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101. COMPLETING THE CENSUS OF Lyα EMITTERS AT THE REIONIZATION EPOCH**The data presented herein were partly obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.††Based in part on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.

Author

Kashikawa, Nobunari, Shimasaku, Kazuhiro, Matsuda, Yuichi, Egami, Eiichi, Jiang, Linhua, Nagao, Tohru, Ouchi, Masami, Malkan, Matthew A, Hattori, Takashi, Ota, Kazuaki, Taniguchi, Yoshiaki, Okamura, Sadanori, Ly, Chun, Iye, Masanori, Furusawa, Hisanori, Shioya, Yasuhiro, Shibuya, Takatoshi, Ishizaki, Yoshifumi, and Toshikawa, Jun

Subjects
cosmology: observations, early universe, galaxies: formation, galaxies: high-redshift, astro-ph.CO, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We carried out extended spectroscopic confirmations of Lyα emitters (LAEs) at z = 6.5 and 5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs is 45 and 54 at z = 6.5 and 5.7, respectively, and at least 81% (70%) of our photometric candidates at z = 6.5 (5.7) have been spectroscopically identified as real LAEs. We made careful measurements of the Lyα luminosity, both photometrically and spectroscopically, to accurately determine the Lyα and rest-UV luminosity functions (LFs). The substantially improved evaluation of the Lyα LF at z = 6.5 shows an apparent deficit from z = 5.7 at least at the bright end, and a possible decline even at the faint end, though small uncertainties remain. The rest-UV LFs at z = 6.5 and 5.7 are in good agreement, at least at the bright end, in clear contrast to the differences seen in the Lyα LF. These results imply an increase in the neutral fraction of the intergalactic medium from z = 5.7 to 6.5. The rest-frame equivalent width (EW0) distribution at z = 6.5 seems to be systematically smaller than z = 5.7, and it shows an extended tail toward larger EW0. The bright end of the rest-UV LF can be reproduced from the observed Lyα LF and a reasonable EW0-UV luminosity relation. Integrating this rest-UV LF provides the first measurement of the contribution of LAEs to the photon budget required for reionization. The derived UV LF suggests that the fractional contribution of LAEs to the photon budget among Lyman break galaxies significantly increases toward faint magnitudes. Low-luminosity LAEs could dominate the ionizing photon budget, though this inference depends strongly on the uncertain faint-end slope of the Lyα LF. © 2011. The American Astronomical Society. All rights reserved.

Published
2011

102. The SSA22 H i Tomography Survey (SSA22-HIT). I. Data Set and Compiled Redshift Catalog

Author

Mawatari, Ken, primary, Inoue, Akio K., additional, Yamada, Toru, additional, Hayashino, Tomoki, additional, Prochaska, J. Xavier, additional, Lee, Khee-Gan, additional, Tejos, Nicolas, additional, Kashikawa, Nobunari, additional, Otsuka, Takuya, additional, Yamanaka, Satoshi, additional, Schlegel, David J., additional, Matsuda, Yuichi, additional, Hennawi, Joseph F., additional, Iwata, Ikuru, additional, Umehata, Hideki, additional, Mukae, Shiro, additional, Ouchi, Masami, additional, Sugahara, Yuma, additional, and Tamura, Yoichi, additional

Published
2023
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104. End‐tidal oxygen partial pressure is a strong prognostic predictive factor in patients with cardiac disease.

Author

Ogura, Asami, Izawa, Kazuhiro P., Tawa, Hideto, Wada, Masaaki, Kanai, Masashi, Kubo, Ikko, Makihara, Ayano, Yoshikawa, Ryohei, and Matsuda, Yuichi

Subjects
PARTIAL pressure, CARDIAC patients, EXERCISE tests, PROGNOSIS, HYPERVENTILATION, ANAEROBIC threshold
Abstract

