The performance of JWST's Mid-Infrared Instrument (MIRI) is predicted by a model that uses a number of parameters derived from laboratory measurements.
The pre-flight performance of MIRI has been studied in detail by Glasse et al. (2015) and Boccaletti et al. (2015). These studies bring together performance metrics from laboratory testing with a sensitivity model formulated by Swinyard et al. (2004). The performance is being updated with in-flight measurements.
These models, modified by in-flight measurements have been adapted by the Exposure Time Calculator (ETC). Operational overheads (Gordon et al. 2014), including target acquisition, small angle maneuvers to allow efficient background subtraction, time spent moving MIRI mechanisms, or taking calibration observations are incorporated and included in the final time calculated by the Astronomer's Proposal Tool (APT).
Available JWST Mid-Infrared Instrument (MIRI) performance articles are listed below:
More articles will be released in the near future.
Boccaletti, A. et al. 2015, PASP, 127, 633
The Mid-Infrared Instrument for the James Webb Space Telescope, V: Predicted Performance of the MIRI Coronagraphs
Glasse, A. et al., 2015, PASP, 127, 686
The Mid-Infrared Instrument for the James Webb Space Telescope, IX: Predicted Sensitivit
Gordon, K. D. et al., 2014, PASP, 127, 696
The Mid-Infrared Instrument for the James Webb Space Telescope, X: Operations and Data Reduction
Swinyard B. M., et al., 2004, Proc. SPIE, 5487, 785
Sensitivity estimates for the mid-infrared instrument (MIRI) on the JWST