activity
20072023
most citedThe VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1

56 citations · 115 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023

Identification and Characterization of Six Spectroscopically Confirmed Massive Protostructures at

Ekta A. Shah, Brian Lemaux, Benjamin Forrest +22

We present six spectroscopically confirmed massive protostructures, spanning a redshift range of in the Extended Chandra Deep Field South (ECDFS) field discovered as pa…

astro-ph.GA2023★ 18 cited

The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue

M. Talia, C. Schreiber, B. Garilli +36

VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted…

astro-ph.IM2022★ 22 cited

Euclid preparation: XXII. Selection of Quiescent Galaxies from Mock Photometry using Machine Learning

Euclid Collaboration, A. Humphrey, L. Bisigello +206

The Euclid Space Telescope will provide deep imaging at optical and near-infrared wavelengths, along with slitless near-infrared spectroscopy, across ~15,000 sq deg of the sky. Euc…

astro-ph.GA2022★ 18 cited

Euclid preparation. XXI. Intermediate-redshift contaminants in the search for galaxies within the Euclid Deep Survey

Euclid Collaboration, S. E. van Mierlo, K. I. Caputi +203

(Abridged) The Euclid mission is expected to discover thousands of z>6 galaxies in three Deep Fields, which together will cover a ~40 deg2 area. However, the limited number of Eucl…

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…