Background: Cardiopulmonary exercise testing (CPET) variables represent central and peripheral factors and combined factors in the pathology of patients with cardiac disease. The difference in end‐tidal oxygen partial pressure from resting to anaerobic threshold (ΔPETO2) may represent predominantly peripheral factors. This study aimed to verify the prognostic significance of ΔPETO2 for major adverse cardiac and cerebrovascular events (MACCE) in cardiac patients, including comparison with the minute ventilation–carbon dioxide production relationship (VE/VCO2 slope), and peak oxygen uptake (VO2). Methods: In total, 185 patients with cardiac disease who underwent CPET were consecutively enroled in this retrospective study. The primary endpoint was 3‐year MACCE. The ability of ΔPETO2, VE/VCO2 slope, and peak VO2 to predict MACCE was examined. Results: Optimal cut‐off values for predicting MACCE were 2.0 mmHg for ΔPETO2 (area under the curve [AUC]: 0.829), 29.8 for VE/VCO2 slope (AUC: 0.734), and 19.0 mL/min/kg for peak VO2 (AUC: 0.755). The AUC of ΔPETO2 was higher than those of VE/VCO2 slope and peak VO2. The MACCE‐free survival rate was significantly lower in the ΔPETO2 ≤ 2.0 group versus the ΔPETO2 > 2.0 group (44.4% vs. 91.2%, p < 0.001). ΔPETO2 ≤ 2.0 was an independent predictor of MACCE after adjustment for age and VE/VCO2 slope (hazard ratio [HR], 7.28; p < 0.001) and after adjustment for age and peak VO2 (HR, 6.52; p < 0.001). Conclusion: ΔPETO2 was a strong predictor of MACCE independent of and superior to VE/VCO2 slope and peak VO2 in patients with cardiac disease. [ABSTRACT FROM AUTHOR]

Published
2023
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105. Lyα Emitters at z = 5.7 in the Subaru Deep Field

Author

Shimasaku, Kazuhiro, Kashikawa, Nobunari, Doi, Mamoru, Ly, Chun, Malkan, Matthew A, Matsuda, Yuichi, Ouchi, Masami, Hayashino, Tomoki, Iye, Masanori, Motohara, Kentaro, Murayama, Takashi, Nagao, Tohru, Ohta, Kouji, Okamura, Sadanori, Sasaki, Toshiyuki, Shioya, Yasuhiro, and Taniguchi, Yoshiaki

Subjects
galaxies : evolution, galaxies : high-redshift, galaxies : luminosity function, mass function, galaxies : photometry, astro-ph, Astronomical and Space Sciences, Astronomy & Astrophysics
Abstract

We present the properties of Ly Alpha emitters (LAEs) at z = 5.7 in theSubaru Deep Field. A photometric sample of 89 LAE candidates is constructedfrom narrow-band (NB816) data down to NB816 = 26.0 (AB) in a continuous 725arcmin^2 area. Spectra of 39 objects satisfying the photometric selectioncriteria for LAEs were obtained with Subaru and Keck II Telescopes, among which28 were confirmed LAEs, one was a nearby galaxy, and eight were unclassified.We also obtained spectra of another 24 NB816-excess objects in the field,identifying six additional LAEs. We find that the Ly Alpha luminosity functionderived from the photometric sample is reproduced well by a Schechter functionwith L* = (7.9+3.0-2.2) x 10^42 erg/s and phi* = (6.3+3.0-2.0) x 10^-4 Mpc^-3for alpha = -1.5 (fixed) over the whole luminosity range of L ~= 3x10^42 -3x10^43 erg/s. We then measure rest-frame Ly Alpha equivalent widths (EWs) forthe confirmed LAEs, to find that the median among the 28 objects satisfying thephotometric selection criteria is W_0^i = 233 A. We infer that 30% - 40% ofLAEs at z=5.7 exceed W_0^i = 240 A. These large-EW objects probably cannot beaccounted for by ordinary star-forming populations with a Salpeter IMF. We alsofind that LAEs with fainter far-UV luminosities have larger EWs. Finally, wederive the far-UV luminosity function of LAEs down to M_UV ~= -19.6 using thephotometric sample, and compare it with that of Lyman-break galaxies (LBGs). Wefind that as high as about 80% of LBGs at z ~ 6 have W_0^i >= 100 A, in sharpcontrast to lower-z counterparts.

Published
2006

106. Ly alpha emitters at z=5.7 in the Subaru deep field

Author

Shimasaku, Kazuhiro, Kashikawa, Nobunari, Doi, Mamoru, Ly, Chun, Malkan, Matthew A, Matsuda, Yuichi, Ouchi, Masami, Hayashino, Tomoki, Iye, Masanori, Motohara, Kentaro, Murayama, Takashi, Nagao, Tohru, Ohta, Kouji, Okamura, Sadanori, Sasaki, Toshiyuki, Shioya, Yasuhiro, and Taniguchi, Yoshiaki

Subjects
galaxies : evolution, galaxies : high-redshift, galaxies : luminosity function, mass function, galaxies : photometry, astro-ph, galaxies : luminosity function, mass function, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

