activity
19992023
most citedEuclid preparation. XVIII. The NISP photometric system

85 citations · 303 across the 8 of their papers we have counts for

collaborators

8 papers

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.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-ph.IM2022★ 85 cited

Euclid preparation. XVIII. The NISP photometric system

Euclid Collaboration, M. Schirmer, K. Jahnke +220

Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95-2.02 m range, to a 5 point-source median depth of 24.4 AB mag. This unique photomet…

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-ph2008★ 75 cited

SPACE: the SPectroscopic All-sky Cosmic Explorer

A. Cimatti, M. Robberto, C. M. Baugh +18

We describe the scientific motivations, the mission concept and the instrumentation of SPACE, a class-M mission proposed for concept study at the first call of the ESA Cosmic-Visio…

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…