Emu: A Case Study for TDI-like Imaging for Infrared Observation from Space
Joice Mathew, James Gilbert, Robert Sharp, Alexey Grigoriev, Adam D., Rains, Anna M. Moore, Annino Vaccarella, Aurelie Magniez, David Chandler, Ian, Price, Luca Casagrande, Maru\v{s}a \v{Z}erjal, Michael Ireland, Michael S., Bessell, Nicholas Herrald, Shanae King

TL;DR
The Emu space telescope employs TDI-like imaging with advanced infrared detectors from the ISS to survey cool stars at 1.4 μm, enabling new astrophysical insights into stellar properties and compositions.
Contribution
This paper introduces the Emu mission's TDI-like imaging technique using SAPHIRA detectors for infrared sky surveys from space, a novel approach for studying cool stars.
Findings
Demonstrated the feasibility of TDI-like imaging in space-based infrared observations.
Simulated the instrument's capability to measure water absorption in cool stars.
Outlined the science potential for understanding stellar compositions and galaxy formation.
Abstract
A wide-field zenith-looking telescope operating in a mode similar to Time-Delay-Integration (TDI) or drift scan imaging can perform an infrared sky survey without active pointing control but it requires a high-speed, low-noise infrared detector. Operating from a hosted payload platform on the International Space Station (ISS), the Emu space telescope employs the paradigm-changing properties of the Leonardo SAPHIRA electron avalanche photodiode array to provide powerful new observations of cool stars at the critical water absorption wavelength (1.4 m) largely inaccessible to ground-based telescopes due to the Earth's own atmosphere. Cool stars, especially those of spectral-type M, are important probes across contemporary astrophysics, from the formation history of the Galaxy to the formation of rocky exoplanets. Main sequence M-dwarf stars are the most abundant stars in the Galaxy…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Stellar, planetary, and galactic studies · Astronomical Observations and Instrumentation
