12 July 2008 The JWST tunable filter imager (TFI)
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The Fine Guidance Sensor (FGS) of the James Webb Space Telescope (JWST) features a tunable filter imager (TFI) module covering the wavelength range from 1.6 to 4.9 μm at a resolving power of ~100 over a field of view of 2.2'x2.2'. TFI also features a set of 4 occulting spots for coronagraphy. A review of the current design and development status of TFI is presented along with two key TFI science programs: the detection of first light, high-redshift Lyα emitters and the detection/characterization of exoplanets.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. Doyon, R. Doyon, N. Rowlands, N. Rowlands, J. Hutchings, J. Hutchings, C. E. Evans, C. E. Evans, E. Greenberg, E. Greenberg, A. D. Scott, A. D. Scott, D. Touhari, D. Touhari, M. Beaulieu, M. Beaulieu, R. Abraham, R. Abraham, L. Ferrarese, L. Ferrarese, A. W. Fullerton, A. W. Fullerton, R. Jayawardhana, R. Jayawardhana, D. Johnston, D. Johnston, M. R. Meyer, M. R. Meyer, J. Pipher, J. Pipher, M. Sawicki, M. Sawicki, } "The JWST tunable filter imager (TFI)", Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 70100X (12 July 2008); doi: 10.1117/12.789504; https://doi.org/10.1117/12.789504


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