Fig. 1.

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Some examples of the SED fitting performed with Cigale on the galaxies included in the highest redshift bin. The squares indicate the photometric points from JWST, A3COSMOS and the 870 μm from the deblending of the S2COSMOS maps by Simpson et al. (2019). The circular points report the ancillary photometry from HSC, VISTA, Spitzer, and from the super-deblending of the Herschel Maps. The inset shows the Gaussianized p(z) computed with Cigale. The top row shows the cutouts (3 arcsec side) in the NIRCam and MIRI filters of COSMOS-Web.
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