No Evidence for Millimeter Continuum Source Overdensities in the Environments of z ≳ 6 Quasars-Reference-Cited by-同舟云学术

No Evidence for Millimeter Continuum Source Overdensities in the Environments of z ≳ 6 Quasars

Published:2018-11-12 Issue:2 Volume:867 Page:153
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Champagne Jaclyn B.^ORCID,Decarli Roberto^ORCID,Casey Caitlin M.^ORCID,Venemans Bram^ORCID,Bañados Eduardo^ORCID,Walter Fabian^ORCID,Bertoldi Frank^ORCID,Fan Xiaohui^ORCID,Farina Emanuele Paolo^ORCID,Mazzucchelli Chiara^ORCID,Riechers Dominik A.^ORCID,Strauss Michael A.^ORCID,Wang Ran,Yang Yujin^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/867/i=2/a=153/pdf

Reference129 articles.

1. Cosmological Parameters from Observations of Galaxy Clusters

2. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND, AND PROPERTIES OF THE FAINTEST DUSTY STAR-FORMING GALAXIES

3. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: SEARCH FOR [${\rm{C}}\,{\rm{II}}$] LINE AND DUST EMISSION IN 6

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