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The ALPINE-ALMA [C II] survey. Molecular gas budget in the early Universe as traced by [C II]

Dessauges-Zavadsky, M. and Ginolfi, M. and Pozzi, F. and Béthermin, M. and Le Fèvre, O. and Fujimoto, S. and Silverman, J. D. and Jones, G. C. and Vallini, L. and Schaerer, D. and Faisst, A. L. and Khusanova, Y. and Fudamoto, Y. and Cassata, P. and Loiacono, F. and Capak, P. L. and Yan, L. and Amorin, R. and Bardelli, S. and Boquien, M. and Cimatti, A. and Gruppioni, C. and Hathi, N. P. and Ibar, E. and Koekemoer, A. M. and Lemaux, B. C. and Narayanan, D. and Oesch, P. A. and Rodighiero, G. and Romano, M. and Talia, M. and Toft, S. and Vergani, D. and Zamorani, G. and Zucca, E. (2020) The ALPINE-ALMA [C II] survey. Molecular gas budget in the early Universe as traced by [C II]. Astronomy and Astrophysics, 643 . Art. No. A5. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20201028-123903558

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Abstract

The molecular gas content of normal galaxies at z >  4 is poorly constrained because the commonly used molecular gas tracers become hard to detect at these high redshifts. We use the [C II] 158 μm luminosity, which was recently proposed as a molecular gas tracer, to estimate the molecular gas content in a large sample of main sequence star-forming galaxies at z = 4.4 − 5.9, with a median stellar mass of 10^(9.7) M_⊙, drawn from the ALMA Large Program to INvestigate [C II] at Early times survey. The agreement between the molecular gas masses derived from [C II] luminosities, dynamical masses, and rest-frame 850 μm luminosities extrapolated from the rest-frame 158 μm continuum supports [C II] as a reliable tracer of molecular gas in our sample. We find a continuous decline of the molecular gas depletion timescale from z = 0 to z = 5.9, which reaches a mean value of (4.6 ± 0.8) × 10⁸ yr at z ∼ 5.5, only a factor of between two and three shorter than in present-day galaxies. This suggests a mild enhancement of the star formation efficiency toward high redshifts. Our estimates also show that the previously reported rise in the molecular gas fraction flattens off above z ∼ 3.7 to achieve a mean value of 63%±3% over z = 4.4 − 5.9. This redshift evolution of the gas fraction is in line with that of the specific star formation rate. We use multi-epoch abundance-matching to follow the gas fraction evolution across cosmic time of progenitors of z = 0 Milky Way-like galaxies in ∼10¹³ M_⊙ halos and of more massive z = 0 galaxies in ∼10¹⁴ M⊙ halos. Interestingly, the former progenitors show a monotonic increase of the gas fraction with redshift, while the latter show a steep rise from z = 0 to z ∼ 2 followed by a constant gas fraction from z ∼ 2 to z = 5.9. We discuss three possible effects, namely outflows, a pause in gas supply, and over-efficient star formation, which may jointly contribute to the gas fraction plateau of the latter massive galaxies.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361/202038231DOIArticle
https://arxiv.org/abs/2004.10771arXivDiscussion Paper
ORCID:
AuthorORCID
Dessauges-Zavadsky, M.0000-0003-0348-2917
Ginolfi, M.0000-0002-9122-1700
Pozzi, F.0000-0002-7412-647X
Béthermin, M.0000-0002-3915-2015
Le Fèvre, O.0000-0001-5891-2596
Fujimoto, S.0000-0001-7201-5066
Silverman, J. D.0000-0002-0000-6977
Jones, G. C.0000-0002-0267-9024
Vallini, L.0000-0002-3258-3672
Schaerer, D.0000-0001-7144-7182
Faisst, A. L.0000-0002-9382-9832
Khusanova, Y.0000-0002-7220-397X
Fudamoto, Y.0000-0001-7440-8832
Cassata, P.0000-0002-6716-4400
Loiacono, F.0000-0002-8858-6784
Capak, P. L.0000-0003-3578-6843
Yan, L.0000-0003-1710-9339
Amorin, R.0000-0001-5758-1000
Bardelli, S.0000-0002-8900-0298
