activity
20072022
most citedThe ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

173 citations · 302 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2022★ 19 cited

The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation

Michael Romano, L. Morselli, P. Cassata +22

The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…

astro-ph.GA2020★ 173 cited

The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr

D. Schaerer, M. Ginolfi, M. Bethermin +34

The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…

astro-ph.GA2018★ 53 cited

The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to

Louis Legrand, Henry Joy McCracken, Iary Davidzon +7

Using precise galaxy stellar mass function measurements in the COSMOS field we determine the stellar-to-halo mass relationship (SHMR) using a parametric abundance matching techniqu…

astro-ph2008★ 1 cited

Testing gravity on large scales. The skewness of the galaxy distribution at z~1

C. Marinoni, L. Guzzo, A. Cappi +54

We study the evolution of the low-order moments of the galaxy overdensity distribution over the redshift interval 0.7<z<1.5. We find that the variance and the normalized skewness e…

astro-ph2007★ 56 cited

The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1

B. Meneux, L. Guzzo, B. Garilli +43

Aims: We use the VVDS-Deep first-epoch data to measure the dependence of galaxy clustering on galaxy stellar mass, at z~0.85. Methods: We measure the projected correlation function…