Identification and properties of intense star-forming galaxies at redshifts z > 10

Identification and properties of intense star-forming galaxies at redshifts z > 10

Apr 4, 2023·
Brant E. Robertson
,
Sandro Tacchella
,
Benjamin D. Johnson
,
Kevin Hainline
,
Lily Whitler
,
Daniel J. Eisenstein
,
Ryan Endsley
,
Marcia Rieke
,
Daniel P. Stark
,
Stacey Alberts
,
Alan Dressler
,
Eiichi Egami
,
Ryan Hausen
,
George Rieke
,
Irene Shivaei
,
Christina C. Williams
,
Christopher N. A. Willmer
,
Santiago Arribas
,
Nina Bonaventura
,
Andrew Bunker
,
Alex J. Cameron
,
Stefano Carniani
,
Stéphane Charlot
,
Jacopo Chevallard
,
Mirko Curti
,
Emma Curtis-Lake
,
Francesco D'Eugenio
,
Peter Jakobsen
,
Tobias J. Looser
,
Nora Lützgendorf
,
Roberto Maiolino
,
Michael v. Maseda
,
Tim Rawle
,
Hans-Walter Rix
,
Renske Smit
,
Hannah Übler
,
Chris Willott
,
Joris Witstok
,
Stefi Baum
,
Rachana Bhatawdekar
,
Kristan Boyett
,
Zuyi Chen
,
Anna De Graaff
,
Michael Florian
Jakob M. Helton
Jakob M. Helton
,
Raphael E. Hviding
,
Zhiyuan Ji
,
Nimisha Kumari
,
Jianwei Lyu
,
Erica Nelson
,
Lester Sandles
,
Aayush Saxena
,
Katherine A. Suess
,
Fengwu Sun
,
Michael Topping
,
Imaan E. B. Wallace
Abstract
Surveys with the James Webb Space Telescope (JWST) have discovered candidate galaxies in the first $400$ Myr of cosmic time. Preliminary indications have suggested these candidate galaxies may be more massive and abundant than previously thought. However, without confirmed distances, their inferred properties remain uncertain. Here we identify four galaxies located in the JWST Advanced Deep Extragalactic Survey Near-Infrared Camera imaging with photometric redshifts $z$ of roughly $10-13$ . These galaxies include the first redshift $z > 12$ systems discovered with distances spectroscopically confirmed by JWST in a companion paper. Using stellar population modelling, we find the galaxies typically contain $100$ million solar masses in stars, in stellar populations that are less than $100$ million years old. The moderate star-formation rates and compact sizes suggest elevated star-formation rate surface densities, a key indicator of their formation pathways. Taken together, these measurements show that the first galaxies contributing to cosmic reionization formed rapidly and with intense internal radiation fields.
Type
Publication
Nature Astronomy, Volume 7, pages 611-621