activity
19942023
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 12.7k across the 142 of their papers we have counts for

collaborators

142 papers

astro-ph.GA2023★ 2 cited

MIDIS: Unveiling the Role of Strong Ha-emitters during the Epoch of Reionization with JWST

P. Rinaldi, K. I. Caputi, E. Iani +40

By using the ultra-deep \textit{JWST}/MIRI image at 5.6 in the Hubble eXtreme Deep Field, we constrain the role of strong H-emitters (HAEs) during Cosmic Reionization at $z…

astro-ph.GA2023★ 158 cited

Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey

Pablo G. Pérez-González, Luca Costantin, Danial Langeroodi +41

We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at derived from deep NIRCam observations taken in parallel with th…

astro-ph.GA2022★ 15 cited

The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at with [OII] and [CII] Line Emission ISM Properties and [OII]SFR Relation

Brittany N. Vanderhoof, A. L. Faisst, L. Shen +23

We present main-sequence ALPINE galaxies (log() = 9.2-11.1 and ) at with optical [OII] measurements from Ke…

astro-ph.GA2021★ 59 cited

The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5

M. Romano, P. Cassata, L. Morselli +25

Galaxy mergers are thought to be one of the main mechanisms of the mass assembly of galaxies. Recently, many works have suggested a possible increase in the fraction of major merge…

astro-ph.GA2021★ 43 cited

The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe

F. Pozzi, F. Calura, Y. Fudamoto +32

The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observa…

astro-ph.CO2021★ 8 cited

The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS

R. Thomas, L. Pentericci, O. Le Fèvre +22

Aim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift g…