| DOI | Resolve DOI: https://doi.org/10.3847/1538-4357/ab63dd |
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| Author | Search for: Miller, Tim B.1; Search for: Chapman, Scott C.1; Search for: Hayward, Christopher C.ORCID identifier: https://orcid.org/0000-0003-4073-3236; Search for: Behroozi, Peter S.; Search for: Bradford, Matt; Search for: Willott, Chris J.1ORCID identifier: https://orcid.org/0000-0002-4201-7367; Search for: Wagg, Jeff |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Abstract | We present a search for companion [C ii] emitters to known luminous sources at 6 < z < 6.5 in deep, archival ALMA observations. The observations are deep enough to detect sources with L [C ii] ~10⁸ L⊙ at z ~ 6. We identify three new robust line detections from a blind search of five deep fields centered on ultraluminous infrared galaxies and QSOs. We calculate the volume density of companions and find a relative overdensity of 6₋₃⁺⁴ and 86₋₃₇⁺⁶⁰ when comparing to current observational constraints and theoretical predictions, respectively. These results suggest that the central sources may be highly biased tracers of mass in the early universe. We find these companion lines to have comparable properties to other known galaxies at the same epoch. All companions lie less than 650 km s⁻¹ and between 25 and 60 kpc (projected) from their central source. To place these discoveries in context, we employ a mock galaxy catalog to estimate the luminosity function for [C ii] during reionization and compare to our observations. The simulations support this result by showing a similar level of elevated counts found around such luminous [C ii] sources. |
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| Publication date | 2020-01-29 |
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| Publisher | IOP Publishing |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 9c82a7ac-e4ca-48cf-9044-8a7a7bdd3cac |
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| Record created | 2020-07-08 |
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| Record modified | 2021-09-17 |
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