Zobrazeno 41 - 50
of 192
pro vyhledávání: '"Kusakabe, Haruka"'
Autor:
Yamaguchi, Yuki, Kohno, Kotaro, Hatsukade, Bunyo, Wang, Tao, Yoshimura, Yuki, Ao, Yiping, Caputi, Karina I., Dunlop, James S., Egami, Eiichi, Espada, Daniel, Fujimoto, Seiji, Hayatsu, Natsuki H., Ivison, Rob J., Kodama, Tadayuki, Kusakabe, Haruka, Nagao, Tohru, Ouchi, Masami, Rujopakarn, Wiphu, Tadaki, Ken-ichi, Tamura, Yoichi, Ueda, Yoshihiro, Umehata, Hideki, Wang, Wei-Hao, Yun, Min S.
We report detections of two 1.2 mm continuum sources ($S_\mathrm{1.2mm}$ ~ 0.6 mJy) without any counterparts in the deep $H$- and/or $K$-band image (i.e., $K$-band magnitude $\gtrsim$ 26 mag). These near-infrared-dark faint millimeter sources are unc
Externí odkaz:
http://arxiv.org/abs/1903.02744
Akademický článek
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Akademický článek
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Autor:
Itoh, Ryohei, Ouchi, Masami, Zhang, Haibin, Inoue, Akio K., Mawatari, Ken, Shibuya, Takatoshi, Harikane, Yuichi, Ono, Yoshiaki, Kusakabe, Haruka, Shimasaku, Kazuhiro, Fujimoto, Seiji, Iwata, Ikuru, Kajisawa, Masaru, Kashikawa, Nobunari, Kawanomoto, Satoshi, Komiyama, Yutaka, Lee, Chien-Hsiu, Nagao, Tohru, Taniguchi, Yoshiaki
We present the Ly$\alpha$ luminosity function (LF) derived from 34 Ly$\alpha$ emitters (LAEs) at $z=7.0$ on the sky of $3.1$ deg$^2$, the largest sample compared to those in the literature obtained at a redshift $z\gtrsim7$. The LAE sample is made by
Externí odkaz:
http://arxiv.org/abs/1805.05944
Autor:
Kusakabe, Haruka, Shimasaku, Kazuhiro, Momose, Rieko, Ouchi, Masami, Nakajima, Kimihiko, Hashimoto, Takuya, Harikane, Yuichi, Silverman, John D., Capak, Peter L.
The physical origin of diffuse Ly$\alpha$ halos (LAHs) around star-forming galaxies is still a matter of debate. We present the dependence of LAH luminosity ($L({\rm Ly}\alpha)_H$) on the stellar mass ($M_\star$), $SFR$, color excess ($E(B-V)_\star$)
Externí odkaz:
http://arxiv.org/abs/1803.10265
Autor:
Inoue, Akio K., Hasegawa, Kenji, Ishiyama, Tomoaki, Yajima, Hidenobu, Shimizu, Ikkoh, Umemura, Masayuki, Konno, Akira, Harikane, Yuichi, Shibuya, Takatoshi, Ouchi, Masami, Shimasaku, Kazuhiro, Ono, Yoshiaki, Kusakabe, Haruka, Higuchi, Ryo, Lee, Chien-Hsiu
The survey of Lyman $\alpha$ emitters (LAEs) with Subaru Hyper Suprime-Cam, called SILVERRUSH (Ouchi et al.), is producing massive data of LAEs at $z\gtrsim6$. Here we present LAE simulations to compare the SILVERRUSH data. In 162$^3$ comoving Mpc$^3
Externí odkaz:
http://arxiv.org/abs/1801.00067
Autor:
Kusakabe, Haruka, Shimasaku, Kazuhiro, Ouchi, Masami, Nakajima, Kimihiko, Goto, Ryosuke, Hashimoto, Takuya, Konno, Akira, Harikane, Yuichi, Silverman, John D., Capak, Peter L.
We present average stellar population properties and dark matter halo masses of $z \sim 2$ \lya emitters (LAEs) from SED fitting and clustering analysis, respectively, using $\simeq$ $1250$ objects ($NB387\le25.5$) in four separate fields of $\simeq
Externí odkaz:
http://arxiv.org/abs/1707.09373
Autor:
Konno, Akira, Ouchi, Masami, Shibuya, Takatoshi, Ono, Yoshiaki, Shimasaku, Kazuhiro, Taniguchi, Yoshiaki, Nagao, Tohru, Kobayashi, Masakazu A. R., Kajisawa, Masaru, Kashikawa, Nobunari, Inoue, Akio K., Oguri, Masamune, Furusawa, Hisanori, Goto, Tomotsugu, Harikane, Yuichi, Higuchi, Ryo, Komiyama, Yutaka, Kusakabe, Haruka, Miyazaki, Satoshi, Nakajima, Kimihiko, Wang, Shiang-Yu
We present the Ly$\alpha$ luminosity functions (LFs) at $z=$5.7 and 6.6 derived from a new large sample of 1,266 Ly$\alpha$ emitters (LAEs) identified in total areas of 14 and 21 deg$^2$, respectively, based on the early narrowband data of the Subaru
Externí odkaz:
http://arxiv.org/abs/1705.01222
Autor:
Shibuya, Takatoshi, Ouchi, Masami, Harikane, Yuichi, Rauch, Michael, Ono, Yoshiaki, Mukae, Shiro, Higuchi, Ryo, Kojima, Takashi, Yuma, Suraphong, Lee, Chien-Hsiu, Furusawa, Hisanori, Konno, Akira, Martin, Crystal L., Shimasaku, Kazuhiro, Taniguchi, Yoshiaki, Kobayashi, Masakazu A. R., Kajisawa, Masaru, Nagao, Tohru, Goto, Tomotsugu, Kashikawa, Nobunari, Komiyama, Yutaka, Kusakabe, Haruka, Momose, Rieko, Nakajima, Kimihiko, Tanaka, Masayuki, Wang, Shiang-Yu
We present Lya and UV-nebular emission line properties of bright Lya emitters (LAEs) at z=6-7 with a luminosity of log L_Lya/[erg s-1] = 43-44 identified in the 21-deg2 area of the SILVERRUSH early sample developed with the Subaru Hyper Suprime-Cam (
Externí odkaz:
http://arxiv.org/abs/1705.00733
Autor:
Shibuya, Takatoshi, Ouchi, Masami, Konno, Akira, Higuchi, Ryo, Harikane, Yuichi, Ono, Yoshiaki, Shimasaku, Kazuhiro, Taniguchi, Yoshiaki, Kobayashi, Masakazu A. R., Kajisawa, Masaru, Nagao, Tohru, Furusawa, Hisanori, Goto, Tomotsugu, Kashikawa, Nobunari, Komiyama, Yutaka, Kusakabe, Haruka, Lee, Chien-Hsiu, Momose, Rieko, Nakajima, Kimihiko, Tanaka, Masayuki, Wang, Shiang-Yu, Yuma, Suraphong
We present an unprecedentedly large catalog consisting of 2,230 > L* Lya emitters (LAEs) at z=5.7 and 6.6 on the 13.8 and 21.2 deg2 sky, respectively, that are identified by the SILVERRUSH program with the first narrowband imaging data of the Hyper S
Externí odkaz:
http://arxiv.org/abs/1704.08140