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19992024
most citedUV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields

1.2k citations · 14k across the 71 of their papers we have counts for

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26 papers · 1 filter

astro-ph.GA2024★ 30 cited

An Hα view of galaxy build-up in the first 2 Gyr: luminosity functions at z~4-6.5 from NIRCam/grism spectroscopy

Alba Covelo-Paz, Emma Giovinazzo, Pascal A. Oesch +22

The Hα nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z>3 for the first time…

astro-ph.GA2023★ 37 cited

Unveiling the hidden universe with JWST: The contribution of dust-obscured galaxies to the stellar mass function at

R. Gottumukkala, L. Barrufet, P. A. Oesch +17

With the advent of JWST, we can probe the rest-frame optical emission of galaxies at with high sensitivity and spatial resolution, making it possible to accurately characteri…

astro-ph.GA2023★ 12 cited

Accelerated Formation of Ultra-Massive Galaxies in the First Billion Years

Mengyuan Xiao, Pascal Oesch, David Elbaz +35

Recent JWST observations have revealed an unexpected abundance of massive galaxy candidates in the early Universe, extending further in redshift and to lower luminosity than what h…

astro-ph.GA2023★ 8 cited

The galaxy UV luminosity function at from a suite of public JWST ERS, ERO and Cycle-1 programs

D. J. McLeod, C. T. Donnan, R. J. McLure +8

We present a new determination of the evolving galaxy UV luminosity function (LF) over the redshift range based on a wide-area ( arcmin) data set of JWST NIR…

astro-ph.GA2023★ 13 cited

The JWST FRESCO Survey: Legacy NIRCam/Grism Spectroscopy and Imaging in the two GOODS Fields

P. A. Oesch, G. Brammer, R. P. Naidu +38

We present the JWST Cycle 1 53.8hr medium program FRESCO, short for "First Reionization Epoch Spectroscopically Complete Observations". FRESCO covers 62 arcmin in each of the t…

astro-ph.GA2023★ 53 cited

Deciphering Lyman- Emission Deep into the Epoch of Reionisation

Callum Witten, Nicolas Laporte, Sergio Martin-Alvarez +18

During the epoch of reionisation the first galaxies were enshrouded in pristine neutral gas, with one of the brightest emission lines in star-forming galaxies, Lyman- (Ly), e…

astro-ph.GA2023★ 232 cited

A massive quiescent galaxy at redshift 4.658

A. C. Carnall, R. J. McLure, J. S. Dunlop +10

The extremely rapid assembly of the earliest galaxies during the first billion years of cosmic history is a major challenge for our understanding of galaxy formation physics. The a…

astro-ph.GA2022★ 76 cited

The abundance of galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging

C. T. Donnan, D. J. McLeod, R. J. McLure +4

We utilise JWST NIRCam medium-band imaging to search for extreme redshift () galaxy candidates in the Hubble Ultra Deep Field (HUDF) and the additional pointing within…

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…

astro-ph.GA2022★ 429 cited

The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging

C. T. Donnan, D. J. McLeod, J. S. Dunlop +11

We reduce and analyse the available James Webb Space Telescope (JWST) ERO and ERS NIRCam imaging (SMACS0723, GLASS, CEERS) in combination with the latest deep ground-based near-inf…

astro-ph.GA2022★ 441 cited

Two Remarkably Luminous Galaxy Candidates at Revealed by JWST

Rohan P. Naidu, Pascal A. Oesch, Pieter van Dokkum +22

The first few hundred Myrs at mark the last major uncharted epoch in the history of the Universe, where only a single galaxy (GNz11 at ) is currently spectroscop…

astro-ph.GA2021★ 45 cited

The Prevalence of Galaxy Overdensities Around UV-Luminous Lyman Emitters in the Epoch of Reionization

E. Leonova, P. A. Oesch, Y. Qin +19

Before the end of the epoch of reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly lines of galaxies in th…

astro-ph.GA2021★ 25 cited

The Spitzer/IRAC Legacy over the GOODS Fields: Full-Depth 3.6, 4.5, 5.8 and 8.0um Mosaics and Photometry for > 9000 Galaxies at z~3.5-10 from the GOODS Re-ionization Era wide-Area Treasury from Spitzer (GREATS)

