Zobrazeno 1 - 10
of 808
pro vyhledávání: '"MIYAZAKI, SATOSHI"'
Autor:
Oguri, Masamune, Miyazaki, Satoshi
Clusters of galaxies can be identified from peaks in weak lensing aperture mass maps constructed from weak lensing shear catalogs. Such purely gravitational cluster selection considerably differs from traditional cluster selections based on baryonic
Externí odkaz:
http://arxiv.org/abs/2409.12361
Autor:
Chiu, I-Non, Chen, Kai-Feng, Oguri, Masamune, Rau, Markus M., Hamana, Takashi, Lin, Yen-Ting, Miyatake, Hironao, Miyazaki, Satoshi, More, Surhud, Sunayama, Tomomi, Sugiyama, Sunao, Takada, Masahiro
We present cosmological constraints using the abundance of weak-lensing shear-selected galaxy clusters in the Hyper Suprime-Cam (HSC) Subaru Strategic Program. The clusters are selected on the mass maps constructed using the three-year (Y3) weak-lens
Externí odkaz:
http://arxiv.org/abs/2406.11970
Autor:
Chen, Kai-Feng, Chiu, I-Non, Oguri, Masamune, Lin, Yen-Ting, Miyatake, Hironao, Miyazaki, Satoshi, More, Surhud, Hamana, Takashi, Rau, Markus M., Sunayama, Tomomi, Sugiyama, Sunao, Takada, Masahiro
We present the first step towards deriving cosmological constraints through the abundances of galaxy clusters selected in a $510\,\mathrm{deg}^2$ weak-lensing aperture mass map, constructed with the Year-Three shear catalog from the Hyper Suprime-Cam
Externí odkaz:
http://arxiv.org/abs/2406.11966
Autor:
Buie, Marc W., Spencer, John R., Porter, Simon B., Benecchi, Susan D., Parker, Alex H., Stern, S. Alan, Belton, Michael, Binzel, Richard P., Borncamp, David, DeMeo, Francesca, Fabbro, S., Fuentes, Cesar, Furusawa, Hisanori, Fuse, Tetsuharu, Gay, Pamela L., Gwyn, Stephen, Holman, Matthew J., Karoji, H., Kavelaars, J. J., Kinoshita, Daisuke, Miyazaki, Satoshi, Mountain, Matt, Noll, Keith S., Osip, David J., Petit, Jean-Marc, Reid, Neill I., Sheppard, Scott S., Showalter, Mark, Steffl, Andrew J., Sterner, Ray E., Tajitsu, Akito, Tholen, David J., Trilling, David E., Weaver, Harold A., Verbiscer, Anne J., Wasserman, Lawrence H., Yamashita, Takuji, Yanagisawa, Toshifumi, Yoshida, Fumi, Zangari, Amanda M.
Following the Pluto fly-by of the New Horizons spacecraft, the mission provided a unique opportunity to explore the Kuiper Belt in-situ. The possibility existed to fly-by a Kuiper Belt object (KBO) as well as to observe additional objects at distance
Externí odkaz:
http://arxiv.org/abs/2403.04927
Autor:
Kleinebreil, Florian, Grandis, Sebastian, Schrabback, Tim, Ghirardini, Vittorio, Chiu, I-Non, Liu, Ang, Kluge, Matthias, Reiprich, Thomas H., Artis, Emmanuel, Bahar, Emre, Balzer, Fabian, Bulbul, Esra, Clerc, Nicolas, Comparat, Johan, Garrel, Christian, Gruen, Daniel, Li, Xiangchong, Miyatake, Hironao, Miyazaki, Satoshi, Ramos-Ceja, Miriam E., Sanders, Jeremy, Seppi, Riccardo, Okabe, Nobuhiro, Zhang, Xiaoyuan
We aim to participate in the calibration of the X-ray photon count rate to halo mass scaling relation of galaxy clusters selected in the first eROSITA All-Sky Survey on the Western Galactic Hemisphere (eRASS1) using KiDS-1000 weak-lensing (WL) data.
