<i>Euclid</i>preparation

Schirmer, M.; Jahnkę, K.; Seidel, G.; Aussel, H.; Bodendorf, C.; Grupp, F.; Hormuth, F.; Wachter, Stefanie; N. Appleton, P.; Barbier, R.; Brinchmann, J.; M. Carrasco, J.; J. Castander, F.; Coupon, J.; De Paolis, F.; Paula Gebert de Oliveira Franco, Ana; Ganga, K.; Hudelot, P.; Jullo, Eric; Lançon, A.; Nucita, Achille; Paltani, S.; Smadja, G.; Strafella, F.; M. Gaspar Venancio, Luis; Weiler, M.; Amara, A.; Auphan, T.; Auricchio, N.; Balestra, A.; Bender, R.; Bonino, D.; Branchini, E.; Brescia, M.; Capobianco, V.; Carbone, C.; Carretero, J.; Casas, R.; Castellano, M.; Cavuoti, S.; Cimatti, A.; Cledassou, R.; Congedo, G.; J. Conselice, Christopher; Copin, Y.; Copin, Y.; Corcione, L.; Costille, A.; Courbin, F.; Da Silva, A.

doi:10.1051/0004-6361/202142897

Public

Euclidpreparation

Shared by NobleBlocks on Apr 14, 2022 • 12:00 AM UTC

Authors:

M. Schirmer

K. Jahnkę

G. Seidel

Abstract

Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95–2.02 µm range, to a 5 σ point-source median depth of 24.4 AB mag. This unique photometric dataset will find wide use beyond Euclid’s core science. In this paper, we present accurate computations of the Euclid ...

Subject

Physics

Astrophysics

Astronomy

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