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VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift

Castillo, Marta Frias; Hodge, Jacqueline; Rybak, Matus; van der Werf, Paul; Smail, Ian; Birkin, Jack E.; Chen, Chian-Chou; Chapman, Scott C.; Hill, Ryley; del P.Lagos, Claudia; Liao, Cheng-Lin; da Cunha, Elisabete; Rivera, Gabriela Calistro; Chen, Jianhang; Jiménez-Andrade, E.F.; Murphy, Eric J.; Scott, Douglas; Swinbank, A.M.; Walter, Fabian; Ivison, R.J.; Dannerbauer, Helmut

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Authors

Marta Frias Castillo

Jacqueline Hodge

Matus Rybak

Paul van der Werf

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Jack Birkin jack.birkin@durham.ac.uk
PGR Student Doctor of Philosophy

Chian-Chou Chen

Scott C. Chapman

Ryley Hill

Claudia del P.Lagos

Cheng-Lin Liao

Elisabete da Cunha

Gabriela Calistro Rivera

Jianhang Chen

E.F. Jiménez-Andrade

Eric J. Murphy

Douglas Scott

A.M. Swinbank

Fabian Walter

R.J. Ivison

Helmut Dannerbauer



Abstract

We present the initial results of an ongoing survey with the Karl G. Jansky Very Large Array targeting the CO(J = 1–0) transition in a sample of 30 submillimeter-selected, dusty star-forming galaxies (SFGs) at z = 2–5 with existing mid-J CO detections from the Atacama Large Millimeter/submillimeter Array and NOrthern Extended Millimeter Array, of which 17 have been fully observed. We detect CO(1–0) emission in 11 targets, along with three tentative (∼1.5σ–2σ) detections; three galaxies are undetected. Our results yield total molecular gas masses of 6–23 × 1010 (αCO/1) Me, with gas mass fractions, fgas = Mmol/(M*+Mmol), of 0.1–0.8 and a median depletion time of (140 ± 70) Myr. We find median CO excitation ratios of r31 = 0.75 ± 0.39 and r41 = 0.63 ± 0.44, with significant scatter. We find no significant correlation between the excitation ratio and a number of key parameters such as redshift, CO(1–0) line width, or ΣSFR. We only find a tentative positive correlation between r41 and the star-forming efficiency, but we are limited by our small sample size. Finally, we compare our results to predictions from the SHARK semi-analytical model, finding a good agreement between the molecular gas masses, depletion times, and gas fractions of our sources and their SHARK counterparts. Our results highlight the heterogeneous nature of the most massive SFGs at high redshift, and the importance of CO(1–0) observations to robustly constrain their total molecular gas content and interstellar medium properties.

Citation

Castillo, M. F., Hodge, J., Rybak, M., van der Werf, P., Smail, I., Birkin, J. E., …Dannerbauer, H. (2023). VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift. Astrophysical Journal, 945(2), Article 128. https://doi.org/10.3847/1538-4357/acb931

Journal Article Type Article
Acceptance Date Feb 1, 2023
Online Publication Date Mar 14, 2023
Publication Date Mar 10, 2023
Deposit Date Jun 12, 2023
Publicly Available Date Jun 12, 2023
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 945
Issue 2
Article Number 128
DOI https://doi.org/10.3847/1538-4357/acb931

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