Hyper Suprime-Cam

By Satoshi Miyazaki, Yutaka Komiyama, H. Nakaya, Y. Kamata, Y. Doi, T. Hamana, Hiroshi Karoji, Hisanori Furusawa, Satoshi Kawanomoto, T. Morokuma and 47 more. Other Conferences, 2012

139 citations recorded by the source corpus.

Subfields: Biomedical Engineering, Fluid Flow and Transfer Processes

View Paper: https://www.semanticscholar.org/paper/b490519c645755974daca23234e4a6842718f653

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Citations in the corpus

• Great 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$^2$ Sky (2017, unknown): “…this study, we present results from our systematic search for very luminous galaxies at z ∼ 4−7 based on wide and deep optical Hyper Suprime-Cam (HSC; Miyazaki et al. 2012; see also Miyazaki et al. 2017; Komiyama et al. 2017; Furusawa et al. 2017; Kawanomoto et al. 2017) images obtained by…”
• J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817 (2017, methodology): “We used the following facilities to perform follow-up optical observations of GW170817: 8.2 m Subaru/HSC (Miyazaki et al. 2012) and MOIRCS (Suzuki et al. 2008) at Mauna Kea in the United States; 2.0 m Nayuta/NIC (near-infrared imager) at the Nishi-Harima Astronomical Observatory in Japan; 1.8 m MOA-”
• SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky (2017, methodology): “2.1 Hyper Suprime-Cam Imaging Observations and Data Reduction In our sample construction for z = 5.7 and 6.6 LAEs, we use narrowband (NB816, NB921) imaging data as well as broadband (g, r, i, z, y) imaging data, which are taken with Subaru/HSC (Miyazaki et al. 2012; see also Miyazaki et al. 2017; Fu”
• SUBARU HIGH-z EXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7 < z < 6.9 (2016, unknown): “It uses the HSC (Miyazaki et al. 2012, S. Miyazaki et al. 2016, in preparation), a wide-field camera newly installed on the Subaru 8.2 m telescope on the summit of Maunakea.”
• The COSMOS2015 galaxy stellar mass function . Thirteen billion years of stellar mass assembly in ten snapshots (2017, background): “One cornerstone of the COSMOS2015 photometry comes from the new Y , J, H, and Ks images from the second data release (DR2) of the UltraVISTA survey (McCracken et al. 2012), along with the z++ band from Suprime-Cam at Subaru (Miyazaki et al. 2012).”
• Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties of ∼2000 Lyα emitters at z = 6–7 over the 0.3–0.5 Gpc2 survey area (2017, methodology): “…observations; the Very Large Telescope/MultiUnit Spectroscopic Explorer (MUSE: Bacon et al. 2010), the Hobby–Eberly Telescope Dark Energy Experiment/ Visible Integral-Field Replicable Unit Spectrograph (HETDEX/VIRUS: Hill et al. 2012), and the Subaru/Hyper Suprime-Cam (HSC: Miyazaki et al. 2012).”
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data (2018, methodology): “The Hyper Suprime-Cam Subaru Strategic Program (HSCSSP, hereafter the HSC survey) is a wide-field imaging survey using a 1.77 deg2 field-of-view imaging camera on the 8.2-meter Subaru telescope (Miyazaki et al. 2012, 2015, 2018; Komiyama et al. 2018; Furusawa et al. 2018; Kawanomoto et al. 2018).”