Mauro Stefanon, Ivo Labbé, Pascal A. Oesch +9

We present the deepest Spitzer/IRAC , , and m wide-area mosaics yet over the GOODS-N and GOODS-S fields as part of the GOODS Re-ionization Era wide-Area Treas…

astro-ph.GA2019★ 161 cited

The Hubble Legacy Field GOODS-S Photometric Catalog

Katherine E. Whitaker, Mohammad Ashas, Garth Illingworth +12

This manuscript describes the public release of the Hubble Legacy Fields (HLF) project photometric catalog for the extended GOODS-South region from the Hubble Space Telescope (HST)…

astro-ph.GA2019★ 34 cited

The Super Eight Galaxies: Properties of a Sample of Very Bright Galaxies at

Joanna S. Bridge, Benne W. Holwerda, Mauro Stefanon +12

We present the Super Eight galaxies - a set of very luminous, high-redshift () galaxy candidates found in Brightest of Reionizing Galaxies (BoRG) Survey fields. The orig…

astro-ph.GA2018★ 65 cited

HDUV: The Hubble Deep UV Legacy Survey

P. A. Oesch, M. Montes, N. Reddy +15

We present the Hubble Deep UV Legacy Survey (HDUV), a 132 orbit imaging program with the WFC3/UVIS camera onboard the Hubble Space Telescope (HST). The HDUV extends and builds on t…

astro-ph.GA2017★ 46 cited

HST imaging of the brightest z~8-9 galaxies from UltraVISTA: the extreme bright end of the UV luminosity function

Mauro Stefanon, Ivo Labbé, Rychard J. Bouwens +13

We report on the discovery of three especially bright candidate galaxies. Five sources were targeted for follow-up with HST/WFC3, selected from a larger sample…

astro-ph.GA2017★ 224 cited

The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies

Naveen A. Reddy, Pascal A. Oesch, Rychard J. Bouwens +13

We use a newly assembled large sample of 3,545 star-forming galaxies with secure spectroscopic, grism, and photometric redshifts at z=1.5-2.5 to constrain the relationship between…

astro-ph.GA2016★ 41 cited

The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging

R. P. Naidu, P. A. Oesch, N. Reddy +14

We present six galaxies at z~2 that show evidence of Lyman continuum (LyC) emission based on the newly acquired UV imaging of the Hubble Deep UV legacy survey (HDUV) conducted with…

astro-ph.GA2016★ 4 cited

The Hubble Legacy Fields (HLF-GOODS-S) v1.5 Data Products: Combining 2442 Orbits of GOODS-S/CDF-S Region ACS and WFC3/IR Images

Garth Illingworth, Daniel Magee, Rychard Bouwens +7

We have submitted to MAST the 1.5 version data release of the Hubble Legacy Fields (HLF) project covering a 25 x 25 arcmin area over the GOODS-S (ECDF-S) region from the HST archiv…

astro-ph.GA2016★ 533 cited

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

P. A. Oesch, G. Brammer, P. G. van Dokkum +15

We present Hubble WFC3/IR slitless grism spectra of a remarkably bright galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging data. A significant…

astro-ph.GA2015★ 735 cited

The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for galaxies

Ivelina G. Momcheva, Gabriel B. Brammer, Pieter G. van Dokkum +27

We present reduced data and data products from the 3D-HST survey, a 248-orbit HST Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five CANDELS fie…

astro-ph.GA2015★ 98 cited

Ultradeep IRAC Imaging Over The HUDF And GOODS-South: Survey Design And Imaging Data Release

I. Labbe, P. A. Oesch, G. D. Illingworth +11

The IRAC ultradeep field (IUDF) and IRAC Legacy over GOODS (IGOODS) programs are two ultradeep imaging surveys at 3.6μm and 4.5μm with the Spitzer Infrared Array Camera (IRAC). The…

astro-ph.GA2015★ 140 cited

The Bright End of the z~9 and z~10 UV Luminosity Functions using all five CANDELS Fields

R. J. Bouwens, P. A. Oesch, I. Labbe +14

The deep, wide-area (~800-900 arcmin**2) near-infrared/WFC3/IR + Spitzer/IRAC observations over the CANDELS fields have been a remarkable resource for constraining the bright end o…