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20022026
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 20.9k across the 253 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

16 papers · 2 filters

astro-ph.GA2019★ 49 cited

NOEMA redshift measurements of bright Herschel galaxies

R. Neri, P. Cox, A. Omont +31

Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Surv…

astro-ph.GA2019★ 37 cited

SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-m-selected galaxies

Chen-Fatt Lim, Wei-Hao Wang, Ian Smail +35

We construct a SCUBA-2 450-m map in the COSMOS field that covers an area of 300 arcmin and reaches a 1 noise level of 0.65 mJy in the deepest region. We extract 256 sou…

astro-ph.GA2019★ 58 cited

On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5

Jorge A. Zavala, C. M. Casey, J. B. Champagne +9

We present ALMA Band 6 (nu=233GHz, lambda=1.3mm) continuum observations towards 68 'normal' star-forming galaxies within two Coma-like progenitor structures at z=2.10 and 2.47, fro…

astro-ph.GA2019★ 6 cited

A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population

J. Greenslade, E. Aguilar, D. L. Clements +19

Dusty star-forming galaxies (DSFGs) detected at provide important examples of the first generations of massive galaxies. However, few examples with spectroscopic confirmati…

astro-ph.GA2019★ 24 cited

SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE

T. Cheng, D. L. Clements, J. Greenslade +21

We present SCUBA-2 850-m observations of 13 candidate starbursting protoclusters selected using Planck and Herschel data. The cumulative number counts of the 850-m sources in…

astro-ph.GA2019★ 20 cited

Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z=2.2

Drew Brisbin, Manuel Aravena, Emanuele Daddi +5

We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z=2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3), a…

astro-ph.GA2019

Astro2020 Science White Paper: Exploration and characterization of the earliest epoch of galaxy formation: beyond the re-ionization era

Kotaro Kohno, Yoichi Tamura, Akio Inoue +9

State-of-the-art rest-frame UV and FIR photometric and spectroscopic observations are now pushing the redshift frontiers of galaxy formation studies up to and beyond. R…

astro-ph.GA2019★ 33 cited

The Dust and Molecular Gas in the Brightest Cluster Galaxy in MACS 1931.8-2635

Kevin Fogarty, Marc Postman, Yuan Li +6

We present new ALMA observations of the molecular gas and far-infrared continuum around the brightest cluster galaxy (BCG) in the cool-core cluster MACS 1931.8-2635. Our observatio…

astro-ph.GA2019★ 65 cited

Confirming Herschel candidate protoclusters from ALMA/VLA CO observations

C. Gómez-Guijarro, D. A. Riechers, R. Pavesi +11

ALMA 870m continuum imaging has uncovered a population of blends of multiple dusty star-forming galaxies (DSFGs) in sources originally detected with the Herschel Space Observato…

astro-ph.GA2019★ 1 cited

The Radio Universe at Low Surface Brightness: Feedback & accretion in the circumgalactic medium

Bjorn Emonts, Mark Lacy, Kristina Nyland +12

Massive galaxies at high-z are known to co-evolve with their circumgalactic medium (CGM). If we want to truly understand the role of the CGM in the early evolution of galaxies and…

astro-ph.GA2019★ 70 cited

The Main Sequence at contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?

A. Puglisi, E. Daddi, D. Liu +20

ALMA measurements for 93 -selected galaxies at in COSMOS reveal a sizable (\%) population with compact star formation (SF) sizes, lyi…

astro-ph.GA2019

Astro2020 Science White Paper: The Extended Cool Gas Reservoirs Within z > 1 (Proto-)Cluster Environments

Kevin C. Harrington, D. Frayer, H. Dannerbauer

High-redshift () proto-clusters will serve as testing grounds to probe the gas supply furnishing the emerging metals, stars, and large-scale structures we see at the current epo…

astro-ph.GA2019★ 1 cited

Mapping Galaxy Clusters in the Distant Universe

H. Dannerbauer, E. van Kampen, J. Afonso +21

We present the science case for mapping several thousand galaxy (proto)clusters at z=1-10 with a large aperture single dish sub-mm facility, producing a high-redshift counterpart t…

astro-ph.GA2019★ 1 cited

The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10

James E. Geach, Manda Banerji, Frank Bertoldi +53

The Sloan Digital Sky Survey (SDSS) was revolutionary because of the extraordinary breadth and ambition of its optical imaging and spectroscopy. We argue that a 'sub-millimeter SDS…

astro-ph.GA2019★ 39 cited

High gas fraction in a CO-selected main-sequence galaxy at

Avani Gowardhan, Dominik Riechers, Riccardo Pavesi +3

We report NOrthern Extended Millimetre Array (NOEMA) observations of warm molecular gas traced by CO() in a gas-rich main-sequence galaxy (MS), initially serendip…

astro-ph.GA2019★ 71 cited

Strong FUV fields drive the [CII]/FIR deficit in z~3 dusty, star-forming galaxies

Matus Rybak, G. Calistro Rivera, J. A. Hodge +11

We present 0.15-arcsec (1 kpc) resolution ALMA observations of the [CII] 157.74 um line and rest-frame 160-um continuum emission in two z~3 dusty, star-forming galaxies - ALESS 49.…