activity
20032018
most citedTowards a complete treatment of the cosmological recombination problem

131 citations · 561 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2018★ 122 cited

The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS

O. Cucciati, B. C. Lemaux, G. Zamorani +22

[Abridged] We unveil the complex shape of a proto-supercluster at z~2.45 in the COSMOS field using the spectroscopic redshifts of the VIMOS Ultra-Deep Survey (VUDS), complemented b…

astro-ph.GA2017★ 103 cited

The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57

B. C. Lemaux, O. Le Fèvre, O. Cucciati +20

Using spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS) we report here on the discovery of PCl J1001+0220, a massive proto-cluster located at $z_{spec}\sim4.5…

astro-ph.GA2016★ 48 cited

Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field

L. Guaita, L. Pentericci, A. Grazian +23

Aim: We aim to measure the LyC signal from a sample of sources in the Chandra deep field south. We collect star-forming galaxies (SFGs) and active galactic nuclei (AGN) with accura…

astro-ph.CO2015★ 20 cited

Simulating the 21cm forest detectable with LOFAR and SKA in the spectra of high-z GRBs

B. Ciardi, S. Inoue, F. B. Abdalla +26

We investigate the feasibility of detecting 21cm absorption features in the afterglow spectra of high redshift long Gamma Ray Bursts (GRBs). This is done employing simulations of c…

astro-ph.GA2015★ 48 cited

The VIMOS Ultra Deep Survey: Ly Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5

Nimish P. Hathi, O. Le Fèvre, O. Ilbert +45

The aim of this paper is to investigate spectral and photometric properties of 854 faint (<~25 mag) star-forming galaxies (SFGs) at 2<z<2.5 using the VIMOS Ultra-Deep Surve…

astro-ph.CO2012★ 51 cited

Imaging neutral hydrogen on large-scales during the Epoch of Reionization with LOFAR

S. Zaroubi, A. G. de Bruyn, G. Harker +17

The first generation of redshifted 21 cm detection experiments, carried out with arrays like LOFAR, MWA and GMRT, will have a very low signal-to-noise ratio per resolution element…