Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202243950e]


Table 2.

Scenarios of simulated data availability in the Euclid Deep Fields considered in this work.

Scenario Description z = 1–6 z = 6–8
Euclid Euclid IE,YE,JE,HE 175 652 315
Euclid + Rubin Euclid IE,YE,JE,HE; Rubin ugrizy (depth after 10 years) 175 652 315
Euclid + Rubin DDF Euclid IE,YE,JE,HE; Rubin ugrizy (Deep Drilling Fields depth) 175 652 315
Euclid + H20 Euclid IE,YE,JE,HE; CFHT u and Subaru HSC griz 175 652 315
Euclid + Spitzer Euclid IE,YE,JE,HE; Spitzer IRAC 3.6 and 4.5 μm 134 562 203
Euclid + Rubin + Spitzer Euclid IE,YE,JE,HE; Rubin ugrizy (depth after 10 years); 134 562 203
Spitzer IRAC 3.6 and 4.5 μm
Euclid + Rubin DDF + Spitzer Euclid IE,YE,JE,HE; Rubin ugrizy (Deep Drilling Fields depth); 134 562 203
Spitzer IRAC 3.6 and 4.5 μm
Euclid + H20 + Spitzer Euclid IE,YE,JE,HE; CFHT u and Subaru HSC griz; Spitzer IRAC 3.6 and 4.5 μm 134 562 203

Photometry 2σ limiting magnitude [AB]

Euclid IE = 29.2; YE = 27.3; JE = 27.5; HE = 27.4
Rubin (10 yr depth) u = 27.1; g = 28.4; r = 28.5; i = 27.8; z = 27.1; y = 25.9
Rubin (DDF depth) u = 27.8; g = 29.4; r = 29.5; i = 29.3; z = 29.0; y = 27.2
H20 u = 27.2; g = 28.5; r = 28.5; i = 28.0; z = 27.5
Spitzer [3.6] = 25.8; [4.5] = 25.7

Notes. Summary of the eight scenarios of combinations of Euclid and ancillary data considered in this work and the corresponding 2σ magnitude limits that were applied to the photometry. The number of intermediate-z and high-z galaxies that are inserted in our simulations (based on their fiducial redshift) is indicated in the last two columns.

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