Euclid on Sky
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Fig. 1

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Colour image of the Perseus cluster released worldwide by the ESA in November 2023. It was created by combining VIS and NISP Euclid images using the IE band in the blue, YE in the green, and HE in the red. The FoV of this image is 0.5 deg2, with the x- and y-axes aligned with the Euclid camera native pixel geometry (see Fig. 13 for an equatorial projection). The three brightest galaxies are NGC 1265 (top of the image), NGC 1272, and NGC 1275 (bottom, from right to left). Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi.

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