Externí odkaz:
http://arxiv.org/abs/2402.08456
Autor:
Homma, Daisuke, Chiba, Masashi, Komiyama, Yutaka, Tanaka, Masayuki, Okamoto, Sakurako, Tanaka, Mikito, Ishigaki, Miho N., Hayashi, Kohei, Arimoto, Nobuo, Lupton, Robert H., Strauss, Michael A., Miyazaki, Satoshi, Wang, Shiang-Yu, Murayama, Hitoshi
We present the final results of our search for new Milky Way (MW) satellites using the data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) survey over $\sim 1,140$ deg$^2$. In addition to three candidates that we already reported, we
Externí odkaz:
http://arxiv.org/abs/2311.05439
Autor:
Kawanomoto, Satoshi, Koike, Michitaro, Bradfield, Fraser, Fujii, Toshihiro, Komiyama, Yutaka, Miyazaki, Satoshi, Morokuma, Tomoki, Murayama, Hitoshi, Oguri, Masamune, Terai, Tsuyoshi
Publikováno v:
Scientific Reports 13, 16091 (2023)
Extensive air showers induced from high-energy cosmic rays provide a window into understanding the most energetic phenomena in the universe. We present a new method for observing these showers using the silicon imaging detector Subaru Hyper Suprime-C
Externí odkaz:
http://arxiv.org/abs/2310.07963
Autor:
Matsuoka, Yoshiki, Onoue, Masafusa, Iwasawa, Kazushi, Strauss, Michael A., Kashikawa, Nobunari, Izumi, Takuma, Nagao, Tohru, Imanishi, Masatoshi, Akiyama, Masayuki, Silverman, John D., Asami, Naoko, Bosch, James, Furusawa, Hisanori, Goto, Tomotsugu, Gunn, James E., Harikane, Yuichi, Ikeda, Hiroyuki, Inayoshi, Kohei, Ishimoto, Rikako, Kawaguchi, Toshihiro, Kikuta, Satoshi, Kohno, Kotaro, Komiyama, Yutaka, Lee, Chien-Hsiu, Lupton, Robert H., Minezaki, Takeo, Miyazaki, Satoshi, Murayama, Hitoshi, Nishizawa, Atsushi J., Oguri, Masamune, Ono, Yoshiaki, Oogi, Taira, Ouchi, Masami, Price, Paul A., Sameshima, Hiroaki, Sugiyama, Naoshi, Tait, Philip J., Takada, Masahiro, Takahashi, Ayumi, Takata, Tadafumi, Tanaka, Masayuki, Toba, Yoshiki, Wang, Shiang-Yu, Yamashita, Takuji
We present the quasar luminosity function (LF) at $z = 7$, measured with 35 spectroscopically confirmed quasars at $6.55 < z < 7.15$. The sample of 22 quasars from the Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs) project, combined
Externí odkaz:
http://arxiv.org/abs/2305.11225
Autor:
Sugiyama, Sunao, Miyatake, Hironao, More, Surhud, Li, Xiangchong, Shirasaki, Masato, Takada, Masahiro, Kobayashi, Yosuke, Takahashi, Ryuichi, Nishimichi, Takahiro, Nishizawa, Atsushi J., Rau, Markus M., Zhang, Tianqing, Dalal, Roohi, Mandelbaum, Rachel, Strauss, Michael A., Hamana, Takashi, Oguri, Masamune, Osato, Ken, Kannawadi, Arun, Armstrong, Robert, Komiyama, Yutaka, Lupton, Robert H., Lust, Nate B., Miyazaki, Satoshi, Murayama, Hitoshi, Okura, Yuki, Price, Paul A., Tait, Philip J., Tanaka, Masayuki, Wang, Shiang-Yu
Publikováno v:
Phys. Rev. D 108, 123521 (2023)
We present cosmological parameter constraints from a blind joint analysis of three two-point correlation functions measured from the Year 3 Hyper Suprime-Cam (HSC-Y3) imaging data, covering 416 deg$^2$, and the SDSS DR11 spectroscopic galaxies spanni
Externí odkaz:
http://arxiv.org/abs/2304.00705
Autor:
Miyatake, Hironao, Sugiyama, Sunao, Takada, Masahiro, Nishimichi, Takahiro, Li, Xiangchong, Shirasaki, Masato, More, Surhud, Kobayashi, Yosuke, Nishizawa, Atsushi J., Rau, Markus M., Zhang, Tianqing, Takahashi, Ryuichi, Dalal, Roohi, Mandelbaum, Rachel, Strauss, Michael A., Hamana, Takashi, Oguri, Masamune, Osato, Ken, Luo, Wentao, Kannawadi, Arun, Hsieh, Bau-Ching, Armstrong, Robert, Komiyama, Yutaka, Lupton, Robert H., Lust, Nate B., MacArthur, Lauren A., Miyazaki, Satoshi, Murayama, Hitoshi, Okura, Yuki, Price, Paul A., Sunayama, Tomomi, Tait, Philip J., Tanaka, Masayuki, Wang, Shiang-Yu
We present cosmology results from a blinded joint analysis of cosmic shear, $\xi_{\pm}(\vartheta)$, galaxy-galaxy weak lensing, $\Delta\!\Sigma(R)$, and projected galaxy clustering, $w_{\rm p}(R)$, measured from the Hyper Suprime-Cam three-year (HSC-
Externí odkaz:
http://arxiv.org/abs/2304.00704