy and Astrophysics, 689, Article A5. https://doi.org/10.1051/0004-6361/202449451

@article{8ec213379b834bcb9dd0e093e630ea95,

title = "JWST MIRI flight performance: Imaging",

abstract = "The Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope (JWST) provides the observatory with a huge advance in mid-infrared imaging and spectroscopy covering the wavelength range of 5a 28 μm. This paper describes the performance and characteristics of the MIRI imager as understood during observatory commissioning activities, and through its first year of science operations. We discuss the measurements and results of the imagera-s point spread function, flux calibration, background, distortion and flat fields as well as results pertaining to best observing practices for MIRI imaging, and discuss known imaging artefacts that may be seen during or after data processing. Overall, we show that the MIRI imager has met or exceeded all its pre-flight requirements, and we expect it to make a significant contribution to mid-infrared science for the astronomy community for years to come.",

keywords = "Instrumentation: photometers, Techniques: photometric, Telescopes",

author = "Dan Dicken and Mar{\'i}n, {Macarena Garc{\'i}a} and Irene Shivaei and Pierre Guillard and Mattia Libralato and Alistair Glasse and Gordon, {Karl D.} and Christophe Cossou and Patrick Kavanagh and Tea Temim and Nicolas Flagey and Pamela Klaassen and Rieke, {George H.} and Gillian Wright and Stacey Alberts and Ruyman Azzollini and Javier {\'A}lvarez-M{\'a}rquez and Patrice Bouchet and Stacey Bright and Misty Cracraft and Alain Coulais and Detre, {Ors Hunor} and Mike Engesser and Fox, {Ori D.} and Andras Gaspar and Ren{\'e} Gastaud and Glauser, {Adrian M.} and Hines, {Dean C.} and Sarah Kendrew and Alvaro Labiano and Lagage, {Pierre Oliver} and David Lee and Law, {David R.} and Morrison, {Jane E.} and Alberto Noriega-Crespo and Olivia Jones and Polychronis Patapis and Silvia Scheithauer and Sloan, {G. C.} and Laszlo Tamas",

note = "Publisher Copyright: {\textcopyright} The Authors 2024.",

year = "2024",

month = sep,

day = "1",

doi = "10.1051/0004-6361/202449451",

language = "English (US)",

volume = "689",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

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Dicken, D, Marín, MG, Shivaei, I, Guillard, P, Libralato, M, Glasse, A, Gordon, KD, Cossou, C, Kavanagh, P, Temim, T, Flagey, N, Klaassen, P, Rieke, GH, Wright, G, Alberts, S, Azzollini, R, Álvarez-Márquez, J, Bouchet, P, Bright, S, Cracraft, M, Coulais, A, Detre, OH, Engesser, M, Fox, OD, Gaspar, A, Gastaud, R, Glauser, AM, Hines, DC, Kendrew, S, Labiano, A, Lagage, PO, Lee, D, Law, DR, Morrison, JE, Noriega-Crespo, A, Jones, O, Patapis, P, Scheithauer, S, Sloan, GC & Tamas, L 2024, 'JWST MIRI flight performance: Imaging', Astronomy and Astrophysics, vol. 689, A5. https://doi.org/10.1051/0004-6361/202449451

TY - JOUR

T1 - JWST MIRI flight performance

T2 - Imaging

AU - Dicken, Dan

AU - Marín, Macarena García

AU - Shivaei, Irene

AU - Guillard, Pierre

AU - Libralato, Mattia

AU - Glasse, Alistair

AU - Gordon, Karl D.

AU - Cossou, Christophe

AU - Kavanagh, Patrick

AU - Temim, Tea

AU - Flagey, Nicolas

AU - Klaassen, Pamela

AU - Rieke, George H.

AU - Wright, Gillian

AU - Alberts, Stacey

AU - Azzollini, Ruyman

AU - Álvarez-Márquez, Javier

AU - Bouchet, Patrice

AU - Bright, Stacey

AU - Cracraft, Misty

AU - Coulais, Alain

AU - Detre, Ors Hunor

AU - Engesser, Mike

AU - Fox, Ori D.

AU - Gaspar, Andras

AU - Gastaud, René

AU - Glauser, Adrian M.

AU - Hines, Dean C.

AU - Kendrew, Sarah

AU - Labiano, Alvaro

AU - Lagage, Pierre Oliver

AU - Lee, David

AU - Law, David R.

AU - Morrison, Jane E.

AU - Noriega-Crespo, Alberto

AU - Jones, Olivia

AU - Patapis, Polychronis

AU - Scheithauer, Silvia

AU - Sloan, G. C.

AU - Tamas, Laszlo

PY - 2024/9/1

Y1 - 2024/9/1

N2 - The Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope (JWST) provides the observatory with a huge advance in mid-infrared imaging and spectroscopy covering the wavelength range of 5a 28 μm. This paper describes the performance and characteristics of the MIRI imager as understood during observatory commissioning activities, and through its first year of science operations. We discuss the measurements and results of the imagera-s point spread function, flux calibration, background, distortion and flat fields as well as results pertaining to best observing practices for MIRI imaging, and discuss known imaging artefacts that may be seen during or after data processing. Overall, we show that the MIRI imager has met or exceeded all its pre-flight requirements, and we expect it to make a significant contribution to mid-infrared science for the astronomy community for years to come.

AB - The Mid-Infrared Instrument (MIRI) aboard the James Webb Space Telescope (JWST) provides the observatory with a huge advance in mid-infrared imaging and spectroscopy covering the wavelength range of 5a 28 μm. This paper describes the performance and characteristics of the MIRI imager as understood during observatory commissioning activities, and through its first year of science operations. We discuss the measurements and results of the imagera-s point spread function, flux calibration, background, distortion and flat fields as well as results pertaining to best observing practices for MIRI imaging, and discuss known imaging artefacts that may be seen during or after data processing. Overall, we show that the MIRI imager has met or exceeded all its pre-flight requirements, and we expect it to make a significant contribution to mid-infrared science for the astronomy community for years to come.

KW - Instrumentation: photometers

KW - Techniques: photometric

KW - Telescopes

UR - http://www.scopus.com/inward/record.url?scp=85202809009&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85202809009&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/202449451

DO - 10.1051/0004-6361/202449451

M3 - Article

AN - SCOPUS:85202809009

SN - 0004-6361

VL - 689

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A5

ER -

JWST MIRI flight performance: Imaging

Abstract

All Science Journal Classification (ASJC) codes

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