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JWST UNCOVER: Discovery of >9 Galaxy Candidates Behind the Lensing Cluster Abell 2744

Physics

JWST UNCOVER: Discovery of >9 Galaxy Candidates Behind the Lensing Cluster Abell 2744

H. Atek, I. Chemerynska, et al.

Discover the fascinating world of high-redshift galaxy candidates as this groundbreaking research identifies 19 potential galaxies from the JWST UNCOVER survey. Conducted by esteemed authors, the study reveals significant insights into the luminosity, mass, and formation rates of these early galaxies, hinting at dramatic evolutionary trends in the universe's history.... show more
Abstract
We present the results of a search for high-redshift (z > 9) galaxy candidates in the JWST UNCOVER survey, using deep NIRCam and NIRISS imaging in 7 bands over ~45 arcmin^2 and ancillary HST observations. The NIRCam observations reach a 5-sigma limiting magnitude of ~29.2 AB. The identification of high-z candidates relies on a combination of a dropout selection and photometric redshifts. We find 16 candidates at 9 < z < 12 and 3 candidates at 12 < z < 13, eight candidates are deemed very robust. Their lensing amplification ranges from mu = 1.2 to 11.5. Candidates have a wide range of (lensing-corrected) luminosities and young ages, with low stellar masses (6.8 < log(M*/Msun) < 9.5) and low star formation rates (SFR = 0.2–7 Msun yr^-1), confirming previous findings in early JWST observations of z > 9. A few galaxies at z ~ 9–10 appear to show a clear Balmer break between the F356W and F444W/F410M bands, which helps constrain their stellar mass. We estimate blue UV continuum slopes between beta = −1.8 and −2.3, typical for early galaxies at z > 9 but not as extreme as the bluest recently discovered sources. We also find evidence for a rapid redshift evolution of the mass–luminosity relation and a redshift evolution of the UV continuum slope for a given range of intrinsic magnitude, in line with theoretical predictions. These findings suggest that deeper JWST observations are needed to reach the fainter galaxy population at those early epochs, and follow-up spectroscopy will help better constrain the physical properties and star formation histories of a larger sample of galaxies.
Publisher
MNRAS
Published On
May 08, 2023
Authors
Hakim Atek, Iryna Chemerynska, Bingjie Wang, Lukas Furtak, Andrea Weibel, Pascal Oesch, John R Weaver, Ivo Labbé, Rachel Bezanson, Pieter Van Dokkum, Adi Zitrin, Pratika Dayal, Christina C Williams, Themiya Nannayakkara, Sedona H Price, Gabriel Brammer, Andy D Goulding, Joel Leja, Danilo Marchesini, Erica J Nelson, Richard Pan, Katherine E Whitaker
Tags
high-redshift galaxies
JWST UNCOVER survey
photometric redshifts
mass-luminosity relation
UV continuum slope
early galaxy candidates
stellar evolution
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