Euclid: Early Release Observations – Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions

Open Access

Fig. 5

Left: Image of Hα+[N II] emission from the galaxy NGC 1275 by CFHT. The filamentary structures show the cooling flow gas (e.g. Conselice et al. 2001). Right: Euclid I_E image. The FoV per panel is 4′ by 4′.

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