activity
20072026
most citedNew Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency

419 citations · 7.9k across the 126 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

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★ 75 cited

Extremely Small Sizes for Faint z~2-8 Galaxies in the Hubble Frontier Fields: A Key Input For Establishing their Volume Density and UV Emissivity

R. J. Bouwens, G. D. Illingworth, P. A. Oesch +3

We provide the first observational constraints on the sizes of the faintest galaxies lensed by the Hubble Frontier Fields (HFF) clusters. Ionizing radiation from faint galaxies lik…

astro-ph.CO2016★ 140 cited

The Extraordinary Amount of Substructure in the Hubble Frontier Fields Cluster Abell 2744

M. Jauzac, D. Eckert, J. Schwinn +21

We present a joint optical/X-ray analysis of the massive galaxy cluster Abell 2744 (z=0.308). Our strong- and weak-lensing analysis within the central region of the cluster, i.e.,…

astro-ph.HE2016★ 37 cited

Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs. II: star formation rates and metallicities at z < 1

J. Japelj, S. D. Vergani, R. Salvaterra +21

Long gamma-ray bursts (LGRBs) are associated with the deaths of massive stars and could thus be a potentially powerful tool to trace cosmic star formation. However, especially at l…

astro-ph.GA2016★ 16 cited

The role of quenching time in the evolution of the mass-size relation of passive galaxies from the WISP survey

A. Zanella, C. Scarlata, E. M. Corsini +13

We analyze how passive galaxies at z 1.5 populate the mass-size plane as a function of their stellar age, to understand if the observed size growth with time can be explaine…

astro-ph.GA2016★ 11 cited

The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field

I. Baronchelli, C. Scarlata, G. Rodighiero +25

We present the Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole (SEP) field. The large area covered (7.7 deg), together with one of the lowest Galactic…