We present the properties of Ly Alpha emitters (LAEs) at z = 5.7 in theSubaru Deep Field. A photometric sample of 89 LAE candidates is constructedfrom narrow-band (NB816) data down to NB816 = 26.0 (AB) in a continuous 725arcmin^2 area. Spectra of 39 objects satisfying the photometric selectioncriteria for LAEs were obtained with Subaru and Keck II Telescopes, among which28 were confirmed LAEs, one was a nearby galaxy, and eight were unclassified.We also obtained spectra of another 24 NB816-excess objects in the field,identifying six additional LAEs. We find that the Ly Alpha luminosity functionderived from the photometric sample is reproduced well by a Schechter functionwith L* = (7.9+3.0-2.2) x 10^42 erg/s and phi* = (6.3+3.0-2.0) x 10^-4 Mpc^-3for alpha = -1.5 (fixed) over the whole luminosity range of L ~= 3x10^42 -3x10^43 erg/s. We then measure rest-frame Ly Alpha equivalent widths (EWs) forthe confirmed LAEs, to find that the median among the 28 objects satisfying thephotometric selection criteria is W_0^i = 233 A. We infer that 30% - 40% ofLAEs at z=5.7 exceed W_0^i = 240 A. These large-EW objects probably cannot beaccounted for by ordinary star-forming populations with a Salpeter IMF. We alsofind that LAEs with fainter far-UV luminosities have larger EWs. Finally, wederive the far-UV luminosity function of LAEs down to M_UV ~= -19.6 using thephotometric sample, and compare it with that of Lyman-break galaxies (LBGs). Wefind that as high as about 80% of LBGs at z ~ 6 have W_0^i >= 100 A, in sharpcontrast to lower-z counterparts.

Published
2006

107. Clustering of Lyman Break Galaxies at z = 4 and 5 in the Subaru Deep Field: Luminosity Dependence of the Correlation Function Slope**Based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.

Author

Kashikawa, Nobunari, Yoshida, Makiko, Shimasaku, Kazuhiro, Nagashima, Masahiro, Yahagi, Hideki, Ouchi, Masami, Matsuda, Yuichi, Malkan, Matthew A, Doi, Mamoru, Iye, Masanori, Ajiki, Masaru, Akiyama, Masayuki, Ando, Hiroyasu, Aoki, Kentaro, Furusawa, Hisanori, Hayashino, Tomoki, Iwamuro, Fumihide, Karoji, Hiroshi, Kobayashi, Naoto, Kodaira, Keiichi, Kodama, Tadayuki, Komiyama, Yutaka, Miyazaki, Satoshi, Mizumoto, Yoshihiko, Morokuma, Tomoki, Motohara, Kentaro, Murayama, Takashi, Nagao, Tohru, Nariai, Kyoji, Ohta, Kouji, Okamura, Sadanori, Sasaki, Toshiyuki, Sato, Yasunori, Sekiguchi, Kazuhiro, Shioya, Yasuhiro, Tamura, Hajime, Taniguchi, Yoshiaki, Umemura, Masayuki, Yamada, Toru, and Yasuda, Naoki

Subjects
cosmology : observations, cosmology : theory, galaxies : high-redshift, large-scale structure of universe, astro-ph, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

We explored the clustering properties of Lyman break galaxies at z = 4 and 5 with an angular two-point correlation function on the basis of the very deep and wide Subaru Deep Field data. We confirmed the previous result that the clustering strength of LBGs depends on the UV luminosity in the sense that brighter LBGs are more strongly clustered. In addition, we found an apparent dependence of the correlation function slope on UV luminosity for LBGs at both z = 4 and 5. More luminous LBGs have a steeper correlation function. The bias parameter was found to be a scale-dependent function for bright LBGs, whereas it appears to be almost scale-independent for faint LBGs. Luminous LBGs have a higher bias at smaller angular scales, which decreases as the scale increases. To compare these observational results, we constructed numerical mock LBG catalogs based on a semianalytic model of hierarchical clustering combined with high-resolution N-body simulation, carefully mimicking the observational selection effects. The luminosity functions and the overall correlation functions for LBGs at z = 4 and 5 predicted by this mock catalog were found to be almost consistent with the observation. The observed dependence of the clustering on UV luminosity was not reproduced by the model, unless subsamples of distinct halo mass were considered. That is, LBGs belonging to more massive dark halos had steeper and larger amplitude correlation functions. With this model, we found that LBG multiplicity in massive dark halos amplifies the clustering strength at small scales, which steepens the correlation function. The hierarchical clustering model could therefore be reconciled with the observed luminosity dependence of the correlation function if there is a tight correlation between UV luminosity and halo mass. Our finding that the slope of the correlation function depends on luminosity could be an indication that massive dark halos hosted multiple bright LBGs. © 2006. The American Astronomical Society. All rights reserved.

