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Probing Cosmic Reionization and Molecular Gas Growth with TIME

Sun, G. and Chang, T.-C. and Uzgil, B. D. and Bock, J. J. and Bradford, C. M. and Butler, V. and Caze-Cortes, T. and Cheng, Y.-T. and Cooray, A. and Crites, A. T. and Hailey-Dunsheath, S. and Emerson, N. and Frez, C. and Hoscheit, B. L. and Hunacek, J. and Keenan, R. P. and Li, C. T. and Madonia, P. and Marrone, D. P. and Moncelsi, L. and Shiu, C. and Trumper, I. and Turner, A. and Weber, A. and Wei, T. S. and Zemcov, M. (2020) Probing Cosmic Reionization and Molecular Gas Growth with TIME. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20210224-085555089

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Abstract

Line intensity mapping (LIM) provides a unique and powerful means to probe cosmic structures by measuring the aggregate line emission from all galaxies across redshift. The method is complementary to conventional galaxy redshift surveys that are object-based and demand exquisite point-source sensitivity. The Tomographic Ionized-carbon Mapping Experiment (TIME) will measure the star formation rate (SFR) during cosmic reionization by observing the redshifted [C II] 158μm line (6 ≲ z ≲ 9) in the LIM regime. TIME will simultaneously study the abundance of molecular gas during the era of peak star formation by observing the rotational CO lines emitted by galaxies at 0.5 ≲ z ≲ 2. We present the modeling framework that predicts the constraining power of TIME on a number of observables, including the line luminosity function, and the auto- and cross-correlation power spectra, including synergies with external galaxy tracers. Based on an optimized survey strategy and fiducial model parameters informed by existing observations, we forecast constraints on physical quantities relevant to reionization and galaxy evolution, such as the escape fraction of ionizing photons during reionization, the faint-end slope of the galaxy luminosity function at high redshift, and the cosmic molecular gas density at cosmic noon. We discuss how these constraints can advance our understanding of cosmological galaxy evolution at the two distinct cosmic epochs for TIME, starting in 2021, and how they could be improved in future phases of the experiment.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/2012.09160arXivDiscussion Paper
ORCID:
AuthorORCID
Sun, G.0000-0003-4070-497X
Chang, T.-C.0000-0001-5929-4187
Uzgil, B. D.0000-0001-8526-3464
Bock, J. J.0000-0002-5710-5212
Bradford, C. M.0000-0001-5261-7094
Cheng, Y.-T.0000-0002-5437-0504
Cooray, A.0000-0002-3892-0190
Hailey-Dunsheath, S.0000-0002-8504-7988
Marrone, D. P.0000-0002-2367-1080
Moncelsi, L.0000-0002-4242-3015
Zemcov, M.0000-0001-8253-1451
Additional Information:We would like to thank Lluis Mas-Ribas for helpful comments on the manuscript and Lin Yan for discussion about the [C II] luminosity function measured from ALPINE survey. We are also grateful for Garrett (Karto) Keating for compiling the observational constraints on molecular gas density. TCC and GS acknowledge support from the JPL Strategic R&TD awards. AC acknowledges support from NSF AST-1313319 and 2015-2016 UCI Office of Research Seed Funding Award. DPM and RPK were supported by the National Science Foundation through CAREER grant AST-1653228. RPK was supported by the National Science Foundation through Graduate Research Fellowship grant DGE-1746060. ATC was supported by a KISS postdoctoral fellowship and a National Science Foundation Astronomy and Astrophysics Postdoctoral Fellowship under Grant No. 1602677. This work is supported by National Science Foundation award number 1910598. Part of the research described in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Software: ares (Mirocha et al. 2017), corner (Foreman-Mackey 2016), emcee (Foreman-Mackey et al. 2013), matplotlib (Hunter 2007), numpy (Walt et al. 2011), pygtc (Bocquet & Carter 2016), and scipy (Jones et al. 2001).
Group:Astronomy Department, Keck Institute for Space Studies
Funders:
Funding AgencyGrant Number
JPL Research and Technology Development FundUNSPECIFIED
NSFAST-1313319
University of California, IrvineUNSPECIFIED
NSFAST-1653228
NSF Graduate Research FellowshipDGE-1746060
Keck Institute for Space Studies (KISS)UNSPECIFIED
NSF Astronomy and Astrophysics FellowshipAST-1602677
NSFAST-1910598
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:cosmology: observations – theory – dark ages, reionization, first stars – large-scale structure of universe – galaxies: ISM
Record Number:CaltechAUTHORS:20210224-085555089
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210224-085555089
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:108164
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 Feb 2021 20:40
Last Modified:24 Feb 2021 20:40

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