First Operation of TES Microcalorimeters in Space with the Micro-X Sounding Rocket

Micro-X is a sounding rocket-borne instrument that uses a microcalorimeter array to perform high-resolution X-ray spectroscopy. This instrument flew for the first time on July 22nd, 2018, from the White Sands Missile Range, USA. This flight marks the first successful operation of a transition-edge s...

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Veröffentlicht in:Journal of low temperature physics 2020-05, Vol.199 (3-4), p.1062-1071
Hauptverfasser: Adams, J. S., Baker, R., Bandler, S. R., Bastidon, N., Danowski, M. E., Doriese, W. B., Eckart, M. E., Figueroa-Feliciano, E., Goldfinger, D. C., Heine, S. N. T., Hilton, G. C., Hubbard, A. J. F., Kelley, R. L., Kilbourne, C. A., Manzagol-Harwood, R. E., McCammon, D., Okajima, T., Porter, F. S., Reintsema, C. D., Serlemitsos, P., Smith, S. J., Ullom, J. N., Wikus, P.
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Sprache:eng
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Zusammenfassung:Micro-X is a sounding rocket-borne instrument that uses a microcalorimeter array to perform high-resolution X-ray spectroscopy. This instrument flew for the first time on July 22nd, 2018, from the White Sands Missile Range, USA. This flight marks the first successful operation of a transition-edge sensor array and its time-division multiplexing readout system in space. This launch was dedicated to the observation of the supernova remnant Cassiopeia A. A failure in the attitude control system prevented the rocket from pointing and led to no time on target. The onboard calibration source provided X-rays in flight, and it is used to compare detector performance during preflight integration, flight, and after the successful post-flight recovery. This calibration data demonstrate the capabilities of the detector in a space environment as well as its potential for future flight.
ISSN:0022-2291
1573-7357
DOI:10.1007/s10909-019-02293-5