Poster
13 December 2020 Properties and characteristics of the Nancy Grace Roman Space Telescope H4RG-10 detectors
Author Affiliations +
Conference Poster
Abstract
The Nancy Grace Roman Space Telescope (Roman) formerly known as the Wide-Field Infrared Survey Telescope will answer fundamental questions about the evolution of dark energy over time and expand the catalog of known exoplanets into new regions of parameter space. Using a Hubble-sized mirror and 18 newly developed HgCdTe 4K × 4K photodiode arrays (H4RG-10), the Roman Space Telescope will measure the positions and shapes of hundreds of millions of galaxies, the light curves of thousands of supernovae, and the microlensing signals of over a thousand exoplanets toward the bulge of the Galaxy. These measurements require unprecedented sensitivity and characterization of the Wide Field Instrument, particularly its detectors. The Roman project undertook an extensive detector development program to create focal plane arrays that meet these science requirements. We present the performance characteristics of these TRL-6 demonstration devices.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gregory Mosby Jr., Bernard J. Rauscher, Robert J. Hill, Roger Foltz, Analia Cillis, Jon Mah, David Cottingham, Yiting Wen, Lane A. Meier, Augustyn Waczynski, Chris Merchant, and Chris Bennett "Properties and characteristics of the Nancy Grace Roman Space Telescope H4RG-10 detectors", Proc. SPIE 11454, X-Ray, Optical, and Infrared Detectors for Astronomy IX, 1145433 (13 December 2020); https://doi.org/10.1117/12.2560256
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KEYWORDS
Sensors

Exoplanets

Galactic astronomy

Infrared telescopes

Detector development

Infrared radiation

Mercury cadmium telluride

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