activity
20042025
most citedUV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields

1.2k citations · 9.5k across the 61 of their papers we have counts for

collaborators

61 papers

astro-ph.GA2025★ 5 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.GA2023★ 23 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.GA2023★ 8 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.GA2023★ 39 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.GA2022★ 105 cited

The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7

Hiddo Algera, Hanae Inami, Pascal Oesch +21

Cosmic dust is an essential component shaping both the evolution of galaxies and their observational signatures. How quickly dust builds up in the early Universe remains an open qu…

astro-ph.GA2022★ 107 cited

Unveiling the Nature of Infrared Bright, Optically Dark Galaxies with Early JWST Data

L. Barrufet, P. A. Oesch, A. Weibel +18

Over the last few years, both ALMA and Spitzer/IRAC observations have revealed a population of likely massive galaxies at that was too faint to be detected in HST rest-frame…