2102.07775.pdf (1.49 MB)
New determinations of the UV luminosity functions from z ~ 9 to 2 show a remarkable consistency with halo growth and a constant star formation efficiency
journal contribution
posted on 2023-06-10, 06:53 authored by R J Bouwens, P A Oesch, M Stefanon, G Illingworth, I Labbé, N Reddy, H Atek, M Montes, R Naidu, T Nanayakkara, E Nelson, Stephen WilkinsStephen WilkinsHere we provide the most comprehensive determinations of the rest-frame UV luminosity function (LF) available to date with the Hubble Space Telescope (HST) at z ~ 2-9. Essentially all of the noncluster extragalactic legacy fields are utilized, including the Hubble Ultra Deep Field, the Hubble Frontier Fields parallel fields, and all five CANDELS fields, for a total survey area of 1136 arcmin2. Our determinations include galaxies at z ~ 2-3 leveraging the deep HDUV, UVUDF, and ERS WFC3/UVIS observations available over an ~150 arcmin2 area in the GOODS-North and GOODS-South regions. All together, our collective samples include >24,000 sources, >2.3 larger than previous selections with HST. We identify 5766, 6332, 7240, 3449, 1066, 601, 246, and 33 sources at z ~ 2, 3, 4, 5, 6, 7, 8, and 9, respectively. Combining our results with an earlier z ~ 10 LF determination by Oesch et al., we quantify the evolution of the UV LF. Our results indicate that there is (1) a smooth flattening of the faint-end slope a from a ~ -2.4 at z ~ 10 to a ~ -1.5 at z ~ 2, (2) minimal evolution in the characteristic luminosity M* at z = 2.5, and (3) a monotonic increase in the normalization from z ~ 10 to 2, which can be well described by a simple second-order polynomial, consistent with an "accelerated"evolution scenario. We find that each of these trends (from z ~ 10 to 2.5 at least) can be readily explained on the basis of the evolution of the halo mass function and a simple constant star formation efficiency model.
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- Published
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- Accepted version
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Astronomical JournalISSN
0004-6256Publisher
American Astronomical SocietyExternal DOI
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162Page range
a47 1-18Department affiliated with
- Physics and Astronomy Publications
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- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2023-04-24First Open Access (FOA) Date
2023-05-02First Compliant Deposit (FCD) Date
2023-04-21Usage metrics
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