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Identification of partially resolved binaries in Pan-STARRS1 data

, , , , , , , , , , , and . (2017)cite arxiv:1702.05491Comment: 31 pages, 15 figures, 3 tables, accepted publication in MNRAS.

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Identification of partially resolved binaries in Pan-STARRS1 data, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1702.05491Comment: 31 pages, 15 figures, 3 tables, accepted publication in MNRAS.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 2QDES Pilot : The luminosity and redshift dependence of quasar clustering, , , , , , , , , and 3 other author(s). (2016)cite arxiv:1603.04849Comment: 20 pages, 15 figures, accepted by MNRAS.First lensed quasar system(s) from the VST-ATLAS survey: one quad and three nearly identical pairs, , , , , and . (2016)cite arxiv:1607.07476Comment: Submitted to the Astronomical Journal.The identification of z-dropouts in Pan-STARRS1: three quasars at 6.5<z<6.7, , , , , , , , , and 23 other author(s). (2015)cite arxiv:1502.01927Comment: 7 pages, 3 figures. Accepted for publication in ApJ Letters.The SAMI Galaxy Survey: The cluster redshift survey, target selection and cluster properties, , , , , , , , , and 33 other author(s). (2017)cite arxiv:1703.00997Comment: 28 pages, 15 figures, 3 tables, accepted for publication in MNRAS.Two bright z > 6 quasars from VST ATLAS and a new method of optical plus mid-infra-red colour selection, , , , , , , , and . (2015)cite arxiv:1502.07748Comment: 5 pages, 2 figures, submitted to MNRAS letters.Physical properties of 15 quasars at $z6.5$, , , , , , , , , and 14 other author(s). (2017)cite arxiv:1710.01251Comment: 29 pages, 18 figures; accepted by ApJ.The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1310.0457Comment: ApJ Letters, in press.Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey, , , , , , , , , and 39 other author(s). (2013)cite arxiv:1310.3828Comment: 27 pages,15 figures, submitted to ApJ.