246 citations · 1.1k across the 16 of their papers we have counts for
49 papers
Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
Olivia R. Cooper, Caitlin M. Casey, Jorge A. Zavala +5
A complete census of dusty star-forming galaxies (DSFGs) at early epochs is necessary to constrain the obscured contribution to the cosmic star formation rate density (CSFRD), howe…
Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo
Justin S. Spilker, Christopher C. Hayward, Daniel P. Marrone +20
The SPT0311-58 system at z=6.900 is an extremely massive structure within the reionization epoch, and offers a chance to understand the formation of galaxies in an extreme peak in…
Multi-Phase ISM in the z = 5.7 Hyperluminous Starburst SPT0346-52
Katrina C. Litke, Daniel P. Marrone, Manuel Aravena +13
SPT0346-52 (z=5.7) is the most intensely star-forming galaxy discovered by the South Pole Telescope, with Sigma_SFR ~ 4200 Msol yr^-1 kpc^-2. In this paper, we expand on previous s…
ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
Christina C. Williams, Stacey Alberts, Justin S. Spilker +6
We report the serendipitous discovery of an overdensity of CO emitters in an X-ray-identified cluster (LogM at z=1.3188) using ALMA. We presen…
The ramp-up of interstellar medium enrichment at z>4
M. Franco, K. E. K. Coppin, J. E. Geach +7
Fluorine is one of the most interesting elements for nuclear and stellar astrophysics. Fluorine abundance was first measured for stars other than the Sun in 1992, then for a handfu…
Quenching of star formation from a lack of inflowing gas to galaxies
Katherine E. Whitaker, Christina C. Williams, Lamiya Mowla +16
Star formation in half of massive galaxies was quenched by the time the Universe was three billion years old. Very low amounts of molecular gas appear responsible for this, at leas…