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

ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of har...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society Vol. 493; no. 3; pp. 4294 - 4307
Main Authors:	Bakx, Tom J L C, Tamura, Yoichi, Hashimoto, Takuya, Inoue, Akio K, Lee, Minju M, Mawatari, Ken, Ota, Kazuaki, Umehata, Hideki, Zackrisson, Erik, Hatsukade, Bunyo, Kohno, Kotaro, Matsuda, Yuichi, Matsuo, Hiroshi, Okamoto, Takashi, Shibuya, Takatoshi, Shimizu, Ikkoh, Taniguchi, Yoshiaki, Yoshida, Naoki
Format:	Journal Article
Language:	English
Published:	London Oxford University Press 01.04.2020
Subjects:	Confidence limits Continuum radiation Cosmic dust Dust Galaxies galaxies: formation galaxies: high-redshift galaxies: ISM Interstellar matter Interstellar radiation Ionization Luminosity Photodissociation Physical properties Radio telescopes galaxies: formation galaxies: ISM galaxies: high-redshift
ISSN:	0035-8711, 1365-2966, 1365-2966
Online Access:	Get full text
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