Published
2006

108. Subtype prediction of primary aldosteronism by combining aldosterone concentrations in the left adrenal vein and inferior vena cava: a multicenter collaborative study on adrenal venous sampling

Author

Fujii, Yuichi, Umakoshi, Hironobu, Wada, Norio, Ichijo, Takamasa, Kamemura, Kohei, Matsuda, Yuichi, Kai, Tatsuya, Fukuoka, Tomikazu, Sakamoto, Ryuichi, Ogo, Atsushi, Suzuki, Tomoko, Nanba, Kazutaka, Tsuiki, Mika, Naruse, Mitsuhide, and on behalf of WAVES-J Study Group

Published
2018
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110. The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field

Author

Hyun, Minhee, primary, Im, Myungshin, additional, Smail, Ian R., additional, Cotton, William D., additional, Birkin, Jack E., additional, Kikuta, Satoshi, additional, Shim, Hyunjin, additional, Willmer, Christopher N. A., additional, Condon, James J., additional, Windhorst, Rogier A., additional, Cohen, Seth H., additional, Jansen, Rolf A., additional, Ly, Chun, additional, Matsuda, Yuichi, additional, Fazio, Giovanni G., additional, Swinbank, A. M., additional, and Yan, Haojing, additional

Published
2023
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112. Association Between Acute Fall in Estimated Glomerular Filtration Rate After Treatment for Primary Aldosteronism and Long-Term Decline in Renal Function

Author

Kobayashi, Hiroki, Abe, Masanori, Nakamura, Yoshihiro, Takahashi, Katsutoshi, Fujita, Megumi, Takeda, Yoshiyu, Yoneda, Takashi, Kurihara, Isao, Itoh, Hiroshi, Tsuiki, Mika, Wada, Norio, Ichijo, Takamasa, Katabami, Takuyuki, Ogawa, Yoshihiro, Kawashima, Junji, Yoshimoto, Takanobu, Sone, Masakatsu, Inagaki, Nobuya, Watanabe, Minemori, Kamemura, Kohei, Matsuda, Yuichi, Izawa, Shoichiro, Tanabe, Makito, Tanabe, Akiyo, Suzuki, Tomoko, and Naruse, Mitsuhide

Published
2019
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113. Sex Difference in the Association Between Subtype Distribution and Age at Diagnosis in Patients With Primary Aldosteronism

Author

Akasaka, Hiroshi, Yamamoto, Koichi, Rakugi, Hiromi, Nagasawa, Motonori, Nakamaru, Ryo, Ichijo, Takamasa, Takeda, Yoshiyu, Kurihara, Isao, Katabami, Takuyuki, Tsuiki, Mika, Wada, Norio, Ogawa, Yoshihiro, Kawashima, Junji, Sone, Masakatsu, Kamemura, Kohei, Yoshimoto, Takanobu, Matsuda, Yuichi, Fujita, Megumi, Kobayashi, Hiroki, Watanabe, Minemori, Tamura, Kouichi, Okamura, Shintaro, Miyauchi, Shozo, Izawa, Shoichiro, Chiba, Yoshiro, Tanabe, Akiyo, and Naruse, Mitsuhide

Published
2019
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114. Impact of adrenocorticotropic hormone stimulation during adrenal venous sampling on outcomes of primary aldosteronism

Author

Takeda, Yoshiyu, Umakoshi, Hironobu, Takeda, Yoshimichi, Yoneda, Takashi, Kurihara, Isao, Katabami, Takuyuki, Ichijo, Takamasa, Wada, Norio, Yoshimoto, Takanobu, Ogawa, Yoshihiro, Kawashima, Junji, Sone, Masakatsu, Takahashi, Katsutoshi, Watanabe, Minemori, Matsuda, Yuichi, Kobayashi, Hiroki, Shibata, Hirotaka, Kamemura, Kohei, Otsuki, Michio, Fujii, Yuichi, Yamamto, Koichi, Ogo, Atsushi, Yanase, Toshihiko, Suzuki, Tomoko, and Naruse, Mitsuhide

Published
2019
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115. An AGN with an Ionized Gas Outflow in a Massive Quiescent Galaxy in a Protocluster at z = 3.09

