Investigating Overdensities around z > 6 Galaxies through ALMA Observations of [C ii]
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab63dd/pdf
Reference57 articles.
1. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: SEARCH FOR [${\rm{C}}\,{\rm{II}}$] LINE AND DUST EMISSION IN 6
2. THE GALAXY ENVIRONMENT OF A QSO ATz∼ 5.7
3. IS THERE A MAXIMUM STAR FORMATION RATE IN HIGH-REDSHIFT GALAXIES?, , ,
4. UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
5. THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROMz= 0-8
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1. The interstellar medium distribution, gas kinematics, and system dynamics of the far-infrared luminous quasar SDSS J2310+1855 at z = 6.0;Astronomy & Astrophysics;2022-12
2. Constraining Galaxy Overdensities around Three z ∼ 6.5 Quasars with ALMA and MUSE;The Astrophysical Journal;2022-03-01
3. Clustering of red and blue galaxies around high-redshift 3C radio sources as seen by the Hubble Space Telescope;Astronomy & Astrophysics;2021-09
4. FIR-luminous [C ii] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z ∼ 4.6;The Astrophysical Journal;2021-02-01
5. Submillimetre galaxies in cosmological hydrodynamical simulations – an opportunity for constraining feedback models;Monthly Notices of the Royal Astronomical Society;2021-01-29
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