The on-board calibration system of the X-ray Imaging Polarimetry Explorer (XIPE)

Authors
  • S. Zane
  • B. Winter
  • C. Theobald
  • T. Theodorou
  • M. Pinchera
  • F. Muleri
  • F. Spada
  • C. Sgro
  • D. Zanetti
  • H. Feng
  • E. del Monte
  • A. Rubini
  • P. Soffitta
  • R. Bellazzini
  • E. Bozzo
  • V. Burwitz
  • A.J. Castro Tirado
  • E. Costa
  • S. Gburek
  • R. Goosmann
  • V. Karas
  • G. Matt
  • K. Nandra
  • M. Pearce
  • J. Poutanen
  • V. Reglero
  • M.D. Sabau
  • A. Santangelo
  • G. Tagliaferri
  • C. Tenzer
  • J. Vink
  • M. Weisskopf
Publication date 2016
Host editors
  • J.-W.A. den Herder
  • T. Takahashi
  • M. Bautz
Book title Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Book subtitle 26 June-1 July 2016, Edinburgh, United Kingdom
ISBN
  • 9781510601895
ISBN (electronic)
  • 9781510601901
Series Proceedings of SPIE
Event Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Article number 99054H
Volume | Issue number 2
Number of pages 15
Publisher Bellingham, WA: SPIE
Abstract
The calibration system for XIPE is aimed at providing a way to check and correct possible variations of performance of the Gas Pixel Detector during the three years of operation in orbit (plus two years of possible extended operation), while facilitating the observation of the celestial sources. This will be performed by using a filter wheel with a large heritage having a set of positions for the calibration and the observation systems. In particular, it will allow for correcting possible gain variation, for measuring the modulation factor using a polarized source, for removing non interesting bright sources in the field of view and for observing very bright celestial sources. The on-board calibration system is composed of three filter wheels, one for each detector and it is expected to operate for a small number of times during the year. Moreover, since it operates once at a time, within the observation mode, it allows for simultaneous calibration and acquisition from celestial sources on different detectors. In this paper we present the scope and the requirements of the on-board calibration system, its design, and a description of its possible use in space.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.2233448
Other links http://adsabs.harvard.edu/abs/2016SPIE.9905E..4HZ
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