activity
20022022
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 2.7k across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.GA2022★ 15 cited

The PAU Survey: Measurements of the 4000 Å spectral break with narrow-band photometry

Pablo Renard, Małgorzata Siudek, Martin B. Eriksen +19

The D4000 spectral break index is one of the most important features in the visible spectrum, as it is a proxy for stellar ages and is also used in galaxy classification. However,…

astro-ph.CO2021★ 2 cited

Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3

Euclid Collaboration, S. A. Stanford, D. Masters +183

The Complete Calibration of the Color-Redshift Relation (C3R2) survey is obtaining spectroscopic redshifts in order to map the relation between galaxy color and redshift to a depth…

astro-ph.GA2021★ 23 cited

The PAU Survey: Measurement of Narrow-band galaxy properties with Approximate Bayesian Computation

Luca Tortorelli, Malgorzata Siudek, Beatrice Moser +22

Narrow-band imaging surveys allow the study of the spectral characteristics of galaxies without the need of performing their spectroscopic follow-up. In this work, we forward-model…

astro-ph.CO2021★ 30 cited

Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data

M. Martinelli, C. J. A. P. Martins, S. Nesseris +92

In physically realistic scalar-field based dynamical dark energy models (including, e.g., quintessence) one naturally expects the scalar field to couple to the rest of the model's…

astro-ph.IM2021★ 4 cited

Euclid: Estimation of the impact of correlated readout noise for flux measurements with the Euclid NISP instrument

A. Jimenez Munoz, J. Macias-Perez, A. Secroun +96

The Euclid satellite, to be launched by ESA in 2022, will be a major instrument for cosmology for the next decades. \Euclid\ is composed of two instruments: the Visible (VIS) instr…

astro-ph.CO2021★ 26 cited

Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses

Euclid Collaboration, A. Pocino, I. Tutusaus +157

The accuracy of photometric redshifts (photo-zs) particularly affects the results of the analyses of galaxy clustering with photometrically-selected galaxies (GCph) and weak lensin…