Joel Leja
educated at: Yale University
occupation: researcher
Works 1
Articles 35
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A population of red candidate massive galaxies ~600 Myr after the Big Bang
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How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-dust Geometry Model in Spectral Energy Distribution Fitting
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Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
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Chronicling the Host Galaxy Properties of the Remarkable Repeating FRB 20201124A
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High Molecular-gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies
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The Diverse Molecular Gas Content of Massive Galaxies Undergoing Quenching at z ∼ 1
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Quenching of star formation from a lack of inflowing gas to galaxies
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Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation
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SPECULATOR: Emulating Stellar Population Synthesis for Fast and Accurate Galaxy Spectra and Photometry
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REQUIEM-2D Methodology: Spatially Resolved Stellar Populations of Massive Lensed Quiescent Galaxies from Hubble Space Telescope 2D Grism Spectroscopy
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How to Measure Galaxy Star Formation Histories. I. Parametric Models
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Millimeter Mapping at z ∼ 1: Dust-obscured Bulge Building and Disk Growth
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How to Measure Galaxy Star Formation Histories. II. Nonparametric Models
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Discovery of a Dark, Massive, ALMA-only Galaxy at z ~ 5–6 in a Tiny 3 mm Survey
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The Hubble Legacy Field GOODS-S Photometric Catalog
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SN 2016iet: The Pulsational or Pair Instability Explosion of a Low-metallicity Massive CO Core Embedded in a Dense Hydrogen-poor Circumstellar Medium
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale
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The Superluminous Supernova SN 2017egm in the Nearby Galaxy NGC 3191: A Metal-rich Environment Can Support a Typical SLSN Evolution
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PS16dtm: A Tidal Disruption Event in a Narrow-line Seyfert 1 Galaxy
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Deriving Physical Properties from Broadband Photometry with Prospector: Description of the Model and a Demonstration of its Accuracy Using 129 Galaxies in the Local Universe
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Where stars form: inside-out growth and coherent star formation from HST H{alpha} maps of 3200 galaxies across the main sequence at 0.7 < z < 1.5
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The relation between [O III]/H{beta} and specific star formation rate in galaxies at z ~ 2
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The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ~ 100,000 galaxies
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Forming compact massive galaxies
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Galaxy structure as a driver of the star formation sequence slope and scatter
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A massive galaxy in its core formation phase three billion years after the Big Bang
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3D-HST+CANDELS: the evolution of the galaxy size-mass distribution since z = 3
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Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5
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Dense cores in galaxies out to z = 2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields
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On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8
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Observations of environmental quenching in groups in the 11 GYR since z = 2.5: different quenching for central and satellite galaxies
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Tight correlations between massive galaxy structural properties and dynamics: the mass fundamental plane was in place by z ~ 2
Human - wd:Q57570207