_version_ 1866917987653517312
author Kokorev, Vasily
Ortiz, Óscar A. Chávez
Taylor, Anthony J.
Finkelstein, Steven L.
Haro, Pablo Arrabal
Dickinson, Mark
Chisholm, John
Fujimoto, Seiji
Muñoz, Julian B.
Endsley, Ryan
Hu, Weida
Napolitano, Lorenzo
Wilkins, Stephen M.
Akins, Hollis B.
Amoriín, Ricardo
Casey, Caitlin M.
Cheng, Yingjie
Cleri, Nikko J.
Cole, Justin
Cullen, Fergus
Daddi, Emanuele
Davis, Kelcey
Donnan, Callum T.
Dunlop, James S.
Fernández, Vital
Giavalisco, Mauro
Grogin, Norman A.
Hathi, Nimish
Hirschmann, Michaela
Kartaltepe, Jeyhan S.
Koekemoer, Anton M.
Leung, Ho-Hin
Lucas, Ray A.
McLeod, Derek
Papovich, Casey
Pentericci, Laura
Pérez-González, Pablo G.
Somerville, Rachel S.
Wang, Xin
Yung, L. Y. Aaron
Zavala, Jorge A.
author_facet Kokorev, Vasily
Ortiz, Óscar A. Chávez
Taylor, Anthony J.
Finkelstein, Steven L.
Haro, Pablo Arrabal
Dickinson, Mark
Chisholm, John
Fujimoto, Seiji
Muñoz, Julian B.
Endsley, Ryan
Hu, Weida
Napolitano, Lorenzo
Wilkins, Stephen M.
Akins, Hollis B.
Amoriín, Ricardo
Casey, Caitlin M.
Cheng, Yingjie
Cleri, Nikko J.
Cole, Justin
Cullen, Fergus
Daddi, Emanuele
Davis, Kelcey
Donnan, Callum T.
Dunlop, James S.
Fernández, Vital
Giavalisco, Mauro
Grogin, Norman A.
Hathi, Nimish
Hirschmann, Michaela
Kartaltepe, Jeyhan S.
Koekemoer, Anton M.
Leung, Ho-Hin
Lucas, Ray A.
McLeod, Derek
Papovich, Casey
Pentericci, Laura
Pérez-González, Pablo G.
Somerville, Rachel S.
Wang, Xin
Yung, L. Y. Aaron
Zavala, Jorge A.
contents We present the first results from the CAPERS survey, utilizing PRISM observations with the JWST/NIRSpec MSA in the PRIMER-UDS field. With just 14 % of the total planned data volume, we spectroscopically confirm two new bright galaxies ($M_{\rm UV}\sim -20.4$) at redshifts $z = 10.562\pm0.034$ and $z = 11.013\pm0.028$. We examine their physical properties, morphologies, and star formation histories, finding evidence for recent bursting star formation in at least one galaxy thanks to the detection of strong (EW$_0\sim70$ A) H$γ$ emission. Combining our findings with previous studies of similarly bright objects at high-$z$, we further assess the role of stochastic star formation processes in shaping early galaxy populations. Our analysis finds that the majority of bright ($M_{\rm UV}\lesssim -20$) spectroscopically-confirmed galaxies at $z>10$ were likely observed during a starburst episode, characterized by a median SFR$_{10}$/SFR$_{100}\sim2$, although with substantial scatter. Our work also finds tentative evidence that $z>10$ galaxies are more preferentially in a bursting phase than similarly bright $z\sim6$ galaxies. We finally discuss the prospects of deeper spectroscopic observations of a statistically significant number of bright galaxies to quantify the true impact of bursting star formation on the evolution of the bright end of the ultraviolet luminosity function at these early epochs.
format Preprint
id arxiv_https___arxiv_org_abs_2504_12504
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe
Kokorev, Vasily
Ortiz, Óscar A. Chávez
Taylor, Anthony J.
Finkelstein, Steven L.
Haro, Pablo Arrabal
Dickinson, Mark
Chisholm, John
Fujimoto, Seiji
Muñoz, Julian B.
Endsley, Ryan
Hu, Weida
Napolitano, Lorenzo
Wilkins, Stephen M.
Akins, Hollis B.
Amoriín, Ricardo
Casey, Caitlin M.
Cheng, Yingjie
Cleri, Nikko J.
Cole, Justin
Cullen, Fergus
Daddi, Emanuele
Davis, Kelcey
Donnan, Callum T.
Dunlop, James S.
Fernández, Vital
Giavalisco, Mauro
Grogin, Norman A.
Hathi, Nimish
Hirschmann, Michaela
Kartaltepe, Jeyhan S.
Koekemoer, Anton M.
Leung, Ho-Hin
Lucas, Ray A.
McLeod, Derek
Papovich, Casey
Pentericci, Laura
Pérez-González, Pablo G.
Somerville, Rachel S.
Wang, Xin
Yung, L. Y. Aaron
Zavala, Jorge A.
Astrophysics of Galaxies
We present the first results from the CAPERS survey, utilizing PRISM observations with the JWST/NIRSpec MSA in the PRIMER-UDS field. With just 14 % of the total planned data volume, we spectroscopically confirm two new bright galaxies ($M_{\rm UV}\sim -20.4$) at redshifts $z = 10.562\pm0.034$ and $z = 11.013\pm0.028$. We examine their physical properties, morphologies, and star formation histories, finding evidence for recent bursting star formation in at least one galaxy thanks to the detection of strong (EW$_0\sim70$ A) H$γ$ emission. Combining our findings with previous studies of similarly bright objects at high-$z$, we further assess the role of stochastic star formation processes in shaping early galaxy populations. Our analysis finds that the majority of bright ($M_{\rm UV}\lesssim -20$) spectroscopically-confirmed galaxies at $z>10$ were likely observed during a starburst episode, characterized by a median SFR$_{10}$/SFR$_{100}\sim2$, although with substantial scatter. Our work also finds tentative evidence that $z>10$ galaxies are more preferentially in a bursting phase than similarly bright $z\sim6$ galaxies. We finally discuss the prospects of deeper spectroscopic observations of a statistically significant number of bright galaxies to quantify the true impact of bursting star formation on the evolution of the bright end of the ultraviolet luminosity function at these early epochs.
title CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2504.12504