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20042025
most citedA Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE

237 citations · 1.1k across the 14 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA20255 cited

REBELS-IFU: Evidence for metal-rich massive galaxies at z~6-8

Lucie E. Rowland, Mauro Stefanon, Rychard Bouwens +30

Metallicity is a crucial tracer of galaxy evolution, providing insights into gas accretion, star formation, and feedback. At high redshift, these processes reveal how early galaxie…

astro-ph.GA202323 cited

The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at

A. P. S. Hygate, J. A. Hodge, E. da Cunha +27

We present Atacama Large Millimeter/Submillimeter Array (ALMA) [CII] and continuum observations of REBELS-25, a massive, morphologically complex ultra-luminous in…

astro-ph.GA20238 cited

The Hα Luminosity Function of Galaxies at z {\sim} 4.5

Victoria Bollo, Valentino González, Mauro Stefanon +5

We present the Hα luminosity function (LF) derived from a large sample of Lyman break galaxies at z {\sim} 4.5 over the GOODS-South and North fields. This study makes use of the ne…

astro-ph.GA202339 cited

The ALMA REBELS Survey: The First Infrared Luminosity Function Measurement at $\mathbf{z \sim 7}

L. Barrufet, P. A. Oesch, R. Bouwens +18

We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a UV-selected galaxy sample with ALMA spectroscopic o…

astro-ph.GA2022124 cited

The ALMA REBELS Survey: the dust content of Lyman Break Galaxies

P. Dayal, A. Ferrara, L. Sommovigo +22

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LB…

astro-ph.GA2022104 cited

The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at

A. Ferrara, L. Sommovigo, P. Dayal +27

We analyse FIR dust continuum measurements for 14 galaxies () in the ALMA REBELS LP to derive their physical properties. Our model uses three input data: (a) the UV spe…