The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N

The Cosmos in Its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-N

Mar 18, 2024·
Kevin N. Hainline
,
Benjamin D. Johnson
,
Brant Robertson
,
Sandro Tacchella
Jakob M. Helton
Jakob M. Helton
,
Fengwu Sun
,
Daniel J. Eisenstein
,
Charlotte Simmonds
,
Michael W. Topping
,
Lily Whitler
,
Christopher N. A. Willmer
,
Marcia Rieke
,
Katherine A. Suess
,
Raphael E. Hviding
,
Alex J. Cameron
,
Stacey Alberts
,
William M. Baker
,
Stefi Baum
,
Rachana Bhatawdekar
,
Nina Bonaventura
,
Kristan Boyett
,
Andrew J. Bunker
,
Stefano Carniani
,
Stephane Charlot
,
Jacopo Chevallard
,
Zuyi Chen
,
Mirko Curti
,
Emma Curtis-Lake
,
Francesco D'Eugenio
,
Eiichi Egami
,
Ryan Endsley
,
Ryan Hausen
,
Zhiyuan Ji
,
Tobias J. Looser
,
Jianwei Lyu
,
Roberto Maiolino
,
Erica Nelson
,
Dávid Puskás
,
Tim Rawle
,
Lester Sandles
,
Aayush Saxena
,
Renske Smit
,
Daniel P. Stark
,
Christina C. Williams
,
Chris Willott
,
Joris Witstok
Abstract
We present a catalog of $717$ candidate galaxies at $z > 8$ selected from $125\ \mathrm{square\ arcmin}$ of NIRCam imaging as part of the JWST Advanced Deep Extragalactic Survey (JADES). We combine the full JADES imaging data set with data from the JWST Extragalactic Medium Survey and First Reionization Epoch Spectroscopic COmplete Survey (FRESCO) along with extremely deep existing observations from Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) for a final filter set that includes $15$ JWST/NIRCam filters and five HST/ACS filters. The high-redshift galaxy candidates were selected from their estimated photometric redshifts calculated using a template-fitting approach, followed by visual inspection from seven independent reviewers. We explore these candidates in detail, highlighting interesting resolved or extended sources, sources with very red long-wavelength slopes, and our highest-redshift candidates, which extend to $z_{\mathrm{phot}} \sim 18$ . Over $93\%$ of the sources are newly identified from our deep JADES imaging, including $31$ new galaxy candidates at $z_{\mathrm{phot}} > 12$ . We also investigate potential contamination by stellar objects, and do not find strong evidence from spectral energy distribution fitting that these faint high-redshift galaxy candidates are low-mass stars. Using $42$ sources in our sample with measured spectroscopic redshifts from NIRSpec and FRESCO, we find excellent agreement to our photometric redshift estimates, with no catastrophic outliers and an average difference of $\langle \Delta z \rangle = \langle z_{\mathrm{phot}} - z_{\mathrm{spec}} \rangle = 0.26$ . These sources comprise one of the most robust samples for probing the early buildup of galaxies within the first few hundred million years of the Universe’s history.
Type
Publication
The Astrophysical Journal, Volume 964, Issue 1, id.71, 35 pages