Boquien, M.0000-0003-0946-6176
Cimatti, A.0000-0002-4409-5633
Gruppioni, C.0000-0002-3718-9180
Hathi, N. P.0000-0001-6145-5090
Koekemoer, A. M.0000-0002-6610-2048
Lemaux, B. C.0000-0002-1428-7036
Narayanan, D.0000-0002-7064-4309
Oesch, P. A.0000-0001-5851-6649
Rodighiero, G.0000-0002-9415-2296
Romano, M.0000-0002-9948-3916
Talia, M.0000-0003-4352-2063
Toft, S.0000-0003-3631-7176
Vergani, D.0000-0003-0898-2216
Zamorani, G.0000-0002-2318-301X
Zucca, E.0000-0002-5845-8132
Additional Information:© 2020 ESO. Article published by EDP Sciences. Received 22 April 2020; Accepted 17 July 2020; Published online 27 October 2020. This paper is dedicated to the memory of Olivier Le Fèvre, PI of the ALPINE survey. The ALPINE survey is based on data obtained with the ALMA Observatory, under Large Program 2017.1.00428.L. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This program receives financial support from the French CNRS-INSU Programme National Cosmologie et Galaxies. F.P., F.L., A.C., C.G., and M.T. acknowledge the support from grant PRIN MIUR 2017 – 20173ML3WW_s. S.F. is supported by the Cosmic Dawn Center of Excellence funded by the Danish National Research Foundation under the grant No. 140. J.D.S is supported by the JSPS KAKENHI Grant Number JP18H04346, and the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. G.C.J. acknowledges ERC Advanced Grant 695671 “QUENCH” and support by the Science and Technology Facilities Council (STFC). M.B. acknowledges FONDECYT regular grant 1170618. E.I. acknowledges partial support from FONDECYT through grant No. 1171710. S.T. acknowledges support from the European Research Council (ERC) Consolidator Grant funding scheme (project “ConTExt”, grant number: 648179). The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140. L.V. acknowledges funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant agreement No. 746119. We are grateful to the anonymous referee for providing a thorough report, which contributed to improve the quality paper.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Institut National des Sciences de l'Univers (INSU)UNSPECIFIED
Ministero dell'Istruzione, dell'Università e della Ricerca (MIUR)20173ML3WW_s
Danish National Research Foundation140
Japan Society for the Promotion of Science (JSPS)JP18H04346
Ministry of Education, Culture, Sports, Science and Technology (MEXT)UNSPECIFIED
European Research Council (ERC)695671
Science and Technology Facilities Council (STFC)UNSPECIFIED
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)1170618
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)1171710
European Research Council (ERC)648179
Marie Curie Fellowship746119
Subject Keywords:galaxies: evolution – galaxies: high-redshift – galaxies: ISM – ISM: molecules
Record Number:CaltechAUTHORS:20201028-123903558
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201028-123903558
Official Citation:The ALPINE-ALMA [C II] survey - Molecular gas budget in the early Universe as traced by [C II]. M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi, M. Béthermin, O. Le Fèvre, S. Fujimoto, J. D. Silverman, G. C. Jones, L. Vallini, D. Schaerer, A. L. Faisst, Y. Khusanova, Y. Fudamoto, P. Cassata, F. Loiacono, P. L. Capak, L. Yan, R. Amorin, S. Bardelli, M. Boquien, A. Cimatti, C. Gruppioni, N. P. Hathi, E. Ibar, A. M. Koekemoer, B. C. Lemaux, D. Narayanan, P. A. Oesch, G. Rodighiero, M. Romano, M. Talia, S. Toft, D. Vergani, G. Zamorani and E. Zucca. A&A, 643 (2020) A5; DOI: https://doi.org/10.1051/0004-6361/202038231
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106330
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Oct 2020 16:47
Last Modified:29 Oct 2020 16:47

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