Share Email Print
cover

Proceedings Paper

The on-board data handling concept for the LOFT large area detector
Author(s): S. Suchy; P. Uter; C. Tenzer; A. Santangelo; A. Argan; M. Feroci; T. E. Kennedy; P. J. Smith; D. Walton; S. Zane; J. Portell; E. García-Berro
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The Large Observatory for X-ray Timing (LOFT) is one of the four candidate ESA M3 missions considered for launch in the timeframe of 2022. It is specifically designed to perform fast X-ray timing and probe the status of the matter near black holes and neutron stars. The LOFT scientific payload consists of a Large Area Detector and a Wide Field Monitor. The LAD is a 10m2-class pointed instrument with high spectral (200 eV @ 6 keV) and timing (< 10 μs) resolution over the 2-80 keV range. It is designed to observe persistent and transient X-ray sources with a very large dynamic range from a few mCrab up to an intensity of 15 Crab. An unprecedented large throughput (~280.000 cts/s from the Crab) is achieved with a segmented detector, making pile-up and dead-time, often worrying or limiting focused experiments, secondary issues. We present the on-board data handling concept that follows the highly segmented and hierarchical structure of the instrument from the front-end electronics to the on-board software. The system features customizable observation modes ranging from event-by-event data for sources below 0.5 Crab to individually adjustable time resolved spectra for the brighter sources. On-board lossless data compression will be applied before transmitting the data to ground.

Paper Details

Date Published: 17 September 2012
PDF: 12 pages
Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 84435M (17 September 2012); doi: 10.1117/12.925663
Show Author Affiliations
S. Suchy, Institut für Astronomie and Astrophysik, Univ. Tübingen (Germany)
P. Uter, Institut für Astronomie and Astrophysik, Univ. Tübingen (Germany)
C. Tenzer, Institut für Astronomie and Astrophysik, Univ. Tübingen (Germany)
A. Santangelo, Institut für Astronomie and Astrophysik, Univ. Tübingen (Germany)
A. Argan, INAF HQ (Italy)
M. Feroci, INAF/IASF Roma (Italy)
T. E. Kennedy, Mullard Space Science Lab., Univ. College London (United Kingdom)
P. J. Smith, Mullard Space Science Lab., Univ. College London (United Kingdom)
D. Walton, Mullard Space Science Lab., Univ. College London (United Kingdom)
S. Zane, Mullard Space Science Lab., Univ. College London (United Kingdom)
J. Portell, Institute for Space Studies of Catalonia (Spain)
Univ. of Barcelona (Spain)
E. García-Berro, Institute for Space Studies of Catalonia (Spain)
Univ. Politècnica de Catalunya (Spain)


Published in SPIE Proceedings Vol. 8443:
Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Stephen S. Murray; Jan-Willem A. den Herder, Editor(s)

© SPIE. Terms of Use
Back to Top