4.2 Article

Measuring a charge-coupled device point spread function Euclid visible instrument CCD273-84 PSF performance

期刊

EXPERIMENTAL ASTRONOMY
卷 39, 期 2, 页码 207-231

出版社

SPRINGER
DOI: 10.1007/s10686-015-9440-7

关键词

Astronomy; Instrumentation; CCD; PSF; Spot projection; Euclid

资金

  1. Euclid Consortium
  2. European Space Agency
  3. STFC [ST/K000977/1] Funding Source: UKRI
  4. Science and Technology Facilities Council [ST/K000977/1] Funding Source: researchfish

向作者/读者索取更多资源

In this paper we present the testing of a back-illuminated development Euclid Visible Instrument (VIS) Charge-Coupled Device (CCD) to measure the intrinsic CCD Point Spread Function (PSF) characteristics using a novel modelling technique. We model the optical spot projection system and the CCD273-84 PSF jointly. We fit a model using Bayesian posterior probability density function, sampling to all available data simultaneously. The generative model fitting is shown, using simulated data, to allow good parameter estimations even when these data are not well sampled. Using available spot data we characterise a CCD273-84 PSF as a function of wavelength and intensity. The CCD PSF kernel size was found to increase with increasing intensity and decreasing wavelength.

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