activity
20072026
most citedThe Spitzer Survey of Stellar Structure in Galaxies (S^4G)

521 citations · 11.4k across the 211 of their papers we have counts for

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Showing 2024Show all

22 papers · 1 filter

astro-ph.GA2024★ 6 cited

Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured Galaxies

Dejene Zewdie, Roberto J. Assef, Trystan Lambert +15

Hot dust-obscured galaxies (Hot DOGs), are a family of hyper-luminous, heavily obscured quasars. A number of studies have shown that these objects reside in significantly overdense…

astro-ph.GA2024★ 6 cited

A Large Molecular Gas Reservoir in the Protocluster SPT234956 at

Dazhi Zhou, Scott C. Chapman, Nikolaus Sulzenauer +13

We present Atacama Compact Array (ACA) Band-3 observations of the protocluster SPT234956, an extreme system hosting submillimeter galaxies (SMGs) at $z\,{=}\,4.3…

astro-ph.GA2024★ 5 cited

Evidence for environmental effects in the protocluster core SPT234956

Chayce Hughes, Ryley Hill, Scott Chapman +16

We present ALMA observations of the [CI] 492 and 806GHz fine-structure lines in 25 dusty star-forming galaxies (DSFGs) at in the core of the SPT234956 protoclu…

astro-ph.GA2024★ 5 cited

The ALMA-CRISTAL Survey: Complex kinematics of the galaxies at the end of the Reionization Era

K. Telikova, J. González-López, M. Aravena +18

The history of gas assembly in early galaxies is reflected in their complex kinematics. While a considerable fraction of galaxies at z~5 are consistent with rotating disks, current…

astro-ph.GA2024★ 10 cited

Kinematic analysis of galaxies in the SPT234956 protocluster core

Aparna Venkateshwaran, Axel Weiss, Nikolaus Sulzenauer +10

SPT234956 is a protocluster discovered in the 2500 deg South Pole Telescope (SPT) survey. In this paper, we study the kinematics of the galaxies found in the core of SPT2349…

astro-ph.GA2024

Characterizing the contribution of dust-obscured star formation at 5 using 18 serendipitously identified [CII] emitters

I. F. van Leeuwen, R. J. Bouwens, P. P. van der Werf +24

We present a new method to determine the star formation rate (SFR) density of the Universe at that includes the contribution of dust-obscured star formation. For this…