activity
20182026
most citedThe PAU Survey: Early demonstration of photometric redshift performance in the COSMOS field

69 citations · 538 across the 43 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023★ 13 cited

Exploring the low-mass regime of galaxy-scale strong lensing: Insights into the mass structure of cluster galaxies

Giovanni Granata, Pietro Bergamini, Claudio Grillo +8

We aim at a direct measurement of the compactness of three galaxy-scale lenses in massive clusters, testing the accuracy of the scaling laws that describe the members in strong len…

astro-ph.GA2023

The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation

G. Manzoni, C. M. Baugh, P. Norberg +27

We use the GALFORM semi-analytical galaxy formation model implemented in the Planck Millennium N-body simulation to build a mock galaxy catalogue on an observer's past lightcone. T…

astro-ph.GA2023★ 7 cited

Fast Forward Modelling of Galaxy Spatial and Statistical Distributions

Pascale Berner, Alexandre Refregier, Beatrice Moser +3

A forward modelling approach provides simple, fast and realistic simulations of galaxy surveys, without a complex underlying model. For this purpose, galaxy clustering needs to be…

astro-ph.GA2023★ 11 cited

The Kormendy relation of early-type galaxies as a function of wavelength in Abell S1063, MACS J0416.1-2403, and MACS J1149.5+2223

L. Tortorelli, A. Mercurio, G. Granata +9

The wavelength dependence of the Kormendy relation (KR) is well characterised at low redshift but poorly studied at intermediate redshifts. The KR provides information on the evolu…

astro-ph.GA2023★ 1 cited

: An automated galaxy structural parameters fitting package

Luca Tortorelli, Amata Mercurio

In today's modern wide-field galaxy surveys, there is the necessity for parametric surface brightness decomposition codes characterised by accuracy, small degree of user interventi…

astro-ph.CO2023★ 8 cited

Searching for galaxy-scale strong-lenses in galaxy clusters with deep networks -- I: methodology and network performance

G. Angora, P. Rosati, M. Meneghetti +10

Galaxy-scale strong lenses in galaxy clusters provide a unique tool to investigate their inner mass distribution and the sub-halo density profiles in the low-mass regime, which can…