Zobrazeno 1 - 10
of 1 017
pro vyhledávání: '"MATSUO, HIROSHI"'
Autor:
Ishii, Nozomi, Hashimoto, Takuya, Ferkinhoff, Carl, Rybak, Matus, Inoue, Akio K., Michiyama, Tomonari, Donevski, Darko, Fujimoto, Seiji, Salak, Dragan, Kuno, Nario, Matsuo, Hiroshi, Mawatari, Ken, Tamura, Yoichi, Izumi, Takuma, Nagao, Tohru, Nakazato, Yurina, Osone, Wataru, Sugahara, Yuma, Usui, Mitsutaka, Wakasugi, Koki, Yajima, Hidenobu, Bakx, Tom J. L. C., Fudamoto, Yoshinobu, Meyer, Romain A., Walter, Fabian, Yoshida, Naoki
We report the highest-redshift detection of [O I] 63 $\mu$m from a luminous quasar, J2054-0005, at $z=6.04$ based on the Atacama Large Millimeter/sub-millimeter Array Band 9 observations. The [O I] 63 $\mu$m line luminosity is $(4.5\pm1.5) \times 10^
Externí odkaz:
http://arxiv.org/abs/2408.09944
Autor:
Bakx, Tom J. L. C., Algera, Hiddo S. B., Venemans, Bram, Sommovigo, Laura, Fujimoto, Seiji, Carniani, Stefano, Hagimoto, Masato, Hashimoto, Takuya, Inoue, Akio K., Salak, Dragan, Serjeant, Stephen, Vallini, Livia, Eales, Stephen, Ferrara, Andrea, Fudamoto, Yoshinobu, Imamura, Chihiro, Inoue, Shigeki, Knudsen, Kirsten K., Matsuo, Hiroshi, Sugahara, Yuma, Tamura, Yoichi, Taniguchi, Akio, Yamanaka, Satoshi
We present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the [O$_{\rm III}$] 88 $\mu$m emission of a sample of thirteen galaxies at $z$ = 6 to 7.6 selected as [C$_{\rm II}$]-emitting companion sources of quasars. To disentangle
Externí odkaz:
http://arxiv.org/abs/2406.19439
Autor:
Harikane, Yuichi, Inoue, Akio K., Ellis, Richard S., Ouchi, Masami, Nakazato, Yurina, Yoshida, Naoki, Ono, Yoshiaki, Sun, Fengwu, Sato, Riku A., Ferrami, Giovanni, Fujimoto, Seiji, Kashikawa, Nobunari, McLeod, Derek J., Perez-Gonzalez, Pablo G., Sawicki, Marcin, Sugahara, Yuma, Xu, Yi, Yamanaka, Satoshi, Carnall, Adam C., Cullen, Fergus, Dunlop, James S., Egami, Eiichi, Grogin, Norman, Isobe, Yuki, Koekemoer, Anton M., Laporte, Nicolas, Lee, Chien-Hsiu, Magee, Dan, Matsuo, Hiroshi, Matsuoka, Yoshiki, Mawatari, Ken, Nakajima, Kimihiko, Nakane, Minami, Tamura, Yoichi, Umeda, Hiroya, Yanagisawa, Hiroto
We present the number densities and physical properties of the bright galaxies spectroscopically confirmed at $z\sim7-14$. Our sample is composed of 60 galaxies at $z_\mathrm{spec}\sim7-14$, including recently-confirmed galaxies at $z_\mathrm{spec}=1
Externí odkaz:
http://arxiv.org/abs/2406.18352
Autor:
Sugahara, Yuma, Álvarez-Márquez, Javier, Hashimoto, Takuya, Colina, Luis, Inoue, Akio K., Costantin, Luca, Fudamoto, Yoshinobu, Mawatari, Ken, Ren, Yi W., Arribas, Santiago, Bakx, Tom J. L. C., Blanco-Prieto, Carmen, Ceverino, Daniel, Gómez, Alejandro Crespo, Hagimoto, Masato, Hashigaya, Takeshi, Marques-Chaves, Rui, Matsuo, Hiroshi, Nakazato, Yurina, Pereira-Santaella, Miguel, Tamura, Yoichi, Usui, Mitsutaka, Yoshida, Naoki
We present JWST NIRCam imaging of B14-65666 ("Big Three Dragons"), a bright Lyman-break galaxy system ($M_\text{UV}=-22.5$ mag) at $z=7.15$. The high angular resolution of NIRCam reveals the complex morphology of two galaxy components: galaxy E has a
Externí odkaz:
http://arxiv.org/abs/2403.17133
Autor:
Hashimoto, Takuya, Álvarez-Márquez, Javier, Fudamoto, Yoshinobu, Colina, Luis, Inoue, Akio K., Nakazato, Yurina, Ceverino, Daniel, Yoshida, Naoki, Costantin, Luca, Sugahara, Yuma, Gómez, Alejandro Crespo, Blanco-Prieto, Carmen, Mawatari, Ken, Arribas, Santiago, Marques-Chaves, Rui, Pereira-Santaella, Miguel, Bakx, Tom J. L. C., Hagimoto, Masato, Hashigaya, Takeshi, Matsuo, Hiroshi, Tamura, Yoichi, Usui, Mitsutaka, Ren, Yi W.
