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Proceedings Paper

Preliminary study of the EChO data sampling and processing
Author(s): M. Farina; A. M. Di Giorgio; M. Focardi; E. Pace; G. Micela; E. Galli; G. Giusi; S. J. Liu; S. Pezzuto
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Paper Abstract

The EChO Payload is an integrated spectrometer with six different channels covering the spectral range from the visible up to the thermal infrared. A common Instrument Control Unit (ICU) implements all the instrument control and health monitoring functionalities as well as all the onboard science data processing. To implement an efficient design of the ICU on board software, separate analysis of the unit requirements are needed for the commanding and housekeeping collection as well as for the data acquisition, sampling and compression. In this work we present the results of the analysis carried out to optimize the EChO data acquisition and processing chain. The HgCdTe detectors used for EChO mission allow for non-destructive readout modes, such that the charge may be read without removing it after reading out. These modes can reduce the equivalent readout noise and the gain in signal to noise ratio can be computed using well known relations based on fundamental principles. In particular, we considered a multiaccumulation approach based on non-destructive reading of detector samples taken at equal time intervals. All detectors are periodically reset after a certain number of samples have been acquired and the length of the reset interval, as well as the number of samples and the sampling rate can be adapted to the brightness of the considered source. The estimation of the best set of parameters for the signal to noise ratio optimization and of the best sampling technique has been done by taking into account also the needs of mitigating the expected radiation effects on the acquired data. Cosmic rays can indeed be one of the major sources of data loss for a space observatory, and the studies made for the JWST mission allowed us to evaluate the actual need of the implementation of a dedicated deglitching procedure on board EChO.

Paper Details

Date Published: 28 August 2014
PDF: 9 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 914356 (28 August 2014); doi: 10.1117/12.2056269
Show Author Affiliations
M. Farina, INAF - Osservatorio Astronomico di Palermo (Italy)
INAF-Istituto di Astrofisica e Planetologia Spaziali (Italy)
A. M. Di Giorgio, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)
M. Focardi, INAF - Osservatorio Astrofisico di Arcetri (Italy)
E. Pace, Univ. degli Studi di Firenze (Italy)
G. Micela, INAF - Osservatorio Astronomico di Palermo (Italy)
E. Galli, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)
G. Giusi, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)
S. J. Liu, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)
S. Pezzuto, INAF - Istituto di Astrofisica e Planetologia Spaziali (Italy)


Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)

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