activity
20122026
most citedCEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST

524 citations · 16.2k across the 348 of their papers we have counts for

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Showing 2021Show all

16 papers · 1 filter

astro-ph.GA2021★ 30 cited

On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation

Minjung Park, Sandro Tacchella, Erica J. Nelson +7

Observations have shown that the star-formation activity and the morphology of galaxies are closely related, but the underlying physical connection is not well understood. Using th…

astro-ph.GA2021★ 45 cited

The Prevalence of Galaxy Overdensities Around UV-Luminous Lyman Emitters in the Epoch of Reionization

E. Leonova, P. A. Oesch, Y. Qin +19

Before the end of the epoch of reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly lines of galaxies in th…

astro-ph.GA2021★ 83 cited

H-alpha emission in local galaxies: star formation, time variability and the diffuse ionized gas

Sandro Tacchella, Aaron Smith, Rahul Kannan +6

The nebular recombination line H is widely used as a star-formation rate (SFR) indicator in the local and high-redshift Universe. We present a detailed H radiative transfer s…

astro-ph.GA2021★ 57 cited

The physics of Lyman-alpha escape from disc-like galaxies

Aaron Smith, Rahul Kannan, Sandro Tacchella +8

Hydrogen emission lines can provide extensive information about star-forming galaxies in both the local and high-redshift Universe. We present a detailed Lyman continuum (LyC), Lym…

astro-ph.GA2021★ 212 cited

On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times

Sandro Tacchella, Steven L. Finkelstein, Micaela Bagley +18

We present a detailed stellar population analysis of 11 bright () galaxies at (three spectroscopically confirmed) to constrain the chemical enrichment and growth o…

astro-ph.GA2021★ 66 cited

Evidence from Disrupted Halo Dwarfs that -process Enrichment via Neutron Star Mergers is Delayed by Myrs

Rohan P. Naidu, Alexander P. Ji, Charlie Conroy +10

The astrophysical origins of -process elements remain elusive. Neutron star mergers (NSMs) and special classes of core-collapse supernovae (rCCSNe) are leading candidates. Due t…

astro-ph.GA2021★ 1 cited

The Synchrony of Production & Escape: Half the Bright Ly Emitters at have Lyman Continuum Escape Fractions

Rohan P. Naidu, Jorryt Matthee, Pascal A. Oesch +14

The ionizing photon escape fraction (LyC ) of star-forming galaxies is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit t…

astro-ph.GA2021★ 69 cited

(Re)Solving Reionization with Lyα: How Bright Lyα Emitters account for the Cosmic Ionizing Background

Jorryt Matthee, Rohan P. Naidu, Gabriele Pezzulli +12

The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here we introduce an emissivity framework based on Ly emitters (LAEs…

astro-ph.GA2021★ 27 cited

Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting

Abdurro'uf, Yen-Ting Lin, Hiroyuki Hirashita +5

We study spatially resolved properties (on spatial scales of kpc out to at least effective radii) of the stars, dust, and gas in ten nearby spiral galaxies. The prop…

astro-ph.GA2021★ 19 cited

Reproducing the UVJ Color Distribution of Star-forming Galaxies at 0.5 < z < 2.5 with a Geometric Model of Dust Attenuation

Leah Zuckerman, Sirio Belli, Joel Leja +1

We analyze the distribution of rest-frame U-V and V-J colors for star-forming galaxies at 0.5 < z < 2.5. Using stellar population synthesis, stochastic star formation histories, an…

astro-ph.GA2021★ 122 cited

A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields

Steven L. Finkelstein, Micaela Bagley, Mimi Song +21

We present the results from a new search for candidate galaxies at z ~ 8.5-11 discovered over the 850 arcmin^2 area probed by the Cosmic Assembly Near-Infrared Deep Extragalactic L…

astro-ph.GA2021★ 43 cited

High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies

Xuejian Shen, Mark Vogelsberger, Dylan Nelson +5

We post-process galaxies in the IllustrisTNG simulations with SKIRT radiative transfer calculations to make predictions for the rest-frame near-infrared (NIR) and far-infrared (FIR…

astro-ph.GA2021★ 167 cited

Reconstructing the Last Major Merger of the Milky Way with the H3 Survey

Rohan P. Naidu, Charlie Conroy, Ana Bonaca +8

Several lines of evidence suggest the Milky Way underwent a major merger at z~2 with a galaxy known as Gaia-Sausage-Enceladus (GSE). Here we use H3 Survey data to argue that GSE en…

astro-ph.GA2021★ 39 cited

The Diverse Molecular Gas Content of Massive Galaxies Undergoing Quenching at z~1

Sirio Belli, Alessandra Contursi, Reinhard Genzel +20

We present a detailed study of the molecular gas content and stellar population properties of three massive galaxies at 1 < z < 1.3 that are in different stages of quenching. The g…

astro-ph.GA2021★ 170 cited

Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8

Sandro Tacchella, Charlie Conroy, S. M. Faber +14

We investigate the stellar populations for a sample of 161 massive, mainly quiescent galaxies at with deep Keck/DEIMOS rest-frame optical spectros…

astro-ph.GA2021★ 102 cited

Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations

Erica J. Nelson, Sandro Tacchella, Benedikt Diemer +21

We compare the star forming main sequence (SFMS) -- both integrated and resolved on 1kpc scales -- between the high-resolution TNG50 simulation of IllustrisTNG and observations fro…