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A new faint Milky Way satellite discovered in the Pan-STARRS1 3{pi} surveyThe extremely red, young l dwarf PSO J318.5338-22.8603: a free-floating planetary-mass analog to directly imaged young gas-giant planetsSlowly fading super-luminous supernovae that are not pair-instability explosionsA new distant Milky Way globular cluster in the Pan-STARRS1 3{pi} surveySuper-luminous type IC supernovae: catching a magnetar by the tailDetection of a supervoid aligned with the cold spot of the cosmic microwave backgroundThe superluminous supernova PS1-11ap: bridging the gap between low and high redshiftThe Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon SampleOptical confirmation and redshift estimation of the Planck cluster candidates overlapping the Pan-STARRS SurveyCosmological constraints from measurements of type Ia supernovae discovered during the first 1.5 yr of the Pan-STARRS1 surveySystematic uncertainties associated with the cosmological analysis of the first Pan-STARRS1 type Ia supernova sampleA map of dust reddening to 4.5 kpc from Pan-STARRS1Discovery of eight z ~ 6 quasars from Pan-STARRS1A search for fast optical transients in the Pan-STARRS1 medium-deep survey: m-dwarf flares, asteroids, limits on extragalactic rates, and implications for LSSTUltra-bright optical transients are linked with type IC supernovaeHydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep SurveyThe Time-domain Spectroscopic Survey: Target Selection for Repeat SpectroscopyThe time domain spectroscopic survey: variable selection and anticipated resultsFinding, characterizing, and classifying variable sources in multi-epoch sky surveys: QSOs and RR Lyrae in PS1 3{Pi} dataThe Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster EnvironmentsGalaxy and mass assembly (GAMA): projected galaxy clusteringSupervoid Origin of the Cold Spot in the Cosmic Microwave BackgroundThe Pan-STARRS1 medium-deep survey: the role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to z ~ 0.8Pan-STARRS1: Galaxy clustering in the Small Area Survey 2The Pan-STARRS1 Small Area Survey 2Hiding in plain sight – recovering clusters of galaxies with the strongest AGN in their coresA multiwavelength photometric census of AGN and star formation activity in the brightest cluster galaxies of X-ray selected clustersCosmic cookery: making a stereoscopic 3D animated moviePhysical Properties of 15 Quasars at z ≳ 6.5The Pan-STARRS1 distant z > 5.6 quasar survey: more than 100 quasars within the first Gyr of the UniverseConstraining the radio-loud fraction of quasars at z > 5.5The identification of z-dropouts in Pan-STARRS1: three quasars at 6.5< z< 6.7The discovery of eight z ~ 6 quasars from Pan-STARRS1Erratum: Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosionsThe optical-infrared extinction curve and its variation in the Milky WayThe SAMI Galaxy Survey: instrument specification and target selectionA search for optical afterglow from GRB970828A Search for Optical Afterglow from GRB 970828Sagittarius II, Draco II and Laevens 3: three new Milky Way satellites discovered in the Pan-STARRS 1 3{pi} surveyRapidly evolving and luminous transients from Pan-STARRS1
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description
astrofysicus
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hulumtues
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հետազոտող
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name
Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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Nigel Metcalfe
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lccn-no2003061263