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Most Luminous z=9-10 Galaxies: A First Determination of the Bright End of the z~9 and z~10 UV Luminosity Functions using all five CANDELS Fields

, , , , , , , , , , , , , , , , and . (2015)cite arxiv:1506.01035Comment: 22 pages, 14 figures, 6 tables, submitted to the Astrophysical Journal.

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UV Luminosity Functions at redshifts z~4 to z~10: 11000 Galaxies from HST Legacy Fields, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1403.4295Comment: 47 pages, 29 figures, 8 tables, submitted to the Astrophysical Journal.Cosmic Reionization after Planck: The Derived Growth of the Ionizing Background now matches the Growth of the Galaxy UV Luminosity Density, , , , , , and . (2015)cite arxiv:1503.08228Comment: 16 pages, 10 figures, 3 tables, submitted to the Astrophysical Journal, Figure 6 shows the main result of the paper, Table 1 includes a compilation of the many key constraints on the ionisation state of the universe at z>6.Most Luminous z=9-10 Galaxies: A First Determination of the Bright End of the z~9 and z~10 UV Luminosity Functions using all five CANDELS Fields, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1506.01035Comment: 22 pages, 14 figures, 6 tables, submitted to the Astrophysical Journal.Galaxy And Mass Assembly (GAMA): growing up in a bad neighbourhood - how do low-mass galaxies become passive?, , , , , , , , , and 6 other author(s). (2015)cite arxiv:1511.02245Comment: 20 pages, 12 figures, Accepted to MNRAS.Bright galaxies at Hubble's redshift detection frontier: Preliminary results and design from the redshift z~9-10 BoRG pure-parallel HST survey, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1512.05363Comment: Accepted for publication on ApJ. 21 pages, 11 figures, 4 tables.Quantified HI Morphology V: HI Disks in the Virgo Cluster, , , and . (2011)cite arxiv:1104.3305 Comment: 10 pages, 3 figures, accepted by MNRAS, appendixes not included.