The Astrophysical Journal (Jan 2024)
SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution
- Ikki Mitsuhashi,
- Yuichi Harikane,
- Franz E. Bauer,
- Tom J. L. C. Bakx,
- Andrea Ferrara,
- Seiji Fujimoto,
- Takuya Hashimoto,
- Akio K. Inoue,
- Kazushi Iwasawa,
- Yuri Nishimura,
- Masatoshi Imanishi,
- Yoshiaki Ono,
- Toshiki Saito,
- Yuma Sugahara,
- Hideki Umehata,
- Livia Vallini,
- Tao Wang,
- Jorge A. Zavala
Affiliations
- Ikki Mitsuhashi
- ORCiD
- Department of Astronomy, The University of Tokyo , 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan ; [email protected]; National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering, Waseda University , 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan
- Yuichi Harikane
- ORCiD
- Institute for Cosmic Ray Research, The University of Tokyo , 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8582, Japan
- Franz E. Bauer
- ORCiD
- Instituto de Astrofísica and Centro de Astroingeniería , Facultad de Física, Pontificia Universidad Católica de Chile, Campus San Joaquín, Av. Vicuña Mackenna 4860, Macul Santiago, 7820436, Chile; Millennium Institute of Astrophysics , Nuncio Monseñor Sótero Sanz 100, Of 104, Providencia, Santiago, Chile; Space Science Institute , 4750 Walnut Street, Suite 205, Boulder, CO 80301, USA
- Tom J. L. C. Bakx
- ORCiD
- Department of Space, Earth and Environment, Chalmers University of Technology , Gothenburg, Sweden
- Andrea Ferrara
- ORCiD
- Scuola Normale Superiore , Piazza dei Cavalieri 7, I-56126, Pisa, Italy
- Seiji Fujimoto
- ORCiD
- Department of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard Stop C1400, Austin, TX 78712-1205, USA
- Takuya Hashimoto
- ORCiD
- Tomonaga Center for the History of the Universe (TCHoU), Faculty of Pure and Applied Sciences, University of Tsukuba , Tsukuba, Ibaraki 305-8571, Japan
- Akio K. Inoue
- ORCiD
- Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering, Waseda University , 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan; Department of Physics, School of Advanced Science and Engineering, Faculty of Science and Engineering, Waseda University , 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan
- Kazushi Iwasawa
- ORCiD
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB) , Martí i Franquès, 1, 08028 Barcelona, Spain; ICREA , Pg. Lluís Companys 23, 08010 Barcelona, Spain
- Yuri Nishimura
- ORCiD
- Department of Astronomy, The University of Tokyo , 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan ; [email protected]
- Masatoshi Imanishi
- ORCiD
- National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
- Yoshiaki Ono
- ORCiD
- Institute for Cosmic Ray Research, The University of Tokyo , 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8582, Japan
- Toshiki Saito
- National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
- Yuma Sugahara
- ORCiD
- National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering, Waseda University , 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan
- Hideki Umehata
- ORCiD
- Institute for Advanced Research, Nagoya University , Furocho, Chikusa, Nagoya 464-8602, Japan; Department of Physics, Graduate School of Science, Nagoya University , Furocho, Chikusa, Nagoya 464-8602, Japan; Cahill Center for Astronomy and Astrophysics, California Institute of Technology , MS 249-17, Pasadena, CA 91125, USA
- Livia Vallini
- ORCiD
- INAF-Osservatorio di Astrofisica e Scienza dello Spazio , via Gobetti 93/3, I-40129, Bologna, Italy
- Tao Wang
- ORCiD
- School of Astronomy and Space Science, Nanjing University , Nanjing, Jiangsu 210093, People's Republic of China; Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University , Ministry of Education, Nanjing 210093, People's Republic of China
- Jorge A. Zavala
- ORCiD
- National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
- DOI
- https://doi.org/10.3847/1538-4357/ad5675
- Journal volume & issue
-
Vol. 971,
no. 2
p. 161
Abstract
We present an analysis of the Atacama Large Millimeter-submillimeter Array (ALMA) multiband dust continuum observations for 28 spectroscopically confirmed bright Lyman break galaxies at 5 80 K observed in a galaxy at z = 8.3.
Keywords