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20062026
most citedUV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields

1.2k citations · 17.8k across the 216 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.CO2019★ 14 cited

RELICS: A Very Large () Cluster Lens -- RXC J0032.1+1808

Ana Acebron, Adi Zitrin, Dan Coe +38

Extensive surveys with the \textit{Hubble Space Telescope} (HST) over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy-clust…

astro-ph.CO2019★ 80 cited

The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly Visibility During the Epoch of Reionization

Lily R. Whitler, Charlotte A. Mason, Keven Ren +5

The reionization of hydrogen is closely linked to the first structures in the universe, so understanding the timeline of reionization promises to shed light on the nature of these…

astro-ph.GA2019★ 2 cited

Prospects for extending the Mass-Metallicity Relation to low mass at high redshift: a case study at z~1

Alex Cameron, Tucker Jones, Tiantian Yuan +5

We report J-band MOSFIRE spectroscopy of a low-mass (log) star-forming galaxy at showing the detection of [NII] and [SII] alongside a…

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.GA2019★ 33 cited

The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation

Keven Ren, Michele Trenti, Charlotte A. Mason

The Ultraviolet Luminosity Function (UVLF) is a key observable for understanding galaxy formation from cosmic dawn. There has been considerable debate on whether Schechter-like LFs…

astro-ph.GA2019★ 3 cited

An Ultra Deep Field survey with WFIRST

Anton M. Koekemoer, R. J. Foley, D. N. Spergel +69

Studying the formation and evolution of galaxies at the earliest cosmic times, and their role in reionization, requires the deepest imaging possible. Ultra-deep surveys like the HU…