%0 Generic %1 finkelstein2021census %A Finkelstein, Steven L. %A Bagley, Micaela %A Song, Mimi %A Larson, Rebecca %A Papovich, Casey %A Dickinson, Mark %A Finkelstein, Keely %A Koekemoer, Anton M. %A Pirzkal, Norbert %A Somerville, Rachel S. %A Yung, L. Y. Aaron %A Behroozi, Peter %A Ferguson, Harry %A Giavalisco, Mauro %A Grogin, Norman %A Hathi, Nimish %A Hutchison, Taylor %A Jung, Intae %A Kocevski, Dale %A Kawinwanichakij, Lalitwadee %A Rojas-Ruiz, Sofia %A Ryan Jr., Russell %A Snyder, Gregory F. %A Tacchella, Sandro %D 2021 %K library %T A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields %U http://arxiv.org/abs/2106.13813 %X We present the results from a new search for candidate galaxies at z ~ 8.5-11 discovered over the 850 arcmin^2 area probed by the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS). We use a photometric redshift selection including both Hubble and Spitzer Space Telescope photometry to robustly identify galaxies in this epoch at F160W < 26.6. We use a detailed vetting procedure, including screening for persistence, stellar contamination, inclusion of ground-based imaging, and followup space-based imaging to build a robust sample of 11 candidate galaxies, three presented here for the first time. The inclusion of Spitzer/IRAC photometry in the selection process reduces contamination, and yields more robust redshift estimates than Hubble alone. We constrain the evolution of the rest-frame ultraviolet luminosity function via a new method of calculating the observed number densities without choosing a prior magnitude bin size. We find that the abundance at our brightest probed luminosities (M_UV=-22.3) is consistent with predictions from simulations which assume that galaxies in this epoch have gas depletion times at least as short as those in nearby starburst galaxies. Due to large Poisson and cosmic variance uncertainties we cannot conclusively rule out either a smooth evolution of the luminosity function continued from z=4-8, or an accelerate decline at z > 8. We calculate that the presence of seven galaxies in a single field (EGS) is an outlier at the 2-sigma significance level, implying the discovery of a significant overdensity. These scenarios will be imminently testable to high confidence within the first year of observations of the James Webb Space Telescope.

@misc{finkelstein2021census, abstract = {We present the results from a new search for candidate galaxies at z ~ 8.5-11 discovered over the 850 arcmin^2 area probed by the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS). We use a photometric redshift selection including both Hubble and Spitzer Space Telescope photometry to robustly identify galaxies in this epoch at F160W < 26.6. We use a detailed vetting procedure, including screening for persistence, stellar contamination, inclusion of ground-based imaging, and followup space-based imaging to build a robust sample of 11 candidate galaxies, three presented here for the first time. The inclusion of Spitzer/IRAC photometry in the selection process reduces contamination, and yields more robust redshift estimates than Hubble alone. We constrain the evolution of the rest-frame ultraviolet luminosity function via a new method of calculating the observed number densities without choosing a prior magnitude bin size. We find that the abundance at our brightest probed luminosities (M_UV=-22.3) is consistent with predictions from simulations which assume that galaxies in this epoch have gas depletion times at least as short as those in nearby starburst galaxies. Due to large Poisson and cosmic variance uncertainties we cannot conclusively rule out either a smooth evolution of the luminosity function continued from z=4-8, or an accelerate decline at z > 8. We calculate that the presence of seven galaxies in a single field (EGS) is an outlier at the 2-sigma significance level, implying the discovery of a significant overdensity. These scenarios will be imminently testable to high confidence within the first year of observations of the James Webb Space Telescope.}, added-at = {2021-06-29T07:13:25.000+0200}, author = {Finkelstein, Steven L. and Bagley, Micaela and Song, Mimi and Larson, Rebecca and Papovich, Casey and Dickinson, Mark and Finkelstein, Keely and Koekemoer, Anton M. and Pirzkal, Norbert and Somerville, Rachel S. and Yung, L. Y. Aaron and Behroozi, Peter and Ferguson, Harry and Giavalisco, Mauro and Grogin, Norman and Hathi, Nimish and Hutchison, Taylor and Jung, Intae and Kocevski, Dale and Kawinwanichakij, Lalitwadee and Rojas-Ruiz, Sofia and Ryan Jr., Russell and Snyder, Gregory F. and Tacchella, Sandro}, biburl = {https://www.bibsonomy.org/bibtex/243b34ba7e095c059979368d2fa32bced/gpkulkarni}, description = {A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields}, interhash = {7a55d80692ee92d781d64cd6dac6184a}, intrahash = {43b34ba7e095c059979368d2fa32bced}, keywords = {library}, note = {cite arxiv:2106.13813Comment: 47 figures, 25 pages, 10 tables, submitted to the Astrophysical Journal}, timestamp = {2021-06-29T07:13:25.000+0200}, title = {A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields}, url = {http://arxiv.org/abs/2106.13813}, year = 2021 }