Preliminary study of the EChO data sampling and processing

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.

[1]  Enzo Pascale,et al.  An integrated payload design for the Exoplanet Characterisation Observatory (EChO) , 2012, Other Conferences.

[2]  Karl D. Gordon,et al.  Optimal Cosmic-Ray Detection for Nondestructive Read Ramps , 2011, 1109.2626.

[3]  R. Ottensamer,et al.  The instrument control unit of the EChO space mission: electrical architecture and processing requirements , 2014, Astronomical Telescopes and Instrumentation.

[4]  E. Oliva,et al.  An improved version of the Visible and Near Infrared (VNIR) spectrometer of EChO , 2014, Astronomical Telescopes and Instrumentation.

[5]  Markus Loose,et al.  Teledyne Imaging Sensors: infrared imaging technologies for astronomy and civil space , 2008, Astronomical Telescopes + Instrumentation.

[6]  E. Pace,et al.  The Exoplanet Characterisation Observatory (EChO) payload electronics , 2012, Other Conferences.

[7]  Giusi Micela,et al.  EChO payload electronics architecture and SW design , 2015 .

[8]  P. A. R. Ade,et al.  EChO - Exoplanet Characterisation Observatory , 2010, 1112.2728.

[9]  D. J. Fixsen,et al.  Validation of Up‐the‐Ramp Sampling with Cosmic‐Ray Rejection on Infrared Detectors , 2001 .

[10]  The Open University ’ s repository of research publications and other research outputs EChO : Exoplanet characterisation observatory Journal Item , 2012 .

[11]  D. J. Fixsen,et al.  Cosmic‐Ray Rejection and Readout Efficiency for Large‐Area Arrays , 2000, astro-ph/0005486.

[12]  James D. Garnett,et al.  Multiply sampled read-limited and background-limited noise performance , 1993, Defense, Security, and Sensing.