Jeremy Heyl,1 Ilaria Caiazzo,2 Sarah Gallagher,3 Kelsey Hoffman,4 Samar Safi-Harb5
1The Univ. of British Columbia (Canada) 2California Institute of Technology (United States) 3Western Univ. (Canada) 4Bishop's Univ. (Canada) 5Univ. of Manitoba (Canada)
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We propose a high-time-resolution, high-spectral-resolution X-ray telescope that uses transition-edge sensors (TES) as detectors and collector optics to direct the X-rays onto the focal plane, providing a large effective area in a small satellite. The key science driver of the instrument is to study neutron stars and accreting black holes. The proposed instrument is built upon two technologies that are already at high TRL: TES X-ray detectors and collector optics.
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Jeremy Heyl, Ilaria Caiazzo, Sarah Gallagher, Kelsey Hoffman, Samar Safi-Harb, "The Colibrì high-resolution x-ray telescope," Proc. SPIE 11444, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, 114442A (13 December 2020); https://doi.org/10.1117/12.2562625