Author

Kubo, Mariko, primary, Umehata, Hideki, additional, Matsuda, Yuichi, additional, Kajisawa, Masaru, additional, Steidel, Charles C., additional, Yamada, Toru, additional, Tanaka, Ichi, additional, Hatsukade, Bunyo, additional, Tamura, Yoichi, additional, Nakanishi, Kouichiro, additional, Kohno, Kotaro, additional, Lee, Kianhong, additional, Matsuda, Keiichi, additional, Ao, Yiping, additional, Nagao, Tohru, additional, and Yun, Min S., additional

Published
2022
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116. Effect of Intraprocedural Cortisol Measurement on ACTH-stimulated Adrenal Vein Sampling in Primary Aldosteronism

Author

Kometani, Mitsuhiro, primary, Yoneda, Takashi, additional, Karashima, Shigehiro, additional, Takeda, Yoshiyu, additional, Tsuiki, Mika, additional, Yasoda, Akihiro, additional, Kurihara, Isao, additional, Wada, Norio, additional, Katabami, Takuyuki, additional, Sone, Masakatsu, additional, Ichijo, Takamasa, additional, Tamura, Kouichi, additional, Ogawa, Yoshihiro, additional, Kobayashi, Hiroki, additional, Okamura, Shintaro, additional, Inagaki, Nobuya, additional, Kawashima, Junji, additional, Fujita, Megumi, additional, Oki, Kenji, additional, Matsuda, Yuichi, additional, Tanabe, Akiyo, additional, and Naruse, Mitsuhide, additional

Published
2022
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117. Prevalence of Cardiovascular Disease and Its Risk Factors in Primary Aldosteronism: A Multicenter Study in Japan

Author

Ohno, Youichi, Sone, Masakatsu, Inagaki, Nobuya, Yamasaki, Toshinari, Ogawa, Osamu, Takeda, Yoshiyu, Kurihara, Isao, Itoh, Hiroshi, Umakoshi, Hironobu, Tsuiki, Mika, Ichijo, Takamasa, Katabami, Takuyuki, Tanaka, Yasushi, Wada, Norio, Shibayama, Yui, Yoshimoto, Takanobu, Ogawa, Yoshihiro, Kawashima, Junji, Takahashi, Katsutoshi, Fujita, Megumi, Watanabe, Minemori, Matsuda, Yuichi, Kobayashi, Hiroki, Shibata, Hirotaka, Kamemura, Kohei, Otsuki, Michio, Fujii, Yuichi, Yamamoto, Koichi, Ogo, Atsushi, Okamura, Shintaro, Miyauchi, Shozo, Fukuoka, Tomikazu, Izawa, Shoichiro, Yoneda, Takashi, Hashimoto, Shigeatsu, Yanase, Toshihiko, Suzuki, Tomoko, Kawamura, Takashi, Tabara, Yasuharu, Matsuda, Fumihiko, Naruse, Mitsuhide, Kawaguchi, Takahisa, Setoh, Kazuya, Matsuda, Fumihiko, Takahashi, Yoshimitsu, Nakayama, Takeo, and Kosugi, Shinji

Published
2018
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120. Detection of nitrogen and oxygen in a galaxy at the end of reionization

Author

Tadaki, Ken-ichi, primary, Tsujita, Akiyoshi, additional, Tamura, Yoichi, additional, Kohno, Kotaro, additional, Hatsukade, Bunyo, additional, Iono, Daisuke, additional, Lee, Minju M, additional, Matsuda, Yuichi, additional, Michiyama, Tomonari, additional, Nagao, Tohru, additional, Nakanishi, Kouichiro, additional, Nishimura, Yuri, additional, Saito, Toshiki, additional, Umehata, Hideki, additional, and Zavala, Jorge, additional

Published
2022
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124. Gas filaments of the cosmic web located around active galaxies in a protocluster

Author

Fumagalli, M., Smail, I., Swinbank, A. M., Cantalupo, S., Sykes, C., Ivison, R. J., Steidel, C. C., Shapley, A. E., Vernet, J., Nakanishi, K., Kajisawa, M., Umehata, Hideki, Matsuda, Yuichi, Yamada, Toru, Tamura, Yoichi, Kubo, Mariko, Hatsukade, Bunyo, Kohno, Kotaro, Umehata, H, Fumagalli, M, Smail, I, Matsuda, Y, Swinbank, A, Cantalupo, S, Sykes, C, Ivison, R, Steidel, C, Shapley, A, Vernet, J, Yamada, T, Tamura, Y, Kubo, M, Nakanishi, K, Kajisawa, M, Hatsukade, B, and Kohno, K

