Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors

التفاصيل البيبلوغرافية
العنوان: Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors
المؤلفون: Kiyoto Yabe, Carlos Gómez-Guijarro, Sune Toft, Iary Davidzon, Georgios E. Magdis, Martin Sparre, Olivier Ilbert, Johannes Zabl, Gabriel B. Brammer, Masato Onodera, Andreas L. Faisst, Mikkel Stockmann, Christopher C. Hayward, Masayuki Tanaka, Charles L. Steinhardt, Daniel Ceverino, Anna Gallazzi, Mariko Kubo, Francesco Valentino, Jonatan Selsing, Rhythm Shimakawa
المساهمون: Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
المصدر: The Astrophysical Journal
The Astrophysical Journal, 2020, 889, ⟨10.3847/1538-4357/ab64dc⟩
Valentino, F, Tanaka, M, Davidzon, I, Toft, S, Gomez-Guijarro, C, Stockmann, M, Onodera, M, Brammer, G, Ceverino, D, Faisst, A L, Gallazzi, A, Hayward, C C, Ilbert, O, Kubo, M, Magdis, G E, Selsing, J, Shimakawa, R, Sparre, M, Steinhardt, C, Yabe, K & Zabl, J 2020, ' Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors ', Astrophysical Journal, vol. 889, no. 2, 93 . https://doi.org/10.3847/1538-4357/ab64dc
Valentino, F, Tanaka, M, Davidzon, I, Toft, S, Gómez-Guijarro, C, Stockmann, M, Onodera, M, Brammer, G, Ceverino, D, Faisst, A L, Gallazzi, A, Hayward, C C, Ilbert, O, Kubo, M, Magdis, G E, Selsing, J, Shimakawa, R, Sparre, M, Steinhardt, C, Yabe, K & Zabl, J 2020, ' Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors ', Astrophysical Journal, vol. 889, no. 2, 93 . https://doi.org/10.3847/1538-4357/ab64dc
بيانات النشر: HAL CCSD, 2020.
سنة النشر: 2020
مصطلحات موضوعية: 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Emission spectrum, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Physics, Very Large Telescope, Star formation, Astronomy and Astrophysics, Billion years, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Space and Planetary Science, [SDU]Sciences of the Universe [physics], Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Earth and Planetary Astrophysics
الوصف: We report two secure ($z=3.775, 4.012$) and one tentative ($z\approx3.767$) spectroscopic confirmations of massive and quiescent galaxies through $K$-band observations with Keck/MOSFIRE and VLT/X-Shooter. The stellar continuum emission, the absence of strong nebular emission lines and the lack of significant far-infrared detections confirm the passive nature of these objects, disfavoring the alternative solution of low-redshift dusty star-forming interlopers. We derive stellar masses of $\mathrm{log}(M_{\star}/M_\odot)\sim11$ and ongoing star formation rates placing these galaxies $\gtrsim 1-2$ dex below the main sequence at their redshifts. The adopted parametrization of the star formation history suggests that these sources experienced a strong ($\langle \rm SFR \rangle \sim 1200-3500\,M_\odot\,\mathrm{yr}^{-1}$) and short ($\sim 50$ Myr) burst of star formation, peaking $\sim 150-500$ Myr before the time of observation, all properties reminiscent of the characteristics of sub-millimeter galaxies (SMGs) at $z>4$. We investigate this connection by comparing the comoving number densities and the properties of these two populations. We find a fair agreement only with the deepest sub-mm surveys detecting not only the most extreme starbursts, but also more normal galaxies. We support these findings by further exploring the Illustris-TNG cosmological simulation, retrieving populations of both fully quenched massive galaxies at $z\sim3-4$ and SMGs at $z\sim4-5$, with number densities and properties in agreement with the observations at $z\sim3$, but in increasing tension at higher redshift. Nevertheless, as suggested by the observations, not all the progenitors of quiescent galaxies at these redshifts shine as bright SMGs in their past and, similarly, not all bright SMGs quench by $z\sim3$, both fractions depending on the threshold assumed to define the SMGs themselves.
20 pages (+appendix), 11 figures, accepted for publication in the Astrophysical Journal (ApJ). This work comes with a companion letter by Tanaka, Valentino, Toft et al. 2019, ApJL, 885, L34
وصف الملف: application/pdf
اللغة: English
تدمد: 0004-637X
1538-4357
0004-6361
1538-3873
0067-0049
DOI: 10.3847/1538-4357/ab64dc⟩
DOI: 10.3847/1538-4357/ab64dc
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e90f7ee551a4052e975d9f903c939d11
https://hal-insu.archives-ouvertes.fr/insu-03667136
Rights: OPEN
رقم الانضمام: edsair.doi.dedup.....e90f7ee551a4052e975d9f903c939d11
قاعدة البيانات: OpenAIRE
الوصف
تدمد:0004637X
15384357
00046361
15383873
00670049
DOI:10.3847/1538-4357/ab64dc⟩