Search Results - "Finkelstein, Steven L."
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On the Coevolution of the AGN and Star-forming Galaxy Ultraviolet Luminosity Functions at 3 < z < 9
Published in The Astrophysical journal (01-10-2022)“…Abstract Studies of the rest-frame ultraviolet (UV) luminosity functions (LFs) typically treat star-forming galaxies and active galactic nuclei (AGNs)…”
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Legacy of star formation in the pre-reionization universe
Published in Monthly notices of the Royal Astronomical Society (11-09-2019)“…ABSTRACT We utilize gizmo, coupled with newly developed sub-grid models for Population III (Pop III) and Population II (Pop II), to study the legacy of star…”
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Baseline metal enrichment from Population III star formation in cosmological volume simulations
Published in Monthly notices of the Royal Astronomical Society (21-04-2018)“…Abstract We utilize the hydrodynamic and N-body code GIZMO coupled with our newly developed sub-grid Population III (Pop III) Legacy model, designed…”
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On the Stellar Populations of Galaxies at z = 9–11: The Growth of Metals and Stellar Mass at Early Times
Published in The Astrophysical journal (01-03-2022)“…We present a detailed stellar population analysis of 11 bright (H < 26.6) galaxies at z=9−11 (three spectroscopically confirmed) to constrain the chemical…”
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Semi-analytic forecasts for JWST – IV. Implications for cosmic reionization and LyC escape fraction
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT Galaxies forming in low-mass haloes are thought to be primarily responsible for reionizing the Universe during the first billion years after the big…”
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THE EVOLUTION OF THE GALAXY REST-FRAME ULTRAVIOLET LUMINOSITY FUNCTION OVER THE FIRST TWO BILLION YEARS
Published in The Astrophysical journal (01-09-2015)“…ABSTRACT We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4-8. We use deep Hubble Space Telescope…”
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A First Look at the Abundance Pattern—O/H, C/O, and Ne/O—in z > 7 Galaxies with JWST/NIRSpec
Published in Astrophysical journal. Letters (01-11-2022)“…Abstract We analyze the rest-frame near-UV and optical nebular spectra of three z > 7 galaxies from the Early Release Observations taken with the Near-Infrared…”
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Semi-analytic forecasts for JWST – VI. Simulated light-cones and galaxy clustering predictions
Published in Monthly notices of the Royal Astronomical Society (18-08-2022)“…ABSTRACT In anticipation of the new era of high-redshift exploration marked by the commissioning of the James Webb Space Telescope (JWST), we present two sets…”
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Semi-analytic forecasts for JWST – III. Intrinsic production efficiency of Lyman-continuum radiation
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT The James Webb Space Telescope is expected to enable transformational progress in studying galaxy populations in the very early Universe, during the…”
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CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
Published in The Astrophysical journal (01-08-2020)“…The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the…”
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An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
Published in The Astrophysical journal (20-07-2018)“…Deep, pencil-beam surveys from ALMA at 1.1-1.3 mm have uncovered an apparent absence of high-redshift dusty galaxies, with existing redshift distributions…”
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12
The SFR-M Correlation Extends to Low Mass at High Redshift
Published in The Astrophysical journal (20-10-2018)“…To achieve a fuller understanding of galaxy evolution, SED fitting can be used to recover quantities beyond stellar masses (M*) and star formation rates…”
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Exploring AGN and star formation activity of massive galaxies at cosmic noon
Published in Monthly notices of the Royal Astronomical Society (21-09-2020)“…ABSTRACT We investigate the relation between active galactic nucleus (AGN) and star formation (SF) activity at 0.5 < z < 3 by analysing 898 galaxies with X-ray…”
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Near-infrared Spectroscopy of Galaxies During Reionization: Measuring C iii] in a Galaxy at z = 7.5
Published in The Astrophysical journal (10-07-2019)“…We present Keck/MOSFIRE H-band spectroscopy targeting C iii] λ1907, 1909 in a z = 7.5056 galaxy previously identified via Ly emission. We detect strong line…”
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15
Global radiation signature from early structure formation
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…Abstract We use cosmological hydrodynamic zoom-in simulations to study early structure formation in two dark matter (DM) cosmologies, the standard cold dark…”
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Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST
Published in The Astrophysical journal (01-12-2023)“…Abstract The selection of high-redshift galaxies often involves spectral energy distribution (SED) fitting to photometric data, an expectation for…”
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On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from z = 1.5 to 0.4
Published in The Astrophysical journal (20-03-2020)“…We study the evolution in the number density of galaxies at the highest stellar masses over the past 9 Gyr ( ) using the Spitzer/HETDEX Exploratory Large-Area…”
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CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6
Published in The Astrophysical journal (01-12-2021)“…Abstract We report on the gas-phase metallicity gradients of a sample of 238 star-forming galaxies at 0.6 < z < 2.6, measured through deep near-infrared Hubble…”
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The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z = 3–5 over 17.5 deg2 in the SHELA Field
Published in The Astrophysical journal (01-11-2021)“…We present the results of a deep Ks-band (2.1 μm) imaging survey of the Spitzer/HETDEX Exploratory Large-Area (SHELA) field using the NEWFIRM near-infrared…”
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Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
Published in The Astrophysical journal (01-04-2023)“…Abstract We present a catalog of about 25,000 images of massive ( M ⋆ ≥ 10 9 M ⊙ ) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation,…”
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