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The large area detector of LOFT: the Large Observatory for X-ray Timing

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conference contribution
posted on 2016-08-01, 15:11 authored by S. Zane, D. Walton, T. Kennedy, M. Feroci, J-W. Den Herder, M. Ahangarianabhari, A. Argan, P. Azzarello, G. Baldazzi, M. Barbera, D. Barret, G. Bertuccio, P. Bodin, E. Bozzo, L. Bradley, F. Cadoux, P. Cais, R. Campana, J. Coker, A. Cros, E. Del Monte, A. De Rosa, S. Di Cosimo, I. Donnarumma, Y. Evangelista, Y. Favrel, C. Feldmann, G. Fraser, F. Fuschino, M. Grassi, M. R. Hailey, R. Hudec, C. Labanti, D. Macera, P. Malcovati, M. Marisaldi, Adrian Martindale, T. Mineo, F. Muleri, M. Nowak, M. Orlandini, L. Pacciani, E. Perinati, V. Petracek, M. Pohl, A. Rachevski, P. Smith, A. Santangelo, J-Y. Seyler, C. Schmid, P. Soffitta, S. Suchy, C. Tenzer, P. Uttley, A. Vacchi, G. Zampa, N. Zampa, J. Wilms, B. Winter
LOFT (Large Observatory for X-ray Timing) is one of the five candidates that were considered by ESA as an M3 mission (with launch in 2022-2024) and has been studied during an extensive assessment phase. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black holes and neutron stars. Its pointed instrument is the Large Area Detector (LAD), a 10 m2-class instrument operating in the 2-30keV range, which holds the capability to revolutionise studies of variability from X-ray sources on the millisecond time scales. The LAD instrument has now completed the assessment phase but was not down-selected for launch. However, during the assessment, most of the trade-offs have been closed leading to a robust and well documented design that will be reproposed in future ESA calls. In this talk, we will summarize the characteristics of the LAD design and give an overview of the expectations for the instrument capabilities.

History

Citation

Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91442W

Author affiliation

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

Source

Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray, Montreal, CANADA

Version

  • AM (Accepted Manuscript)

Published in

Proc. SPIE 9144

Publisher

Society of Photo-optical Instrumentation Engineers (SPIE)

issn

0277-786X

eissn

1996-756X

Copyright date

2014

Available date

2016-08-01

Publisher version

http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1892043

Editors

Takahashi, T.;DenHerder, J. W. A.;Bautz, M.

Temporal coverage: start date

2014-06-22

Temporal coverage: end date

2014-06-26

Language

en

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