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- W4375851657 abstract "The earliest JWST observations have revealed an unexpected abundance of super-early ($z>10$), massive ($M_*approx 10^9, M_odot$) galaxies at the bright-end ($M_{rm UV}approx -21$) of the ultraviolet luminosity function (UV LF). We present a minimal physical model that explains the observed galaxy abundance at $z=10-14$. The model primarily combines (a) the halo mass function, with (b) an obscured star formation fraction prescription that is consistent with findings of the ALMA REBELS dusty galaxy survey. It has been successfully tested on well-known UV LFs up to $z=7$. The weak evolution from $z=7$ to $zapprox 14$ of the LF bright-end arises from a conspiracy between a decreasing dust attenuation, making galaxies brighter, that almost exactly compensates for the increasing shortage of their host halos. The model also predicts that galaxies at $z > 11$ should contain negligible amounts of dust. We speculate that dust could have been efficiently ejected during the very first phases of galaxy build-up." @default.
- W4375851657 created "2023-05-10" @default.
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- W4375851657 date "2023-05-02" @default.
- W4375851657 modified "2023-10-18" @default.
- W4375851657 title "On the stunning abundance of super-early, luminous galaxies revealed by <i>JWST</i>" @default.
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- W4375851657 doi "https://doi.org/10.1093/mnras/stad1095" @default.
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