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20132026
most citedALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

295 citations · 5.6k across the 141 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.GA2018★ 51 cited

1D Kinematics from stars and ionized gas at from the LEGA-C spectroscopic survey of massive galaxies

Rachel Bezanson, Arjen van der Wel, Caroline Straatman +14

We present a comparison of the observed, spatially integrated stellar and ionized gas velocity dispersions of massive () galaxies…

astro-ph.GA2018★ 58 cited

Spatially Resolved [CII] Emission in SPT0346-52: A Hyper-Starburst Galaxy Merger at z~5.7

Katrina C. Litke, Daniel P. Marrone, Justin S. Spilker +18

SPT0346-52 is one of the most most luminous and intensely star-forming galaxies in the universe, with L_FIR > 10^13 L_sol and Sigma_SFR ~ 4200 M_sol yr^-1 kpc^-2. In this paper, we…

astro-ph.GA2018★ 19 cited

Dense-gas tracers and carbon isotopes in five 2.5<z<4 lensed dusty star forming galaxies from the SPT SMG sample

M. Bethermin, T. R. Greve, C. De Breuck +15

The origin of the high SFR observed in high-z dusty star-forming galaxies is still unknown. Large fractions of dense molecular gas might provide part of the explanation, but there…

astro-ph.GA2018★ 42 cited

Constraining the volume density of Dusty Star-Forming Galaxies through the first 3mm Number Counts from ALMA

J. A. Zavala, C. M. Casey, E. da Cunha +4

We carry out a blind search of 3mm continuum sources using the ALMA Science Archive to derive the first galaxy number counts at this wavelength. The analyzed data are drawn from ob…

astro-ph.GA2018★ 1 cited

Science with an ngVLA: Characterizing Feedback Through Molecular Outflows Across Cosmic Time

Justin Spilker, Kristina Nyland

Galactic winds are ubiquitously observed in galaxies both locally and in the high-redshift Universe. While these winds span many orders of magnitude in both temperature and density…

astro-ph.GA2018★ 108 cited

The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release II: dynamical and stellar population properties of z ~< 1 galaxies in the COSMOS field

Caroline M. S. Straatman, Arjen van der Wel, Rachel Bezanson +18

We present the second data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO 130-night public spectroscopic survey conducted with VIMOS on the Very Large Teles…

astro-ph.GA2018★ 82 cited

Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe

J. S. Spilker, M. Aravena, M. Bethermin +20

Galaxies grow inefficiently, with only a few percent of the available gas converted into stars each free-fall time. Feedback processes, such as outflowing winds driven by radiation…

astro-ph.GA2018★ 60 cited

An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies

Caitlin M. Casey, Jacqueline Hodge, Jorge A. Zavala +5

Deep, pencil-beam surveys from ALMA at 1.1-1.3mm have uncovered an apparent absence of high-redshift dusty galaxies, with existing redshift distributions peaking around $z\sim1.5-2…

astro-ph.GA2018★ 133 cited

The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era

Caitlin M. Casey, Jorge A. Zavala, Justin Spilker +6

Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3m-3mm), constraints on the infrared through millimeter galaxy luminosity function (the `…

astro-ph.GA2018★ 75 cited

Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey

Justin Spilker, Rachel Bezanson, Ivana Barisic +13

A decade of study has established that the molecular gas properties of star-forming galaxies follow coherent scaling relations out to z~3, suggesting remarkable regularity of the i…

astro-ph.GA2018★ 16 cited

Stellar and Molecular Gas Rotation in a Recently-Quenched Massive Galaxy at z~0.7

Qiana Hunt, Rachel Bezanson, Jenny E. Greene +7

The process by which massive galaxies transition from blue, star-forming disks into red, quiescent galaxies remains one of the most poorly-understood aspects of galaxy evolution. I…

astro-ph.GA2018★ 220 cited

A massive core for a cluster of galaxies at a redshift of 4.3

T. B. Miller, S. C. Chapman, M. Aravena +35

Massive galaxy clusters are now found as early as 3 billion years after the Big Bang, containing stars that formed at even earlier epochs. The high-redshift progenitors of these ga…

astro-ph.GA2018★ 62 cited

Stellar Populations of over one thousand Galaxies from LEGA-C: Ages and Star Formation Histories from D4000 and H

Po-Feng Wu, Arjen van der Wel, Anna Gallazzi +18

Drawing from the LEGA-C dataset, we present the spectroscopic view of the stellar population across a large volume- and mass-selected sample of galaxies at large lookback time. We…