Subjects
Active galactic nucleus, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmic web, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Radiation, medicine.disease_cause, 01 natural sciences, 0103 physical sciences, Cluster (physics), medicine, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, Multidisciplinary, 010308 nuclear & particles physics, Star formation, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Astrophysics of Galaxies (astro-ph.GA), Intergalactic travel, Ultraviolet, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

著者人数: 18名, Accepted: 2019-09-02, 資料番号: SA1190151000

Published
2019

126. Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program

Author

Tang, Shenli, primary, Silverman, John D., additional, Ding, Xuheng, additional, Li, Junyao, additional, Lee, Khee-Gan, additional, Strauss, Michael A., additional, Goulding, Andy, additional, Schramm, Malte, additional, Kawinwanichakij, Lalitwadee, additional, Xavier Prochaska, J., additional, Hennawi, Joseph F., additional, Imanishi, Masatoshi, additional, Iwasawa, Kazushi, additional, Toba, Yoshiki, additional, Kayo, Issha, additional, Oguri, Masamune, additional, Matsuoka, Yoshiki, additional, Onoue, Masafusa, additional, Jahnke, Knud, additional, Ichikawa, Kohei, additional, Hartwig, Tilman, additional, Kashikawa, Nobunari, additional, Kawaguchi, Toshihiro, additional, Kohno, Kotaro, additional, Matsuda, Yuichi, additional, Nagao, Tohru, additional, Ono, Yoshiaki, additional, Ouchi, Masami, additional, Shimasaku, Kazuhiro, additional, Suh, Hyewon, additional, Suzuki, Nao, additional, Taniguchi, Yoshiaki, additional, Ueda, Yoshihiro, additional, and Yasuda, Naoki, additional

Published
2021
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127. FOREVER22: galaxy formation in protocluster regions

Author

Yajima, Hidenobu, primary, Abe, Makito, additional, Khochfar, Sadegh, additional, Nagamine, Kentaro, additional, Inoue, Akio K, additional, Kodama, Tadayuki, additional, Arata, Shohei, additional, Dalla Vecchia, Claudio, additional, Fukushima, Hajime, additional, Hashimoto, Takuya, additional, Kashikawa, Nobunari, additional, Kubo, Mariko, additional, Li, Yuexing, additional, Matsuda, Yuichi, additional, Mawatari, Ken, additional, Ouchi, Masami, additional, and Umehata, Hideki, additional

Published
2021
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131. A Massive Quiescent Galaxy Confirmed in a Protocluster at z = 3.09

Author

Kubo, Mariko, primary, Umehata, Hideki, additional, Matsuda, Yuichi, additional, Kajisawa, Masaru, additional, Steidel, Charles C., additional, Yamada, Toru, additional, Tanaka, Ichi, additional, Hatsukade, Bunyo, additional, Tamura, Yoichi, additional, Nakanishi, Kouichiro, additional, Kohno, Kotaro, additional, Lee, Kianhong, additional, and Matsuda, Keiichi, additional

Published
2021
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132. ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media

Author

Umehata, Hideki, primary, Smail, Ian, additional, Steidel, Charles C., additional, Hayes, Matthew, additional, Scott, Douglas, additional, Swinbank, A. M., additional, Ivison, R. J., additional, Nagao, Toru, additional, Kubo, Mariko, additional, Nakanishi, Kouichiro, additional, Matsuda, Yuichi, additional, Ikarashi, Soh, additional, Tamura, Yoichi, additional, and Geach, J. E., additional

Published
2021
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133. Physical Characterization of Serendipitously Uncovered Millimeter-wave Line-emitting Galaxies at z ∼ 2.5 behind the Local Luminous Infrared Galaxy VV 114

Author

Mizukoshi, Shoichiro, primary, Kohno, Kotaro, additional, Egusa, Fumi, additional, Hatsukade, Bunyo, additional, Minezaki, Takeo, additional, Saito, Toshiki, additional, Tamura, Yoichi, additional, Iono, Daisuke, additional, Ueda, Junko, additional, Matsuda, Yuichi, additional, Kawabe, Ryohei, additional, Lee, Minju M., additional, Yun, Min S., additional, and Espada, Daniel, additional

Published
2021
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134. SILVERRUSH. IX. Lyα Intensity Mapping with Star-forming Galaxies at z = 5.7 and 6.6: A Possible Detection of Extended Lyα Emission at ≳100 Comoving Kiloparsecs around and beyond the Virial-radius Scale of Galaxy Dark Matter Halos

