MERLIN, EmilianoEmilianoMERLINFortuni, F.F.FortuniTorelli, M.M.TorelliSANTINI, PaolaPaolaSANTINICASTELLANO, MARCOMARCOCASTELLANOFONTANA, AdrianoAdrianoFONTANAGrazian, A.A.GrazianPENTERICCI, LauraLauraPENTERICCIPilo, S.S.PiloSchmidt, K. B.K. B.Schmidt2021-01-212021-01-2120190035-8711http://hdl.handle.net/20.500.12386/29913We search the five CANDELS fields (COSMOS, EGS, GOODS-North, GOODS-South, and UDS) for passively evolving a.k.a. `red and dead' massive galaxies in the first 2 Gyr after the big bang, integrating and updating the work on GOODS-South presented in a previous paper. We perform SED-fitting on photometric data, with top-hat star-formation histories to model an early and abrupt quenching, and using a probabilistic approach to select only robust candidates. Using libraries without (with) spectral lines emission, starting from a total of more than 20 000 z > 3 sources we end up with 102 (40) candidates, including one at z = 6.7. This implies a minimal number density of 1.73 ± 0.17 × 10<SUP>-5</SUP> (6.69 ± 1.08 × 10<SUP>-6</SUP>) Mpc<SUP>-3</SUP> for 3 < z < 5; applying a correction factor to account for incompleteness yields 2.30 ± 0.20 × 10<SUP>-5</SUP>. We compare these values with those from five recent hydrodynamical cosmological simulations, finding a reasonable agreement at z < 4; tensions arise at earlier epochs. Finally, we use the star-formation histories from the best-fitting models to estimate the contribution of the high-redshift passive galaxies to the global star formation rate density during their phase of activity, finding that they account for ∼5-10 per cent of the total star formation at 3 < z < 8, despite being only ∼ 0.5{{ per cent}} of the total in number. The resulting picture is that early and strong star formation activity, building massive galaxies on short time-scales and followed by a quick and abrupt quenching, is a rare but crucial phenomenon in the early Universe: the evolution of the cosmos must be heavily influenced by the short but powerful activity of these pristine monsters.STAMPAenArticle10.1093/mnras/stz26152-s2.0-85079652479000503993100015https://academic.oup.com/mnras/article/490/3/3309/55718252019MNRAS.490.3309MFIS/05 - ASTRONOMIA E ASTROFISICA