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COSMOS-Web: Intrinsically Luminous z$\gtrsim$10 Galaxy Candidates Test Early Stellar Mass Assembly

Authors :
Casey, Caitlin M.
Akins, Hollis B.
Shuntov, Marko
Ilbert, Olivier
Paquereau, Louise
Franco, Maximilien
Hayward, Christopher C.
Finkelstein, Steven L.
Boylan-Kolchin, Michael
Robertson, Brant E.
Allen, Natalie
Brinch, Malte
Cooper, Olivia R.
Ding, Xuheng
Drakos, Nicole E.
Faisst, Andreas L.
Fujimoto, Seiji
Gillman, Steven
Harish, Santosh
Hirschmann, Michaela
Jin, Shuowen
Kartaltepe, Jeyhan S.
Koekemoer, Anton M.
Kokorev, Vasily
Liu, Daizhong
Long, Arianna S.
Magdis, Georgios
Maraston, Claudia
Martin, Crystal L.
McCracken, Henry Joy
McKinney, Jed
Mobasher, Bahram
Rhodes, Jason
Rich, R. Michael
Sanders, David B.
Silverman, John D.
Toft, Sune
Vijayan, Aswin P.
Weaver, John R.
Wilkins, Stephen M.
Yang, Lilan
Zavala, Jorge A.
Casey, Caitlin M.
Akins, Hollis B.
Shuntov, Marko
Ilbert, Olivier
Paquereau, Louise
Franco, Maximilien
Hayward, Christopher C.
Finkelstein, Steven L.
Boylan-Kolchin, Michael
Robertson, Brant E.
Allen, Natalie
Brinch, Malte
Cooper, Olivia R.
Ding, Xuheng
Drakos, Nicole E.
Faisst, Andreas L.
Fujimoto, Seiji
Gillman, Steven
Harish, Santosh
Hirschmann, Michaela
Jin, Shuowen
Kartaltepe, Jeyhan S.
Koekemoer, Anton M.
Kokorev, Vasily
Liu, Daizhong
Long, Arianna S.
Magdis, Georgios
Maraston, Claudia
Martin, Crystal L.
McCracken, Henry Joy
McKinney, Jed
Mobasher, Bahram
Rhodes, Jason
Rich, R. Michael
Sanders, David B.
Silverman, John D.
Toft, Sune
Vijayan, Aswin P.
Weaver, John R.
Wilkins, Stephen M.
Yang, Lilan
Zavala, Jorge A.
Publication Year :
2023

Abstract

We report the discovery of 15 exceptionally luminous $10\lesssim z\lesssim14$ candidate galaxies discovered in the first 0.28 deg$^2$ of JWST/NIRCam imaging from the COSMOS-Web Survey. These sources span rest-frame UV magnitudes of $-20.5>M_{\rm UV}>-22$, and thus constitute the most intrinsically luminous $z\gtrsim10$ candidates identified by JWST to-date. Selected via NIRCam imaging with Hubble ACS/F814W, deep ground-based observations corroborate their detection and help significantly constrain their photometric redshifts. We analyze their spectral energy distributions using multiple open-source codes and evaluate the probability of low-redshift solutions; we conclude that 12/15 (80%) are likely genuine $z\gtrsim10$ sources and 3/15 (20%) likely low-redshift contaminants. Three of our $z\sim12$ candidates push the limits of early stellar mass assembly: they have estimated stellar masses $\sim5\times10^{9}\,M_\odot$, implying an effective stellar baryon fraction of $\epsilon_{\star}\sim0.2-0.5$, where $\epsilon_{\star}\equiv M_{\star}/(f_{b}M_{halo})$. The assembly of such stellar reservoirs is made possible due to rapid, burst-driven star formation on timescales $<$100\,Myr where the star-formation rate may far outpace the growth of the underlying dark matter halos. This is supported by the similar volume densities inferred for $M_\star\sim10^{10}\,M_\odot$ galaxies relative to $M_\star\sim10^{9}\,M_\odot$ -- both about $10^{-6}$ Mpc$^{-3}$ -- implying they live in halos of comparable mass. At such high redshifts, the duty cycle for starbursts would be of order unity, which could cause the observed change in the shape of the UVLF from a double powerlaw to Schechter at $z\approx8$. Spectroscopic redshift confirmation and ensuing constraints of their masses will be critical to understanding how, and if, such early massive galaxies push the limits of galaxy formation in $\Lambda$CDM.<br />Comment: 30 pages, 9 figures; ApJ submitted

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1405318255
Document Type :
Electronic Resource