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Hainline, KN, Johnson, BD, Robertson, B, Tacchella, S, Helton, JM, Sun, F, Eisenstein, DJ, Simmonds, C, Topping, MW, Whitler, L, Willmer, CNA, Rieke, M, Suess, KA, Hviding, RE, Cameron, AJ, Alberts, S, Baker, WM, Baum, S, Bhatawdekar, R, Bonaventura, N , Boyett, K, Bunker, AJ, Carniani, S, Charlot, S, Chevallard, J, Chen, Z, Curti, M, Curtis-Lake, E, D’Eugenio, F, Egami, E, Endsley, R, Hausen, R, Ji, Z, Looser, TJ, Lyu, J, Maiolino, R, Nelson, E, Puskás, D, Rawle, T, Sandles, L, Saxena, A, Smit, R, Stark, DP, Williams, CC, Willott, C and Witstok, J (2024) The Cosmos in Its Infancy: JADES Galaxy Candidates at z >8 in GOODS-S and GOODS-N. Astrophysical Journal, 964 (1). p. 71. ISSN 0004-637X
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The Cosmos in Its Infancy JADES Galaxy Candidates at z 8 in GOODSS and GOODSN.pdf - Published Version Available under License Creative Commons Attribution. Download (4MB) | Preview |
Abstract
We present a catalog of 717 candidate galaxies at z > 8 selected from 125 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 zphot ∼ 18. Over 93% of the sources are newly identified from our deep JADES imaging, including 31 new galaxy candidates at zphot > 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 〈Δz = zphot − zspec〉 = 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.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | 0201 Astronomical and Space Sciences; 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics; 0306 Physical Chemistry (incl. Structural); Astronomy & Astrophysics |
| Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: | Astrophysics Research Institute |
| Publisher: | American Astronomical Society |
| SWORD Depositor: | A Symplectic |
| Date Deposited: | 20 Aug 2024 11:58 |
| Last Modified: | 20 Aug 2024 12:00 |
| DOI or ID number: | 10.3847/1538-4357/ad1ee4 |
| URI: | https://researchonline.ljmu.ac.uk/id/eprint/23994 |
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