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The Microchannel X-ray Telescope for the Gamma-Ray Burst mission SVOM

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journal contribution
posted on 2016-04-19, 08:53 authored by D. Goetz, J. Osborne, B. Cordier, Julian Paul Paul, Philip Andrew Evans, Andrew Paul Beardmore, Adrian Martindale, Richard Willingale, Paul Thomas O'Brien, S. Basa, C. Rossin, O. Godet, N. Webb, J. Greiner, K. Nandra, N. Meidinger, E. Perinati, A. Satangelo, K. Mercier, F. Gonzalez
We present the Microchannel X-ray Telescope, a new light and compact focussing telescope that will be ying on the Sino-French SVOM mission dedicated to Gamma-Ray Burst science. The MXT design is based on the coupling of square pore micro-channel plates with a low noise pnCCD. MXT will provide an effective area of about 50 cm2, and its point spread function is expected to be better than 3.7 arc min (FWHM) on axis. The estimated sensitivity is adequate to detect all the afterglows of the SVOM GRBs, and to localize them to better then 60 arc sec after five minutes of observation. © (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.

History

Citation

Proceedings of SPIE 9144, Space Telescopes And Instrumentation 2014: Ultraviolet To Gamma Ray, 2014, 914423

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • AM (Accepted Manuscript)

Published in

Proceedings of SPIE 9144

Publisher

Society of Photo-optical Instrumentation Engineers (SPIE)

issn

0277-786X

eissn

1996-756X

Copyright date

2014

Available date

2016-04-19

Publisher version

http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1892364

Editors

Takahashi, T;DenHerder, JWA;Bautz, M

Language

en

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