Detector Calibration for the Micro-X Sounding Rocket X-ray Telescope
Author(s)
Goldfinger, D. C; Adams, J. S; Baker, R.; Bandler, S. R; Bastidon, N.; Danowski, M. E; Doriese, W. B; Eckart, M. E; Figueroa-Feliciano, E.; Heine, S. N T; Hilton, G. C; Hubbard, A. J F; Kelley, R. L; Kilbourne, C. A; Manzagol-Harwood, R. E; McCammon, D.; ... Show more Show less
Download10909_2018_2060_ReferencePDF.pdf (144.5Kb)
Publisher Policy
Publisher Policy
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Terms of use
Metadata
Show full item recordAbstract
Abstract
Micro-X is a sounding rocket-borne X-ray telescope that uses a transition edge sensor microcalorimeter array to provide high-energy-resolution spectroscopy. Micro-X is a versatile instrument with plans to observe the Puppis A supernova remnant during its first flight, as well as future observations of the Milky Way to search for X-ray signals from decaying dark matter. Commissioning and functionality testing are complete, and the thermal performance of the system has been validated. We are currently evaluating the detector performance in the flight cryostat with the flight multiplexing electronics. Operating in this setup has allowed us to characterize sources of detector and readout noise, as well as to implement mitigation techniques to improve performance in anticipation of the upcoming flight. We present an overview of important noise considerations in addition to an update on latest detector performance.
Date issued
2018-09Department
Massachusetts Institute of Technology. Department of PhysicsJournal
Journal of Low Temperature Physics
Publisher
Springer US
ISSN
1573-7357
0022-2291