Euclid - I. Overview of the Euclid mission | Astronomy & Astrophysics (A&A)

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Fig. 22

Impact of the spacecraft orientation on the VIS background. Left: at AA = 0 considerable stray light levels are present that exceed the zodiacal background by more than one order of magnitude. Right: for AA < $- 2_{\cdot}^{\circ} 9$ $\[-2^{\circ}_\cdot9\]$ the stray light is reduced to a few percent of the zodiacal background. It still needs to be modelled for some calibrations and low-surface-brightness science.

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