The protoclusters in the epoch of reionization, traced by galaxies overdensity regions, are ideal laboratories for studying the process of stellar assembly and cosmic reionization. We present the spectroscopic confirmation of the core of the most dis
Externí odkaz:
http://arxiv.org/abs/2305.04741
Autor:
Tamura, Yoichi, Bakx, Tom J. L. C., Inoue, Akio K., Hashimoto, Takuya, Tokuoka, Tsuyoshi, Imamura, Chihiro, Hatsukade, Bunyo, Lee, Minju M., Moriwaki, Kana, Okamoto, Takashi, Ota, Kazuaki, Umehata, Hideki, Yoshida, Naoki, Zackrisson, Erik, Hagimoto, Masato, Matsuo, Hiroshi, Shimizu, Ikkoh, Sugahara, Yuma, Takeuchi, Tsutomu T.
We present the results of 300 pc resolution ALMA imaging of the [OIII] 88 $\mu$m line and dust continuum emission from a $z = 8.312$ Lyman break galaxy MACS0416_Y1. The velocity-integrated [OIII] emission has three peaks which are likely associated w
Externí odkaz:
http://arxiv.org/abs/2303.11539
Autor:
Ura, Ryota, Hashimoto, Takuya, Inoue, Akio K., Fadda, Dario, Hayes, Matthew, Puschnig, Johannes, Zackrisson, Erik, Tamura, Yoichi, Matsuo, Hiroshi, Mawatari, Ken, Fudamoto, Yoshinobu, Hagimoto, Masato, Kuno, Nario, Sugahara, Yuma, Yamanaka, Satoshi, Bakx, Tom J. L. C., Nakazato, Yurina, Usui, Mitsutaka, Yajima, Hidenobu, Yoshida, Naoki
We present integral field, far-infrared (FIR) spectroscopy of Mrk 54, a local Lyman Continuum Emitter (LCE), obtained with FIFI-LS on the Stratospheric Observatory for Infrared Astronomy. This is only the second time, after Haro 11, that [C II] 158 $
Externí odkaz:
http://arxiv.org/abs/2303.11036
Autor:
Ren, Yi W., Fudamoto, Yoshinobu, Inoue, Akio K., Sugahara, Yuma, Tokuoka, Tsuyoshi, Tamura, Yoichi, Matsuo, Hiroshi, Kohno, Kotaro, Umehata, Hideki, Hashimoto, Takuya, Bouwens, Rychard J., Smit, Renske, Kashikawa, Nobunari, Okamoto, Takashi, Shibuya, Takatoshi, Shimizu, Ikkoh
We present updated measurements of the [O III] 88 $\mu$m, [C II] 158 $\mu$m, and dust continuum emission from a star-forming galaxy at $z=7.212$, SXDF-NB1006-2, by utilizing Atacama Large Millimeter/submillimeter Array (ALMA) archival data sets analy
Externí odkaz:
http://arxiv.org/abs/2302.02365
ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
Autor:
Akins, Hollis, Fujimoto, Seiji, Finlator, Kristian, Watson, Darach, Knudsen, Kirsten, Richard, Johan, Bakx, Tom, Hashimoto, Takuya, Inoue, Akio, Matsuo, Hiroshi, Michalowski, Michal, Tamura, Yoichi
We present spatially-resolved morphological properties of [CII] 158 $\mu$m, [OIII] 88 $\mu$m, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at $z=7.13$, by utilizing deep Atacama Large Millim
Externí odkaz:
http://arxiv.org/abs/2206.06939