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19942022
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 4.5k across the 79 of their papers we have counts for

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53 papers · 1 filter

astro-ph.GA202232 cited

The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS

S. A. Urquhart, G. J. Bendo, S. Serjeant +53

We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimeter sources from the Southern fields of the Herschel Astrophysical…

astro-ph.GA202116 cited

ALMA Observations of Lyman-alpha Blob 1: Multiple major-mergers and widely distributed interstellar media

Hideki Umehata, Ian Smail, Charles C. Steidel +11

We present observations of a giant Lyman-alpha blob in the SSA22 proto-cluster at z=3.1, SSA22-LAB1, taken with the Atacama Large Millimeter/submillimeter Array (ALMA). Dust contin…

astro-ph.GA2021

Cosmic evolution of the H2 mass density and the epoch of molecular gas

T. K. Garratt, K. E. K. Coppin, J. E. Geach +13

We present new empirical constraints on the evolution of , the cosmological mass density of molecular hydrogen, back to . We employ a statistical approach…

astro-ph.GA202020 cited

Rise of the Titans: Gas Excitation and Feedback in a Binary Hyper-Luminous Dusty Starburst Galaxy at z~6

Dominik A. Riechers, Hooshang Nayyeri, Denis Burgarella +8

We report new observations toward the hyper-luminous dusty starbursting major merger ADFS-27 (z=5.655), using ATCA and ALMA. We detect CO 2-1, 8-7, 9-8, 10-9 and H2O(321-221) emiss…

astro-ph.GA202040 cited

Is there enough star formation in simulated protoclusters?

Seunghwan Lim, Douglas Scott, Arif Babul +5

As progenitors of the most massive objects, protoclusters are key to tracing the evolution and star-formation history of the Universe, and are responsible for per c…

astro-ph.GA2020

An ALMA survey of the S2CLS UDS field: Optically invisible submillimetre galaxies

Ian Smail, U. Dudzevičiūtė, S. M. Stach +16

We analyse a robust sample of 30 near-infrared-faint (K>25.3, 5 sigma) submillimetre galaxies selected across a 0.96 deg^2 field, to investigate their properties and the cause of t…