Paper
16 July 2008 SPHERE baseline software for reducing calibration data
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Abstract
The Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) instrument for the VLT is designed for discovering and studying new extra-solar giant planets orbiting nearby stars by direct imaging. In this paper, we describe the philosophy behind the SPHERE baseline data processing sequences dealing with calibration observations, and how these can affect the reduction of subsequent calibrations and scientific data. Additionally, we present the result of our detector simulations and the first tests of data reduction recipe prototypes.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Markus Feldt, Ole Möller-Nilsson, Alexey I. Pavlov, Jean-Luc Beuzit, David Mouillet, Raffaele Gratton, Maud Langlois, and Franco Joos "SPHERE baseline software for reducing calibration data", Proc. SPIE 7019, Advanced Software and Control for Astronomy II, 701930 (16 July 2008); https://doi.org/10.1117/12.790337
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Cited by 1 scholarly publication.
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KEYWORDS
Sensors

Calibration

Optical spheres

Quantum efficiency

Signal detection

Astronomy

Infrared sensors

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