Fig. 2.
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Expected IGL amplitudes. Left: The mean IGL flux. Right: The IGL dipole per Eqs. (2) and (3) and assuming V = 370 km s−1. Black plus signs correspond to the entire range of magnitudes. Black, blue, green, and red circles correspond to IGL from galaxies between m1 = 25 and m0 = 18, 19, 20, 21. The IGL is integrated over the JWST latest counts (Windhorst et al. 2023) at the marked central wavelengths. The four Euclid filters are shown per Euclid Collaboration (2022a).
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