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20112026
most citedGalaxy growth in a massive halo in the first billion years of cosmic history

246 citations · 4.5k across the 78 of their papers we have counts for

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Showing 2018Show all

11 papers · 1 filter

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★ 38 cited

Overdensity of submillimeter galaxies around the MAMMOTH-1 nebula

F. Arrigoni Battaia, Chian-Chou Chen, M. Fumagalli +7

In the hierarchical model of structure formation, giant elliptical galaxies form through merging processes within the highest density peaks known as protoclusters. While high-redsh…

astro-ph.GA2018★ 152 cited

ALMA reveals potential evidence for spiral arms, bars, and rings in high-redshift submillimeter galaxies

J. A. Hodge, I. Smail, F. Walter +20

We present sub-kpc-scale mapping of the 870 m ALMA continuum emission in six luminous ( L) submillimeter galaxies (SMGs) from the ALES…

astro-ph.GA2018★ 12 cited

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies

Yu-Yen Chang, Nicholas Ferraro, Wei-Hao Wang +25

We present structural parameters and morphological properties of faint 450-um selected submillimeter galaxies (SMGs) from the JCMT Large Program, STUDIES, in the COSMOS-CANDELS reg…

astro-ph.GA2018★ 36 cited

A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS

FangXia An, S. M. Stach, Ian Smail +23

We describe the application of the supervised machine-learning algorithms to identify the likely multi-wavelength counterparts to submillimeter sources detected in panoramic, singl…

astro-ph.GA2018★ 35 cited

An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources

J. L. Wardlow, J. M. Simpson, Ian Smail +15

We present ALMA observations of the mid-J 12CO emission from six single-dish selected 870-micron sources in the Extended Chandra Deep Field-South (ECDFS) and UKIDSS Ultra-Deep Surv…

astro-ph.GA2018★ 38 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Identifying candidate z~4.5 [CII] emitters

E. A. Cooke, Ian Smail, A. M. Swinbank +18

We report the results of a search for serendipitous [CII] 157.74m emitters at - using the Atacama Large Millimeter/submillimeter Array (ALMA). The search exploits…

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★ 134 cited

Resolving the ISM at the peak of cosmic star formation with ALMA - The distribution of CO and dust continuum in z~2.5 sub-millimetre galaxies

Gabriela Calistro-Rivera, J. A. Hodge, Ian Smail +17

We use ALMA observations of four sub-millimetre galaxies (SMGs) at to investigate the spatially resolved properties of the inter-stellar medium (ISM) at scales of 1--5 k…

astro-ph.GA2018★ 32 cited

Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common

Christopher C. Hayward, Scott C. Chapman, Charles C. Steidel +19

Interferometric observations have demonstrated that a significant fraction of single-dish submillimetre (submm) sources are blends of multiple submm galaxies (SMGs), but the nature…