Fig. 2.
Download original image
Steps of the Euclidisation pipeline. In the top panel (a), we show the original Hubble F606W image of the galaxy cluster MACS J0416 at z = 0.396. The bottom panel (e) shows the final simulated IE band. The intermediate panels (b), (c), and (d), from top to bottom, illustrate: the convolution to match the Euclid PSF, the result of combining the Hubble F606W and F814W filters to produce the IE band, and the re-binning necessary to match the Euclid pixel scale in the IE band (see Sect. 3).
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