Showing 21–40 of 76 results
/ Date/ Name
Nov 9, 2011Clustering properties of BzK-selected galaxies in GOODS-N: environmental quenching and triggering of star formation at z ~ 2Aug 2, 2016Metrology Camera System of Prime Focus Spectrograph for Subaru TelescopeApr 21, 2017Machine Learning Based Real Bogus System for HSC-SSP Moving Object Detecting PipelineNov 9, 2015The Outer Solar System Origins Survey: I. Design and First-Quarter DiscoveriesOct 18, 2021OSSOS. XXIII. 2013 VZ70 and the Temporary Coorbitals of the Giant PlanetDec 31, 2018Near-Infrared Survey and Photometric Redshifts in the Extended GOODS-North fieldSep 27, 2022A low-inclination neutral Trans-Neptunian Object in a extreme orbitApr 3, 2023Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation FunctionsJul 14, 2011Star-forming Region Sh 2-233IR I. Deep NIR Observations toward the Embedded Stellar ClustersAug 3, 2016Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectivesApr 19, 2017Multi-band Photometry of Trans-Neptunian Objects in the Subaru Hyper Suprime-Cam SurveyApr 20, 2017Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ SkyFeb 27, 2017First Data Release of the Hyper Suprime-Cam Subaru Strategic ProgramOct 9, 2012Prime Focus Spectrograph - Subaru's future -Aug 5, 2016Discovery of A New Retrograde Trans-Neptunian Object: Hint of A Common Orbital Plane for Low Semi-Major Axis, High Inclination TNOs and CentaursAug 10, 2017Col-OSSOS: z Band Photometry Reveals Three Distinct TNO Surface TypesMay 29, 2019Second Data Release of the Hyper Suprime-Cam Subaru Strategic ProgramSep 24, 2018Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year dataOct 17, 2018Colors of Centaurs observed by the Subaru/Hyper Suprime-Cam and implications for their originNov 5, 2018Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6