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The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST and ground-based near-infrared imaging
DOI: 10.1093/mnras/stac3472 Bibcode: 2023MNRAS.518.6011D

Moneti, A.; Bowler, R. A. A.; Cullen, F. +11 more

We reduce and analyse the available JWST ERO and ERS NIRCam imaging (SMACS0723, GLASS, CEERS) in combination with the latest deep ground-based near-infrared imaging in the COSMOS field (provided by UltraVISTA DR5) to produce a new measurement of the evolving galaxy UV luminosity function (LF) over the redshift range z = 8 - 15. This yields a new e…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 380
Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field
DOI: 10.1093/mnras/stac3347 Bibcode: 2023MNRAS.518.4755A

Verma, A.; Conselice, C. J.; Adams, N. J. +8 more

We present a reduction and analysis of the James Webb Space Telescope (JWST) SMACS 0723 field using new post-launch calibrations to conduct a search for ultra-high-redshift galaxies (z > 9) present within the Epoch of Reionization. We conduct this search by modelling photometric redshifts in several ways for all sources and by applying conserva…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 251
Revealing galaxy candidates out to z 16 with JWST observations of the lensing cluster SMACS0723
DOI: 10.1093/mnras/stac3144 Bibcode: 2023MNRAS.519.1201A

Charlot, Stéphane; Chevallard, Jacopo; Mahler, Guillaume +8 more

One of the main goals of the JWST is to study the first galaxies in the Universe. We present a systematic photometric analysis of very distant galaxies in the first JWST deep field towards the massive lensing cluster SMACS0723. As a result, we report the discovery of two galaxy candidates at z ~ 16, only 250 million years after the big bang. We al…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 213
A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z 7-8 galaxies
DOI: 10.1093/mnras/stad1919 Bibcode: 2023MNRAS.524.2312E

Charlot, Stéphane; Chisholm, John; Chen, Zuyi +5 more

Spitzer/Infrared Array Camera (IRAC) imaging has revealed that the brightest z ~ 7-8 galaxies often exhibit young ages and strong nebular line emission, hinting at high ionizing efficiency among early galaxies. However, IRAC's limited sensitivity has long hindered efforts to study the fainter, more numerous population often thought largely respons…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 199
JWST/NIRSpec spectroscopy of z = 7-9 star-forming galaxies with CEERS: new insight into bright Lyα emitters in ionized bubbles
DOI: 10.1093/mnras/stad2763 Bibcode: 2023MNRAS.526.1657T

Charlot, Stéphane; Chen, Zuyi; Tang, Mengtao +9 more

We describe new JWST/NIRSpec observations of galaxies at z ≳ 7 taken from the CEERS survey. Previous observations of this area have revealed associations of Lyα emitters at redshifts (z = 7.5, 7.7, and 8.7) where the intergalactic medium (IGM) is thought to be mostly neutral, leading to suggestions that these systems are situated in large ionized …

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 174
Evolution of the UV LF from z 15 to z 8 using new JWST NIRCam medium-band observations over the HUDF/XDF
DOI: 10.1093/mnras/stad1145 Bibcode: 2023MNRAS.523.1036B

van Dokkum, Pieter G.; Illingworth, Garth D.; Brammer, Gabriel +7 more

We present the first constraints on the prevalence of z > 10 galaxies in the Hubble Ultra Deep Field (HUDF) leveraging new NIRCam observations from JEMS (JWST Extragalactic Medium-band Survey). These NIRCam observations probe redward of 1.6 µm, beyond the wavelength limit of HST, allowing us to search for galaxies to z > 10. These obse…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 148
A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
DOI: 10.1093/mnras/stad369 Bibcode: 2023MNRAS.520.3974C

Cullen, F.; McLure, R. J.; Dunlop, J. S. +9 more

We report a robust sample of 10 massive quiescent galaxies at redshift, z > 3, selected using the first data from the JWST Cosmic Evolution Early Release Science programme. Three of these galaxies are at 4 < z < 5, constituting the best evidence to date for quiescent galaxies significantly before z = 4. These extreme galaxies have stellar…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 132
Unveiling the nature of infrared bright, optically dark galaxies with early JWST data
DOI: 10.1093/mnras/stad947 Bibcode: 2023MNRAS.522..449B

Brammer, G.; Oesch, P. A.; van Dokkum, P. +18 more

Over the last few years, both Atacama Large Millimeter/submillimeter Array (ALMA) and Spitzer observations have revealed a population of likely massive galaxies at z > 3 that was too faint to be detected inHubble Space Telescope(HST) rest-frame ultraviolet imaging. However, due to the very limited photometry for individual galaxies, the true na…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 112
The MillenniumTNG project: the galaxy population at z ≥ 8
DOI: 10.1093/mnras/stac3743 Bibcode: 2023MNRAS.524.2594K

Springel, Volker; Hernquist, Lars; Pakmor, Rüdiger +11 more

The early release science results from JWST have yielded an unexpected abundance of high-redshift luminous galaxies that seems to be in tension with current theories of galaxy formation. However, it is currently difficult to draw definitive conclusions form these results as the sources have not yet been spectroscopically confirmed. It is in any ca…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 104
Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times
DOI: 10.1093/mnras/stad004 Bibcode: 2023MNRAS.519.5859W

Charlot, Stéphane; Chevallard, Jacopo; Stark, Daniel P. +3 more

The variety of star formation histories (SFHs) of z ≳ 6 galaxies provides important insights into early star formation, but has been difficult to systematically quantify. Some observations suggest that many z ~ 6-9 galaxies are dominated by ≳200 Myr stellar populations, implying significant star formation at z ≳ 9, while others find that most reio…

2023 Monthly Notices of the Royal Astronomical Society
eHST 103