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20172023
most citedCEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST

524 citations · 2.1k across the 41 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.GA2021★ 19 cited

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…

astro-ph.GA2021★ 89 cited

GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

C. Gómez-Guijarro, D. Elbaz, M. Xiao +36

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally…

astro-ph.GA2021★ 12 cited

An Orientation Bias in Observations of Submillimetre Galaxies

C. C. Lovell, J. E. Geach, R. Davé +5

Recent high-resolution interferometric images of submillimetre galaxies (SMGs) reveal fascinatingly complex morphologies. This raises a number of questions: how does the relative o…

astro-ph.GA2021

The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5

A. Saxena, R. S. Ellis, P. U. Forster +14

We use VANDELS spectroscopic data overlapping with the 7 Ms Chandra Deep Field South survey to extend studies of high-mass X-ray binary systems (XRBs) in 301 normal star-fo…

astro-ph.GA2021★ 7 cited

Low-frequency radio spectra of submillimetre galaxies in the Lockman Hole

J. Ramasawmy, J. E. Geach, M. J. Hardcastle +19

We investigate the radio properties of a sample of 53 sources selected at 850 m from the SCUBA-2 Cosmology Legacy Survey using new deep, low-frequency radio imaging of the Lockm…

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…