Time series observations with the Mid-Infrared Instrument (MIRI) on JWST

被引：6

作者：

Kendrew, Sarah ^{[1
]}

Dicken, Daniel ^{[2
]}

Bouwman, Jeroen ^{[3
]}

Marin, Macarena Garcia ^{[1
]}

Greene, Thomas P. ^{[4
]}

Lagage, Pierre-Olivier ^{[2
]}

Ressler, Mike ^{[5
]}

Crouzet, Nicolas ^{[6
]}

Kreidberg, Laura ^{[7
]}

Batalha, Natalie M. ^{[4
]}

Bean, Jacob L. ^{[8
]}

Stevenson, Kevin B. ^{[9
]}

Glasse, Alistair ^{[10
]}

Wright, Gillian S. ^{[10
]}

Rieke, George H. ^{[11
]}

机构：

[1] Space Telescope Sci Inst, European Space Agcy, 3700 San Martin Dr, Baltimore, MD 21218 USA

[2] CEA Saclay, Paris, France

[3] Max Planck Inst Astron, Heidelberg, Germany

[4] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[5] CALTECH, Jet Prop Lab, Pasadena, CA USA

[6] Inst Astrofis Canarias, Tenerife, Spain

[7] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[8] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA

[9] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[10] Royal Observ Edinburgh, UK Astron Technol Ctr, Edinburgh, Midlothian, Scotland

[11] Univ Arizona, Steward Observ, Tucson, AZ USA

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2018: OPTICAL, INFRARED, AND MILLIMETER WAVE | 2018年 / 10698卷

关键词：

JWST; space telescopes; time series; exoplanets; mid-infrared; WEBB-SPACE-TELESCOPE;

D O I：

10.1117/12.2313951

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Time-variable phenomena such as transiting exoplanets will be a major science theme for the James Webb Space Telescope (JWST). For Guaranteed Time and Early Release Science Observations, over 500 hours of JWST time have been allocated to time series observations (TSOs) of transiting exoplanets. Several dedicated observing modes are available in the instrument suite, whose operations are specifically tailored to these challenging observations. MIRI, the only JWST instrument covering the wavelength range longwards of 5 mu m on JWST, will offer TSOs in two of its modes: the low resolution spectrometer, and the imager. In this paper we will describe these modes for MIRI, and discuss how they differ operationally from regular (non-TSO) observations. We will show performance estimates based on ground testing and modeling, discuss the most relevant detector effects for high precision (spectro-)photometry, and provide some guidelines for planning MIRI TSOs.

引用

页数：10

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