activity
20182022
most citedThe web of the Giant: spectroscopic confirmation of a Large Scale Structure around the z=6.31 quasar SDSS J1030+0524

48 citations · 94 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202224 cited

SFR estimations from z=0 to z=0.9 -- A comparison of SFR calibrators for star-forming galaxies

M. Figueira, A. Pollo, K. Małek +7

Using VIPERS, we estimated a set of SFR based on photometric and spectroscopic data. We used, as estimators, photometric bands from ultraviolet to mid-infrared, and spectral lines.…

astro-ph.HE202216 cited

The central engine of the highest redshift blazar

Silvia Belladitta, Alessandro Caccianiga, Alessandro Diana +8

We report on a LUCI/Large Binocular Telescope near-infrared (NIR) spectrum of PSO J030947.49+271757.31 (hereafter PSO J0309+27), the highest redshift blazar known to date (z6…

astro-ph.GA202048 cited

The web of the Giant: spectroscopic confirmation of a Large Scale Structure around the z=6.31 quasar SDSS J1030+0524

Marco Mignoli, Roberto Gilli, Roberto Decarli +14

We report on the spectroscopic confirmation of a large scale structure around the luminous, z=6.31 QSO SDSS~J1030+0524, that is powered by a billion solar mass black hole. The stru…

astro-ph.GA20206 cited

The VIMOS Ultra-Deep Survey: the Ly emission line morphology at

B. Ribeiro, O. Le Fèvre, A. Paulino-Afonso +20

The Lyman- (Ly) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMO…

astro-ph.CO2020

The first blazar observed at z>6

S. Belladitta, A. Moretti, A. Caccianiga +9

We present the discovery of PSO J030947.49+271757.31, the radio brightest (23.7 mJy at 1.4 GHz) active galactic nucleus (AGN) at z>6.0. It was selected by cross-matching the NRAO V…

astro-ph.GA2019

The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index

R. Thomas, O. Le Fèvre, G. Zamorani +10

Aims. We seek is to identify old and massive galaxies at 0.5<z<2.1 on the basis of the magnesium index MgUV and then study their physical properties. We computed the MgUV index bas…