Author

Kakuma, Ryota, primary, Ouchi, Masami, additional, Harikane, Yuichi, additional, Ono, Yoshiaki, additional, Inoue, Akio K., additional, Komiyama, Yutaka, additional, Kusakabe, Haruka, additional, Lee, Chien-Hsiu, additional, Matsuda, Yuichi, additional, Matsuoka, Yoshiki, additional, Mawatari, Ken, additional, Momose, Rieko, additional, Shibuya, Takatoshi, additional, and Taniguchi, Yoshiaki, additional

Published
2021
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137. Older phase 2 cardiac rehabilitation patients engaged in gardening maintained physical function during the COVID-19 pandemic

Author

Ogura, Asami, primary, Izawa, Kazuhiro P., additional, Tawa, Hideto, additional, Kureha, Fumie, additional, Wada, Masaaki, additional, Harada, Nobuko, additional, Ikeda, Yuki, additional, Kimura, Kaemi, additional, Kondo, Naomi, additional, Kanai, Masashi, additional, Kubo, Ikko, additional, Yoshikawa, Ryohei, additional, and Matsuda, Yuichi, additional

Published
2021
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139. ALMA observations of Lyman Alpha Blobs

Author

Matsuda, Yuichi

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We will introduce our dust and CO observations of high-z extended Lyman Alpha nebulae (Lyman Alpha Blobs or LABs). LABs are the best targets to study the relation between galaxy formation and the circum galactic medium. We detect dust continuum sources for 4 giant LABs suggesting that these star-formation activity is required to illuminate the circum galactic medium in emission. Our CO observations revealed that the associated star-forming galaxies have faint CO luminosity compared to normal SMGs suggesting that they may be at a transient phase from star- burst galaxies to passive galaxies.

Published
2019
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141. CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview

Author

Inoue, Akio K, primary, Yamanaka, Satoshi, additional, Ouchi, Masami, additional, Iwata, Ikuru, additional, Shimasaku, Kazuhiro, additional, Taniguchi, Yoshiaki, additional, Nagao, Tohru, additional, Kashikawa, Nobunari, additional, Ono, Yoshiaki, additional, Mawatari, Ken, additional, Shibuya, Takatoshi, additional, Hayashi, Masao, additional, Ikeda, Hiroyuki, additional, Zhang, Haibin, additional, Liang, Yongming, additional, Lee, Chien-Hsiu, additional, Hilmi, Miftahul, additional, Kikuta, Satoshi, additional, Kusakabe, Haruka, additional, Furusawa, Hisanori, additional, Hayashino, Tomoki, additional, Kajisawa, Masaru, additional, Matsuda, Yuichi, additional, Nakajima, Kimihiko, additional, Momose, Rieko, additional, Harikane, Yuichi, additional, Saito, Tomoki, additional, Kodama, Tadayuki, additional, Kikuchihara, Shotaro, additional, Iye, Masanori, additional, and Goto, Tomotsugu, additional

Published
2020
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142. Dual Supermassive Black Holes at Close Separation Revealed by the Hyper Suprime-Cam Subaru Strategic Program

Author

Silverman, John D., primary, Tang, Shenli, additional, Lee, Khee-Gan, additional, Hartwig, Tilman, additional, Goulding, Andy, additional, Strauss, Michael A., additional, Schramm, Malte, additional, Ding, Xuheng, additional, Riffel, Rogemar A., additional, Fujimoto, Seiji, additional, Hikage, Chiaki, additional, Imanishi, Masatoshi, additional, Iwasawa, Kazushi, additional, Jahnke, Knud, additional, Kayo, Issha, additional, Kashikawa, Nobunari, additional, Kawaguchi, Toshihiro, additional, Kohno, Kotaro, additional, Luo, Wentao, additional, Matsuoka, Yoshiki, additional, Matsuda, Yuichi, additional, Nagao, Tohru, additional, Oguri, Masamune, additional, Ono, Yoshiaki, additional, Onoue, Masafusa, additional, Ouchi, Masami, additional, Shimasaku, Kazuhiro, additional, Suh, Hyewon, additional, Suzuki, Nao, additional, Taniguchi, Yoshiaki, additional, Toba, Yoshiki, additional, Ueda, Yoshihiro, additional, and Yasuda, Naoki, additional

Published
2020
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143. Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Author

