Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Yamamoto, Naoaki"'
Autor:
Laishram, Ronaldo, Kodama, Tadayuki, Morishita, Takahiro, Faisst, Andreas, Koyama, Yusei, Yamamoto, Naoaki
We explore the morphological features and star formation activities of [OII] emitters in the COSMOS UltraDeep field at $z \sim 1.5$ using JWST NIRCam data from the COSMOS-Web survey and Subaru Hyper Suprime-Cam. We also report the discovery of large
Externí odkaz:
http://arxiv.org/abs/2403.06369
Autor:
Mao, Zhiying, Kodama, Tadayuki, Pérez-Martínez, Jose Manuel, Suzuki, Tomoko L., Yamamoto, Naoaki, Adachi, Kouta
Publikováno v:
A&A 666, A141 (2022)
Galaxy quenching is a critical step in galaxy evolution. In this work, we present a statistical study of galaxy quenching in 17 cluster candidates at 0.5
Externí odkaz:
http://arxiv.org/abs/2208.00722
Autor:
Misato, Rana, Toba, Yoshiki, Ota, Naomi, Yamamoto, Naoaki, Kodama, Tadayuki, Okabe, Nobuhiro, Oguri, Masamune, Mitsuishi, Ikuyuki
We present herein a systematic X-ray analysis of blue galaxy-clusters at $z=0.84$ discovered by the Subaru telescope. The sample consisted of 43 clusters identified by combining red-sequence and blue-cloud surveys, covering a wide range of emitter fr
Externí odkaz:
http://arxiv.org/abs/2201.00597
Autor:
Aihara, Hiroaki, AlSayyad, Yusra, Ando, Makoto, Armstrong, Robert, Bosch, James, Egami, Eiichi, Furusawa, Hisanori, Furusawa, Junko, Harasawa, Sumiko, Harikane, Yuichi, Hsieh, Bau-Ching, Ikeda, Hiroyuki, Ito, Kei, Iwata, Ikuru, Kodama, Tadayuki, Koike, Michitaro, Kokubo, Mitsuru, Komiyama, Yutaka, Li, Xiangchong, Liang, Yongming, Lin, Yen-Ting, Lupton, Robert H., Lust, Nate B, MacArthur, Lauren A., Mawatari, Ken, Mineo, Sogo, Miyatake, Hironao, Miyazaki, Satoshi, More, Surhud, Morishima, Takahiro, Murayama, Hitoshi, Nakajima, Kimihiko, Nakata, Fumiaki, Nishizawa, Atsushi J., Oguri, Masamune, Okabe, Nobuhiro, Okura, Yuki, Ono, Yoshiaki, Osato, Ken, Ouchi, Masami, Pan, Yen-Chen, Malagón, Andrés A. Plazas, Price, Paul A., Reed, Sophie L, Rykoff, Eli S., Shibuya, Takatoshi, Simunovic, Mirko, Strauss, Michael A., Sugimori, Kanako, Suto, Yasushi, Suzuki, Nao, Takada, Masahiro, Takagi, Yuhei, Takata, Tadafumi, Takita, Satoshi, Tanaka, Masayuki, Tang, Shenli, Taranu, Dan S., Terai, Tsuyoshi, Toba, Yoshiki, Turner, Edwin L., Uchiyama, Hisakazu, Vijarnwannaluk, Bovornpratch, Waters, Christopher Z, Yamada, Yoshihiko, Yamamoto, Naoaki, Yamashita, Takuji
The paper presents the third data release of Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP), a wide-field multi-band imaging survey with the Subaru 8.2m telescope. HSC-SSP has three survey layers (Wide, Deep, and UltraDeep) with different area
Externí odkaz:
http://arxiv.org/abs/2108.13045
Autor:
Shimakawa, Rhythm, Higuchi, Yuichi, Shirasaki, Masato, Tanaka, Masayuki, Lin, Yen-Ting, Hayashi, Masao, Momose, Rieko, Lee, Chien-Hsiu, Kusakabe, Haruka, Kodama, Tadayuki, Yamamoto, Naoaki
Subaru Strategic Program with the Hyper-Suprime Cam (HSC-SSP) has proven to be successful with its extremely-wide area coverage in past years. Taking advantages of this feature, we report initial results from exploration and research of expansive ove
Externí odkaz:
http://arxiv.org/abs/2103.04291
Autor:
Asano, Tetsuro, Kodama, Tadayuki, Motohara, Kentaro, Lubin, Lori, Lemaux, Brian C., Gal, Roy, Tomczak, Adam, Kocevski, Dale, Hayashi, Masao, Koyama, Yusei, Tanaka, Ichi, Suzuki, Tomoko L., Yamamoto, Naoaki, Kimura, Daiki, Konishi, Masahiro, Takahashi, Hidenori, Terao, Yasunori, Kushibiki, Kosuke, Kono, Yukihiro, Yoshii, Yuzuru, team, the SWIMS
Galaxies change their properties as they assemble into clusters. In order to understand the physics behind that, we need to go back in time and observe directly what is occurring in galaxies as they fall into a cluster. We have conducted a narrow-ban
Externí odkaz:
http://arxiv.org/abs/2006.10053
Autor:
Hayashi, Masao, Koyama, Yusei, Kodama, Tadayuki, Komiyama, Yutaka, Lin, Yen-Ting, Miyazaki, Satoshi, Shimakawa, Rhythm, Suzuki, Tomoko L., Tanaka, Ichi, Yamamoto, Moegi, Yamamoto, Naoaki
We present the large-scale structure over more than 50 comoving Mpc scale at z $\sim$ 0.9 where the CL1604 supercluster, which is one of the largest structures ever known at high redshifts, is embedded. The wide-field deep imaging survey by the Subar
Externí odkaz:
http://arxiv.org/abs/1905.13437
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