9 research outputs found

    Unveiling the distant Universe: Characterizing z9z\ge9 Galaxies in the first epoch of COSMOS-Web

    Full text link
    We report the identification of 15 galaxy candidates at z9z\ge9 using the initial COSMOS-Web JWST observations over 77 arcmin2^2 through four NIRCam filters (F115W, F150W, F277W, F444W) with an overlap with MIRI (F770W) of 8.7 arcmin2^2. We fit the sample using several publicly-available SED fitting and photometric redshift codes and determine their redshifts between z=9.3z=9.3 and z=10.9z=10.9 (z=10.0\langle z\rangle=10.0), UV-magnitudes between MUV_{\rm UV} = -21.2 and -19.5 (with \langle MUV=20.2_{\rm UV}\rangle=-20.2) and rest-frame UV slopes (β=2.4\langle \beta\rangle=-2.4). These galaxies are, on average, more luminous than most z9z\ge9 candidates discovered by JWST so far in the literature, while exhibiting similar blue colors in their rest-frame UV. The rest-frame UV slopes derived from SED-fitting are blue (β\beta\sim[-2.0, -2.7]) without reaching extremely blue values as reported in other recent studies at these redshifts. The blue color is consistent with models that suggest the underlying stellar population is not yet fully enriched in metals like similarly luminous galaxies in the lower redshift Universe. The derived stellar masses with log10(\langle \log_{\rm 10} (M/_\star/M)89_\odot)\rangle\approx8-9 are not in tension with the standard Λ\LambdaCDM model and our measurement of the volume density of such UV luminous galaxies aligns well with previously measured values presented in the literature at z910z\sim9-10. Our sample of galaxies, although compact, are significantly resolved.Comment: Submitted to Ap
    corecore