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Sub-Pixel Response Measurement of Near-Infrared Sensors

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arxiv astro-ph/0611339 v1 pith:LVPVK46H submitted 2006-11-10 astro-ph

classification astro-ph
keywords near-infraredsub-pixelinstrumentslargephotometryprecisionresponsesystem
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Wide-field survey instruments are used to efficiently observe large regions of the sky. To achieve the necessary field of view, and to provide a higher signal-to-noise ratio for faint sources, many modern instruments are undersampled. However, precision photometry with undersampled imagers requires a detailed understanding of the sensitivity variations on a scale much smaller than a pixel. To address this, a near-infrared spot projection system has been developed to precisely characterize near-infrared focal plane arrays and to study the effect of sub-pixel non uniformity on precision photometry. Measurements of large format near-infrared detectors demonstrate the power of this system for understanding sub-pixel response.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. ExoSim 2: the new Exoplanet Observation Simulator applied to the Ariel space mission

    astro-ph.IM 2025-01 conditional novelty 6.0 of 10

    ExoSim 2 is a modular, publicly available rewrite of the Exoplanet Observation Simulator that produces time-resolved focal planes, jittered sub-exposures, and noisy non-destructive reads for Ariel-like observations.

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