Harikane, Yuichi, primary, Ouchi, Masami, additional, Inoue, Akio K., additional, Matsuoka, Yoshiki, additional, Tamura, Yoichi, additional, Bakx, Tom, additional, Fujimoto, Seiji, additional, Moriwaki, Kana, additional, Ono, Yoshiaki, additional, Nagao, Tohru, additional, Tadaki, Ken-ichi, additional, Kojima, Takashi, additional, Shibuya, Takatoshi, additional, Egami, Eiichi, additional, Ferrara, Andrea, additional, Gallerani, Simona, additional, Hashimoto, Takuya, additional, Kohno, Kotaro, additional, Matsuda, Yuichi, additional, Matsuo, Hiroshi, additional, Pallottini, Andrea, additional, Sugahara, Yuma, additional, and Vallini, Livia, additional

Published
2020
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144. Three-dimensional Distribution Map of H i Gas and Galaxies around an Enormous Lyα Nebula and Three QSOs at z = 2.3 Revealed by the H i Tomographic Mapping Technique

Author

Mukae, Shiro, primary, Ouchi, Masami, additional, Cai, Zheng, additional, Lee, Khee-Gan, additional, Prochaska, J. Xavier, additional, Cantalupo, Sebastiano, additional, Ono, Yoshiaki, additional, Zheng, Zheng, additional, Nagamine, Kentaro, additional, Suzuki, Nao, additional, Silverman, John D., additional, Misawa, Toru, additional, Inoue, Akio K., additional, Hennawi, Joseph F., additional, Matsuda, Yuichi, additional, Mawatari, Ken, additional, Sugahara, Yuma, additional, Kojima, Takashi, additional, Shibuya, Takatoshi, additional, Harikane, Yuichi, additional, Fujimoto, Seiji, additional, Chiang, Yi-Kuan, additional, Zhang, Haibin, additional, and Kakuma, Ryota, additional

Published
2020
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146. ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy

Author

Bakx, Tom J L C, primary, Tamura, Yoichi, additional, Hashimoto, Takuya, additional, Inoue, Akio K, additional, Lee, Minju M, additional, Mawatari, Ken, additional, Ota, Kazuaki, additional, Umehata, Hideki, additional, Zackrisson, Erik, additional, Hatsukade, Bunyo, additional, Kohno, Kotaro, additional, Matsuda, Yuichi, additional, Matsuo, Hiroshi, additional, Okamoto, Takashi, additional, Shibuya, Takatoshi, additional, Shimizu, Ikkoh, additional, Taniguchi, Yoshiaki, additional, and Yoshida, Naoki, additional

Published
2020
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147. ALMA band 8 observations of DLA 2233+131 at z = 3.150

Author

Ogura, Kazuyuki, primary, Umehata, Hideki, primary, Taniguchi, Yoshiaki, primary, Matsuda, Yuichi, primary, Kashikawa, Nobunari, primary, Sheth, Kartik, primary, Murata, Katsuhiro, primary, Kajisawa, Masaru, primary, Kobayashi, Masakazu A R, primary, Murayama, Takashi, primary, and Nagao, Tohru, primary

Published
2020
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148. Effect of cosyntropin during adrenal venous sampling on subtype of primary aldosteronism: analysis of surgical outcome

Author

Kobayashi, Hiroki, primary, Nakamura, Yoshihiro, additional, Abe, Masanori, additional, Kurihara, Isao, additional, Itoh, Hiroshi, additional, Ichijo, Takamasa, additional, Takeda, Yoshiyu, additional, Yoneda, Takashi, additional, Katabami, Takuyuki, additional, Tsuiki, Mika, additional, Wada, Norio, additional, Ogawa, Yoshihiro, additional, Sakamoto, Ryuichi, additional, Kawashima, Junji, additional, Sone, Masakatsu, additional, Inagaki, Nobuya, additional, Yoshimoto, Takanobu, additional, Yamada, Tetsuya, additional, Okamoto, Ryuji, additional, Matsuda, Yuichi, additional, Fujita, Megumi, additional, Watanabe, Minemori, additional, Tamura, Kouichi, additional, Tanabe, Akiyo, additional, Naruse, Mitsuhide, additional, and _, _, additional

Published
2020
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149. Planck Far-infrared Detection of Hyper Suprime-Cam Protoclusters at z ∼ 4: Hidden AGN and Star Formation Activity

Author

Kubo, Mariko, primary, Toshikawa, Jun, additional, Kashikawa, Nobunari, additional, Chiang, Yi-Kuan, additional, Overzier, Roderik, additional, Uchiyama, Hisakazu, additional, Clements, David L., additional, Alexander, David M., additional, Matsuda, Yuichi, additional, Kodama, Tadayuki, additional, Ono, Yoshiaki, additional, Goto, Tomotsugu, additional, Cheng, Tai-An, additional, and Ito, Kei, additional

Published
2019
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