1.2k citations · 17.8k across the 216 of their papers we have counts for
9 papers · 1 filter
Inferences on the distribution of Ly-alpha emission of z~7 and z~8 galaxies
T. Treu, M. Trenti, M. Stiavelli +2
Spectroscopic confirmation of galaxies at z~7 and above has been extremely difficult, owing to a drop in intensity of Ly-alpha emission in comparison with samples at z~6. This cruc…
Overdensities of Y-dropout Galaxies from the Brightest-of-Reionizing Galaxies Survey: A Candidate Protocluster at Redshift z~8
M. Trenti, L. D. Bradley, M. Stiavelli +8
Theoretical and numerical modeling of dark-matter halo assembly predicts that the most luminous galaxies at high redshift are surrounded by overdensities of fainter companions. We…
UV-continuum slopes at z~4-7 from the HUDF09+ERS+CANDELS observations: Discovery of a well-defined UV-color magnitude relationship for z>=4 star-forming galaxies
R. J. Bouwens, G. D. Illingworth, P. A. Oesch +8
Ultra-deep ACS and WFC3/IR HUDF+HUDF09 data, along with the wide-area GOODS+ERS+CANDELS data over the CDF-S GOODS field, are used to measure UV colors, expressed as the UV-continuu…
Critical Star-Formation Rates for Reionization: Full Reionization occurs at z = 7
Michael Shull, Anthony Harness, Michele Trenti +1
We assess the probable redshift (z_rei ~ 7) for full reionization of the intergalactic medium (IGM) using a prescription for the co-moving star-formation-rate (SFR) density (rho_SF…
Morphological evolution of galaxies from ultradeep HST WFC3 imaging: the Hubble sequence at z~2
Daniel Szomoru, Marijn Franx, Rychard J. Bouwens +4
We use ultradeep HST WFC3/IR imaging of the HUDF to investigate the rest-frame optical morphologies of a mass-selected sample of galaxies at z~2. We find a large variety of galaxy…
The UDF05 Follow-up of the Hubble Ultra Deep Field. III. The Luminosity Function at z~6
Jian Su, Massimo Stiavelli, Pascal Oesch +13
In this paper, we present a derivation of the rest-frame 1400A luminosity function (LF) at redshift six from a new application of the maximum likelihood method by exploring the fiv…