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Time series observations with the mid-infrared instrument (MIRI) on JWST

MPS-Authors

Kendrew,  Sarah
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Dicken,  Daniel
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bouwman,  Jeroen
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Garcia Marin,  Macarena
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Greene,  Thomas P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lagage,  Pierre-Olivier
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ressler,  Mike
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Crouzet,  Nicolas
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kreidberg,  Laura
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Batalha,  Natalie M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bean,  Jacob L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Stevenson,  Kevin B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Glasse,  Alistair
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Wright,  Gillian S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Rieke,  George H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Kendrew, S., Dicken, D., Bouwman, J., Garcia Marin, M., Greene, T. P., Lagage, P.-O., et al. (2018). Time series observations with the mid-infrared instrument (MIRI) on JWST.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CCDC-E
Abstract
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 ob- servations. MIRI, the only JWST instrument covering the wavelength range longwards of 5 µm 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.