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High-resolution spectroscopic imaging of CO in a z=4.05 proto-cluster

, , , , and . (2013)cite arxiv:1307.4763Comment: Accepted to ApJ.

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Dynamical Characterization of Galaxies at z~4-6 via Tilted Ring Fitting to ALMA CII Observations, , , , , , , , , and . (2017)cite arxiv:1709.04954Comment: 20 pages, 6 figures, Accepted for publication in ApJ.No overdensity of Lyman Alpha Emitting Galaxies around a quasar at z~5.7, , , , , , and . (2016)cite arxiv:1611.02870Comment: Accepted by ApJ.Karl G. Jansky Very Large Array observations of cold dust and molecular gas in starbursting quasar host galaxies at z~4.5, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1401.1213Comment: 16 pages , 4 figures. Accepted for publication in ApJ.Constraining the Nature of Two Ly-alpha Emitters detected by ALMA at z = 4.7, , , , , , , , , and . (2014)cite arxiv:1401.3791Comment: 6 pages, 5 figures, accepted for publication in MNRAS.Very High Gas Fractions and Extended Gas Reservoirs in z = 1.5 Disk Galaxies, , , , , , , , , and 3 other author(s). \apj, (April 2010)CO excitation of normal star forming galaxies out to $z=1.5$ as regulated by the properties of their interstellar medium, , , , , , , , , and 8 other author(s). (2014)cite arxiv:1409.8158Comment: 18 pages, 17 figures, 4 tables, submitted to A&A.High-resolution spectroscopic imaging of CO in a z=4.05 proto-cluster, , , , and . (2013)cite arxiv:1307.4763Comment: Accepted to ApJ.A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1312.6365Comment: Accepted for publication in ApJ.Discovery of eight z ~ 6 quasars from Pan-STARRS1, , , , , , , , , and 17 other author(s). (2014)cite arxiv:1405.3986Comment: AJ in press, 16 pages, 5 figures, 7 tables.The kiloparsec-scale star formation law at redshift 4: wide-spread, highly efficient star formation in the dust-obscured starburst galaxy GN20, , , , , , and . (2014)cite arxiv:1412.2132Comment: 6 pages, 5 figures, accepted to ApJL.