Search Results - "Niinuma, Kotaro"

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    A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies by Hatsukade, Bunyo, Tominaga, Nozomu, Morokuma, Tomoki, Morokuma-Matsui, Kana, Matsuda, Yuichi, Tamura, Yoichi, Niinuma, Kotaro, Motogi, Kazuhiro

    Published in The Astrophysical journal (01-11-2021)
    “…Abstract We present the results of 3 GHz radio continuum observations of 23 superluminous supernovae (SLSNe) and their host galaxies by using the Karl G…”
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    Journal Article
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    Spatially resolved molecular gas properties of host galaxy of Type I superluminous supernova SN 2017egm by Hatsukade, Bunyo, Morokuma-Matsui, Kana, Hayashi, Masao, Tominaga, Nozomu, Tamura, Yoichi, Niinuma, Kotaro, Motogi, Kazuhiro, Morokuma, Tomoki, Matsuda, Yuichi

    “…Abstract We present the results of CO(1–0) observations of the host galaxy of a Type I superluminous supernova (SLSN-I), SN 2017egm, one of the closest SLSNe-I…”
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    Journal Article
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    The Yamaguchi Interferometer by Fujisawa, Kenta, Aoki, Takahiro, Kanazawa, Sho, Akimoto, Masanori, Ogura, Tatsuya, Mori, Kurena, Niinuma, Kotaro, Motogi, Kazuhito, Sawada-Satoh, Satoko, Takefuji, Kazuhiro, Ogawa, Hideo, Kimura, Kimihiro, Yonekura, Yoshinori, Honma, Mareki

    “…Abstract We report on the Yamaguchi Interferometer (YI), a one-baseline radio interferometer consisting of two radio telescopes with diameters of 32 m and 34…”
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    Mid-infrared Excess from the West Hot Spot of the Radio Galaxy Pictor A Unveiled by WISE by Isobe, Naoki, Koyama, Shoko, Kino, Motoki, Wada, Takehiko, Nakagawa, Takao, Matsuhara, Hideo, Niinuma, Kotaro, Tashiro, Makoto

    Published in The Astrophysical journal (01-12-2017)
    “…Mid-infrared properties are reported of the west hot spot of the radio galaxy Pictor A with the Wide-field Infrared Survey Explorer (WISE). The mid-infrared…”
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    Journal Article
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    Observations of V404 Cygni during the 2015 outburst by the Nasu telescope array at 1.4 GHz by Asuma, Kuniyuki, Niinuma, Kotaro, Takefuji, Kazuhiro, Aoki, Takahiro, Kida, Sumiko, Nakajima, Hirochika, Tsubono, Kimio, Daishido, Tsuneaki

    “…Abstract Waseda University Nasu telescope array is a spatial fast Fourier transform interferometer consisting of eight linearly aligned antennas with 20 m…”
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    Accelerating a water maser face-on jet from a high mass young stellar object by Motogi, Kazuhito, Sorai, Kazuo, Honma, Mareki, Hirota, Tomoya, Hachisuka, Kazuya, Niinuma, Kotaro, Sugiyama, Koichiro, Yonekura, Yoshinori, Fujisawa, Kenta

    “…Abstract We report on long-term single-dish and VLBI monitoring for intermittent flare activities of a dominant blue-shifted H2O maser associated with a…”
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    A Face-on Accretion System in High-mass Star Formation: Possible Dusty Infall Streams within 100 AU by Motogi, Kazuhito, Hirota, Tomoya, Sorai, Kazuo, Yonekura, Yoshinori, Sugiyama, Koichiro, Honma, Mareki, Niinuma, Kotaro, Hachisuka, Kazuya, Fujisawa, Kenta, Walsh, Andrew J.

    Published in The Astrophysical journal (01-11-2017)
    “…We report on interferometric observations of a face-on accretion system around the high-mass young stellar object, G353.273+0.641. The innermost accretion…”
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    HINOTORI and Its Perspectives in the Black-Hole Jet Study by Tsutsumi, Toshihisa, Niinuma, Kotaro, Imai, Hiroshi, Amari, Ryoko, Shimizu, Yusuke, Ogawa, Hideo, Nishimura, Atsushi, Miyazawa, Chieko, Oyama, Tomoaki, Kaneko, Hiroyuki, Nakashima, Keisuke, Sawada-Satoh, Satoko, Aoki, Takahiro

    Published in Galaxies (01-02-2023)
    “…Simultaneous multi-band very long baseline interferometry (VLBI) observations at millimeter wavelengths have huge potential for various science cases. However,…”
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    Observations of the bursting activity of the 6.7 GHz methanol maser in G33.641−0.228 by Fujisawa, Kenta, Aoki, Nozomu, Nagadomi, Yoshito, Kimura, Saki, Shimomura, Tadashi, Takase, Genta, Sugiyama, Koichiro, Motogi, Kazuhito, Niinuma, Kotaro, Hirota, Tomoya, Yonekura, Yoshinori

    “…Abstract We have observed bursting variability of the 6.7 GHz methanol maser of G33.641−0.228. Five bursts were detected in the observation period of 294 days…”
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    Journal Article