Galaxies in the First Billion Years After the Big Bang

By D. Stark. 2016

201 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/f8e2dbf45fb794390af2c6a65dfc9397e64f5047

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Citations in the corpus

Dust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy (2017, methodology): “…demographics analyzed through photometric data from HST and the Spitzer Space Telescope, spectroscopic diagnostics are being gathered to gauge the nature of their stellar populations and their capability for releasing the necessary number of ionizing photons (for a recent review see Stark 2016).”
Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era (2018, background): “…(Planck Collaboration et al. 2018), and the latest Hubble Space Telescope (HST) surveys have revealed more than a hundred candidate z8 Lyman break galaxies (LBGs, e.g., Bouwens et al. 2015; Ishigaki et al. 2018; see Stark 2016 for a review) out to = - +z 11.1 0.12 0.08 (Oesch et al. 2016).”
JADES Initial Data Release for the Hubble Ultra Deep Field: Revealing the Faint Infrared Sky with Deep JWST NIRCam Imaging (2023, background): “In addition, for galaxies at z spec > 5, Spitzer / IRAC colors revealed that galaxies have very high equivalent width emission lines ( e.g., Smit et al. 2014, 2015; Roberts-Borsani et al. 2016; Stark 2016 ) , which improve photometric redshifts signi ﬁ cantly when properly included in templates.”
CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST (2022, background): “The epoch of reionization marks the period when energetic photons (presumably from massive stars in early galaxies; e.g., Stark 2016; Finkelstein et al. 2019; Robertson 2022) ionized the gas in the intergalactic medium (IGM).”
A Comprehensive Study of Galaxies at z ∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch (2022, background): “One of the most important goals in astronomy today is to understand galaxy formation from the birth stage to the current stage (Stark 2016; Dayal & Ferrara 2018; Ouchi et al. 2020; Robertson 2022).”
The Dearth of z ∼ 10 Galaxies in All HST Legacy Fields—The Rapid Evolution of the Galaxy Population in the First 500 Myr (2017, background): “…51, 1290 Versoix, Switzerland; pascal.oesch@unige.ch 3 Leiden Observatory, Leiden University, NL-2300 RA Leiden, Netherlands 4 UCO/Lick Observatory, University of California, Santa Cruz, CA 95064, USA a factor 2× growth per redshift bin (see e.g. Stark 2016; Finkelstein 2016, for recent reviews).”
Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky (2017, background): “Great progress has been made in determining the faint end of the UV LFs (see the recent review of Stark 2016).”
The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 – 15 from deep JWST and ground-based near-infrared imaging (2022, background): “Over the last decade, major instrumental advances have enabled astronomers to clarify the background cosmology of the Universe and push studies of galaxies back to within a billion years of the Big Bang (see Dunlop (2013), Madau & Dickinson (2014) & Stark (2016) for reviews).”
New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency (2021, background): “…of the volume density in the context of SFR and stellar mass measurements allow for connections to the underlying dark matter halos (e.g., Behroozi et al. 2013; Harikane et al. 2016, 2018; Finkelstein 2016; Stark 2016; Stefanon et al. 2017a; Dayal & Ferrara 2018; Tacchella et al. 2018).”
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z ≳ 4 (2018, background): “…only been measured poorly, mainly because of insufficient data quality: the sensitivity and resolution of present observations are too low to probe the light of old stars at wavelengths longer than the age-sensitive Balmer break, which moves into the mid-IR at these redshifts (e.g. Stark 2016).”
RELICS: Reionization Lensing Cluster Survey (2019, background): “Detailed studies are required to determine galaxies’ ages, stellar masses, compositions, and ionizing strengths (see Stark 2016 for a review).”
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging (2022, background): “…Hubble Space Telescope (HST) pushed our cosmic horizons well into the epoch of reionization, the time when energetic photons (presumably from massive stars in early galaxies) ionized the gas in the intergalactic medium (e.g., Finkelstein 2016; Stark 2016; Robertson 2022, and references therein).”