Forecasting [C II] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly
Abstract
We combine recent simulation work on the SFR–[C II] correlation at high redshift with empirical modeling of the galaxy–halo connection (via UniverseMachine) to forecast [C ii] auto power spectra from z ~ 4 to z ~ 8. We compare these to sensitivities realistically expected from various instruments expected to come online in the next decade. If the predictions of our model are correct, [C II] should be detectable up to z ~ 6 in this generation of surveys, but detecting [C II] past the end of reionization will require a generational leap in line-intensity survey capabilities.
- Authors:
-
- Stanford Univ., CA (United States)
- Stanford Univ., CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1616993
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 892; Journal Issue: 1; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Chung, Dongwoo T., Viero, Marco P., Church, Sarah E., and Wechsler, Risa H. Forecasting [C II] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly. United States: N. p., 2020.
Web. doi:10.3847/1538-4357/ab798f.
Chung, Dongwoo T., Viero, Marco P., Church, Sarah E., & Wechsler, Risa H. Forecasting [C II] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly. United States. https://doi.org/10.3847/1538-4357/ab798f
Chung, Dongwoo T., Viero, Marco P., Church, Sarah E., and Wechsler, Risa H. Fri .
"Forecasting [C II] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly". United States. https://doi.org/10.3847/1538-4357/ab798f. https://www.osti.gov/servlets/purl/1616993.
@article{osti_1616993,
title = {Forecasting [C II] Line-intensity Mapping Measurements between the End of Reionization and the Epoch of Galaxy Assembly},
author = {Chung, Dongwoo T. and Viero, Marco P. and Church, Sarah E. and Wechsler, Risa H.},
abstractNote = {We combine recent simulation work on the SFR–[C II] correlation at high redshift with empirical modeling of the galaxy–halo connection (via UniverseMachine) to forecast [C ii] auto power spectra from z ~ 4 to z ~ 8. We compare these to sensitivities realistically expected from various instruments expected to come online in the next decade. If the predictions of our model are correct, [C II] should be detectable up to z ~ 6 in this generation of surveys, but detecting [C II] past the end of reionization will require a generational leap in line-intensity survey capabilities.},
doi = {10.3847/1538-4357/ab798f},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 892,
place = {United States},
year = {Fri Mar 20 00:00:00 EDT 2020},
month = {Fri Mar 20 00:00:00 EDT 2020}
}
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