Poster + Paper
23 August 2024 Pandora astrophysics pioneers SmallSat​ detector testing progress
Trevor O. Foote, Nikole K. Lewis, Elisa V. Quintana, Thomas Barclay, Thomas P. Greene, Gregory Mosby, Jessie L. Dotson, Christina Hedges, Jordan Karburn, Collin Averill, Peter Heatwole, Lance Simms, Michael Wong
Author Affiliations +
Conference Poster
Abstract
The Pandora NASA Astrophysics Pioneers SmallSat mission employs a dual-channel observational approach, simultaneously utilizing visible photometry and infrared spectroscopy to assess stellar contamination of exoplanet transmission spectra. For the near-infrared spectroscopy Pandora will use a 2.5-micron cutoff Teledyne H2RG detector. The engineering design unit has undergone thermal-vacuum testing at Lawrence Livermore National Labs to characterize its performance under flight-like conditions. This paper provides an overview of testing conducted to date, shedding light on critical detector properties derived from subsequent analyses. Key parameters include read noise, gain, and saturation, offering insights into the detector’s capabilities and paving the way for enhanced data interpretation in the pursuit of unraveling the complexities within exoplanetary atmospheres.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Trevor O. Foote, Nikole K. Lewis, Elisa V. Quintana, Thomas Barclay, Thomas P. Greene, Gregory Mosby, Jessie L. Dotson, Christina Hedges, Jordan Karburn, Collin Averill, Peter Heatwole, Lance Simms, and Michael Wong "Pandora astrophysics pioneers SmallSat​ detector testing progress", Proc. SPIE 13092, Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave, 130922P (23 August 2024); https://doi.org/10.1117/12.3019278
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KEYWORDS
Sensors

Exoplanets

Signal detection

Astrophysics

Readout integrated circuits

Near infrared

Contamination

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