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ALMACAL VI : molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers.

Klitsch, Anne and Péroux, Céline and Zwaan, Martin A. and Smail, Ian and Nelson, Dylan and Popping, Gergö and Chen, Chian-Chou and Diemer, Benedikt and Ivison, R. J. and Allison, James R. and Muller, Sébastien and Swinbank, A. Mark and Hamanowicz, Aleksandra and Biggs, Andrew D. and Dutta, Rajeshwari (2019) 'ALMACAL VI : molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers.', Monthly notices of the Royal Astronomical Society., 490 (1). pp. 1220-1230.

Abstract

We are just starting to understand the physical processes driving the dramatic change in cosmic star-formation rate between z ∼ 2 and the present day. A quantity directly linked to star formation is the molecular gas density, which should be measured through independent methods to explore variations due to cosmic variance and systematic uncertainties. We use intervening CO absorption lines in the spectra of mm-bright background sources to provide a census of the molecular gas mass density of the Universe. The data used in this work are taken from ALMACAL, a wide and deep survey utilizing the ALMA calibrator archive. While we report multiple Galactic absorption lines and one intrinsic absorber, no extragalactic intervening molecular absorbers are detected. However, thanks to the large redshift path surveyed (Δz = 182), we provide constraints on the molecular column density distribution function beyond z ∼ 0. In addition, we probe column densities of N(H2) > 1016 atoms cm−2, five orders of magnitude lower than in previous studies. We use the cosmological hydrodynamical simulation IllustrisTNG to show that our upper limits of ρ(H2) ≲ 108.3M⊙Mpc−3 at 0 < z ≤ 1.7 already provide new constraints on current theoretical predictions of the cold molecular phase of the gas. These results are in agreement with recent CO emission-line surveys and are complementary to those studies. The combined constraints indicate that the present decrease of the cosmic star-formation rate history is consistent with an increasing depletion of molecular gas in galaxies compared to z ∼ 2.

Item Type:Article
Full text:(AM) Accepted Manuscript
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Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/stz2660
Publisher statement:This article has been accepted for publication in the Monthly notices of the Royal Astronomical Society ©: 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:17 September 2019
Date deposited:04 October 2019
Date of first online publication:21 September 2019
Date first made open access:15 October 2019

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