Euclid on Sky
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Fig. 11

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Spectral response of Euclid’s imaging (VIS: IE; NISP: YE, JE, HE) and spectroscopic channels (NISP: BGE, RGE) at the beginning of the mission. The expected transmission loss at the end of the mission due to space weathering and non-volatile contamination is at most 0.05. For reference we show the Gaia G passband from their third data release (Gaia Collaboration 2023b), the atmospheric transmission for a precipitable water vapour level of 1.0 mm (Rothman et al. 2013), and some of the JWST passbands of their Near Infrared Camera (NIRCam; Rieke et al. 2005).

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