activity
19942025
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 27.9k across the 311 of their papers we have counts for

collaborators
Showing 2020Show all

14 papers · 1 filter

astro-ph.CO2020

Euclid: Forecasts for -cut Point Statistics

P. L. Taylor, T. Kitching, V. F. Cardone +92

Modelling uncertainties at small scales, i.e. high in the power spectrum , due to baryonic feedback, nonlinear structure growth and the fact that galaxies are biased trac…

astro-ph.EP2020★ 13 cited

Euclid: Identification of asteroid streaks in simulated images using StreakDet software

M. Pöntinen, M. Granvik, A. A. Nucita +57

The ESA Euclid space telescope could observe up to 150 000 asteroids as a side product of its primary cosmological mission. Asteroids appear as trailed sources, that is streaks, in…

astro-ph.CO2020★ 166 cited

Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations

Euclid Collaboration, M. Knabenhans, J. Stadel +131

We present a new, updated version of the EuclidEmulator (called EuclidEmulator2), a fast and accurate predictor for the nonlinear correction of the matter power spectrum. Percent-l…

astro-ph.GA2020★ 114 cited

Euclid preparation: X. The Euclid photometric-redshift challenge

Euclid Collaboration, G. Desprez, S. Paltani +170

Forthcoming large photometric surveys for cosmology require precise and accurate photometric redshift (photo-z) measurements for the success of their main science objectives. Howev…

astro-ph.GA2020★ 70 cited

The VIMOS Ultra Deep Survey: The reversal of the star-formation rate density relation at

B. C. Lemaux, O. Cucciati, O. Le Fèvre +28

Utilizing spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS), new observations from Keck/DEIMOS, and publicly available observations of large samples of star-f…

astro-ph.GA2020

MOONRISE: The Main MOONS GTO Extragalactic Survey

R. Maiolino, M. Cirasuolo, J. Afonso +34

The MOONS instrument possesses an exceptional combination of large multiplexing, high sensitivity, broad simultaneous spectral coverage (from optical to near-infrared bands), large…

astro-ph.GA2020★ 22 cited

Euclid preparation: VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release

Euclid Collaboration, V. Guglielmo, R. Saglia +145

The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic effort involving ESO and Keck facilities designed to empirically calibrate the galaxy colo…

astro-ph.CO2020★ 76 cited

Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes

M. Martinelli, C. J. A. P. Martins, S. Nesseris +82

In metric theories of gravity with photon number conservation, the luminosity and angular diameter distances are related via the Etherington relation, also known as the distance-du…

astro-ph.CO2020★ 53 cited

Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey

I. Tutusaus, M. Martinelli, V. F. Cardone +87

The data from the Euclid mission will enable the measurement of the photometric redshifts, angular positions, and weak lensing shapes for over a billion galaxies. This large datase…

astro-ph.GA2020★ 22 cited

Euclid: The selection of quiescent and star-forming galaxies using observed colours

L. Bisigello, U. Kuchner, C. J. Conselice +71

The Euclid mission will observe well over a billion galaxies out to and beyond. This will offer an unrivalled opportunity to investigate several key questions for understa…

astro-ph.GA2020★ 20 cited

The role of galaxy mass on AGN emission: a view from the VANDELS survey

M. Magliocchetti, L. Pentericci, M. Cirasuolo +13

We present a comparative analysis of the properties of AGN emitting at radio and X-ray wavelengths. The study is performed on 907 X-ray AGN and 100 radio AGN selected on the CDFS a…

astro-ph.IM2020★ 9 cited

CHIPP: INAF pilot project for HTC, HPC and HPDA

Giuliano Taffoni, Ugo Becciani, Bianca Garilli +5

CHIPP (Computing HTC in INAF Pilot Project) is an Italian project funded by the Italian Institute for Astrophysics (INAF) and promoted by the ICT office of INAF. The main purpose o…

astro-ph.GA2020★ 88 cited

Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5

A. C. Carnall, S. Walker, R. J. McLure +19

We present a sample of 151 massive () quiescent galaxies at , based on a sophisticated Bayesian spectral energy distribution fitting analy…

astro-ph.GA2020★ 34 cited

The VANDELS survey: A strong correlation between Ly equivalent width and stellar metallicity at

F. Cullen, R. J. McLure, J. S. Dunlop +26

We present the results of a new study investigating the relationship between observed Ly equivalent width ((Ly)) and the metallicity of the ionizing stellar population (…