Paper
20 July 2016 Optimizing parallel observations for the JWST/MIRI instrument
Macarena Garcìa-Marìn, Christopher N. A. Willmer, Alvaro Labiano, Stacey Alberts, George Rieke, Gillian Wright, Marcia Rieke
Author Affiliations +
Abstract
Using unprecedented sensitivity and angular resolution, the Mid-IR (MIRI) instrument for the James Webb Space Telescope (JWST) will provide imaging, coronagraphy, single slit and integral-field spectroscopy for many science observations. The expectation is that the operational design of the JWST will include parallel modes. We have been studying the intricacies of combining MIRI (5-28.5 μm) and Near-IR Camera (NIRCam) (0.6-5 μm) imaging observations for a deep imaging use-case. Such programs present particular challenges from an operations point of view. This contribution presents the overall design of the MIRI observations in parallel with NIRCam, opening the path to collaborative science opportunities between MIRI and the other JWST instruments.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Macarena Garcìa-Marìn, Christopher N. A. Willmer, Alvaro Labiano, Stacey Alberts, George Rieke, Gillian Wright, and Marcia Rieke "Optimizing parallel observations for the JWST/MIRI instrument", Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99101R (20 July 2016); https://doi.org/10.1117/12.2233513
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KEYWORDS
James Webb Space Telescope

Sensors

Galactic astronomy

Electroluminescent displays

Coronagraphy

Observatories

Point spread functions

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