Micro-X Sounding Rocket: Transitioning from First Flight to a Dark Matter Configuration

J. S. Adams, A. J. Anderson, R. Baker, S. R. Bandler, N. Bastidon, D. Castro, M. E. Danowski, W. B. Doriese, M. E. Eckart, E. Figueroa-Feliciano, D. C. Goldfinger, S. N.T. Heine, G. C. Hilton, A. J.F. Hubbard*, R. L. Kelley, C. A. Kilbourne, R. E. Manzagol-Harwood, D. McCammon, T. Okajima, F. S. PorterC. D. Reintsema, P. Serlemitsos, S. J. Smith, P. Wikus

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

The Micro-X sounding rocket flew for the first time on July 22, 2018, becoming the first program to fly Transition-Edge Sensors and multiplexing SQUID readout electronics in space. While a rocket pointing failure led to no time on-target, the success of the flight systems was demonstrated. The successful flight operation of the instrument puts the program in a position to modify the payload for indirect galactic dark matter searches. The payload modifications are motivated by the science requirements of this observation. Micro-X can achieve world-leading sensitivity in the keV regime with a single flight. Dark matter sensitivity projections have been updated to include recent observations and the expected sensitivity of Micro-X to these observed fluxes. If a signal is seen (as seen in the X-ray satellites), Micro-X can differentiate an atomic line from a dark matter signature.

Original languageEnglish (US)
Pages (from-to)1072-1081
Number of pages10
JournalJournal of Low Temperature Physics
Volume199
Issue number3-4
DOIs
StatePublished - May 1 2020

Keywords

  • Dark matter
  • Sounding rocket
  • Sterile neutrino
  • TES
  • X-ray

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics
  • Materials Science(all)
  • Condensed Matter Physics

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