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      Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O iii] 88 μm, [C ii] 158 μm, and dust continuum with ALMA

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            The Galactic Disk Mass Function: Reconciliation of the [ITAL]Hubble Space Telescope[/ITAL] and Nearby Determinations

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                Author and article information

                Journal
                Title: Publications of the Astronomical Society of Japan
                Publisher: Oxford University Press (OUP)
                ISSN (Print): 0004-6264
                ISSN (Electronic): 2053-051X
                Publication date Created: June 17 2019
                Publication date (Electronic): June 17 2019
                Affiliations
                [1 ]Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan
                [2 ]Department of Environmental Science and Technology, Faculty of Design Technology, Osaka Sangyo University, 3-1-1 Nagaito, Daito, Osaka 574-8530, Japan
                [3 ]National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
                [4 ]Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan
                [5 ]Division of Particle and Astrophysical Science, Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
                [6 ]Department of Astronomical Science, School of Physical Sciences, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
                [7 ]Department of Physics, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
                [8 ]Department of Computer Science, Kitami Institute of Technology, 165 Koen-cho, Kitami, Hokkaido 090-8507, Japan
                [9 ]Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden
                [10 ]Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan
                [11 ]Research Center for the Early Universe, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
                [12 ]Observational Astrophysics, Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
                [13 ]Department of Cosmosciences, Graduates School of Science, Hokakido University, N10 W8, Kitaku, Sapporo, Hokkaido 060-0810, Japan
                [14 ]Geneva Observatory, University of Geneva, Ch. des Maillettes, 51, 1290 Versoix, Switzerland
                [15 ]Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan
                [16 ]Kyoto University Research Administration Office, Yoshida-Honmachi, Sakyo-ku, Kyoto, Kyoto 606-8501, Japan
                [17 ]Theoretical Astrophysics, Department of Earth & Space Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan
                [18 ]The Open University of Japan, 2-11 Wakaba, Mihama-ku, Chiba, Chiba 261-8586, Japan
                [19 ]RIKEN Cluster for Pioneering Research, 2-1 Hirosawa, Wako-shi, Saitama, Saitama 351-0198, Japan
                [20 ]Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Lyngbyvej 2, 4. sal, DK-2100 Copenhagen, Denmark
                Article
                DOI: 10.1093/pasj/psz049
                SO-VID: 9c9cfd60-f5ee-4978-98ff-5d143323e1e5
                Copyright © © 2019
                License:

                https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model

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