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Robertson, B, Johnson, BD, Tacchella, S, Eisenstein, DJ, Hainline, K, Arribas, S, Baker, WM, Bunker, AJ, Carniani, S, Cargile, PA, Carreira, C, Charlot, S, Chevallard, J, Curti, M, Curtis-Lake, E, D’Eugenio, F, Egami, E, Hausen, R, Helton, JM, Jakobsen, P , Ji, Z, Jones, GC, Maiolino, R, Maseda, MV, Nelson, E, Pérez-González, PG, Puskás, D, Rieke, M, Smit, R, Sun, F, Übler, H, Whitler, L, Williams, CC, Willmer, CNA, Willott, C and Witstok, J (2024) Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang. Astrophysical Journal, 970 (1). ISSN 0004-637X
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Earliest Galaxies in the JADES Origins Field Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang.pdf - Published Version Available under License Creative Commons Attribution. Download (6MB) | Preview |
Abstract
We characterize the earliest galaxy population in the JADES Origins Field, the deepest imaging field observed with JWST. We make use of ancillary Hubble Space Telescope optical images (five filters spanning 0.4-0.9 μm) and novel JWST images with 14 filters spanning 0.8−5 μm, including seven medium-band filters, and reaching total exposure times of up to 46 hr per filter. We combine all our data at >2.3 μm to construct an ultradeep image, reaching as deep as ≈31.4 AB mag in the stack and 30.3-31.0 AB mag (5σ, r = 0.″1 circular aperture) in individual filters. We measure photometric redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts z = 11.5−15. These objects show compact half-light radii of R 1/2 ∼ 50−200 pc, stellar masses of M ⋆ ∼ 107−108 M ☉, and star formation rates ∼ 0.1−1 M ☉ yr−1. Our search finds no candidates at 15 < z < 20, placing upper limits at these redshifts. We develop a forward-modeling approach to infer the properties of the evolving luminosity function without binning in redshift or luminosity that marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the impact of nondetections. We find a z = 12 luminosity function in good agreement with prior results, and that the luminosity function normalization and UV luminosity density decline by a factor of ∼2.5 from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical models for evolution of the dark matter halo mass function.
| Item Type: | Article |
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| 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 10:57 |
| Last Modified: | 20 Aug 2024 11:00 |
| DOI or ID number: | 10.3847/1538-4357/ad463d |
| URI: | https://researchonline.ljmu.ac.uk/id/eprint/23990 |
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