ALMA Lensing Cluster Survey: Bright [CII] 158 $\mu$m Lines from a Multiply Imaged Sub-$L^{\star}$ Galaxy at $z=6.0719$ - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue Astrophys.J. Année : 2021

ALMA Lensing Cluster Survey: Bright [CII] 158 $\mu$m Lines from a Multiply Imaged Sub-$L^{\star}$ Galaxy at $z=6.0719$

Seiji Fujimoto
Masamune Oguri
Gabriel Brammer
Yuki Yoshimura
  • Fonction : Auteur
Nicolas Laporte
Jorge Gonzalez-Lopez
  • Fonction : Auteur
Gabriel B. Caminha
  • Fonction : Auteur
Kotaro Kohno
Adi Zitrin
Masami Ouchi
  • Fonction : Auteur
Franz E. Bauer
  • Fonction : Auteur
Ian Smail
Bunyo Hatsukade
  • Fonction : Auteur
Yoshiaki Ono
  • Fonction : Auteur
Vasily Kokorev
Hideki Umehata
  • Fonction : Auteur
Kirsten Knudsen
  • Fonction : Auteur
Fengwu Sun
Georgios Magdis
Francesco Valentino
Yiping Ao
  • Fonction : Auteur
Sune Toft
Miroslava Dessauges-Zavadsky
Kazuhiro Shimasaku
  • Fonction : Auteur
Karina Caputi
  • Fonction : Auteur
Haruka Kusakabe
  • Fonction : Auteur
Kana Morokuma-Matsui
  • Fonction : Auteur
Kikuchihara Shotaro
  • Fonction : Auteur
Eiichi Egami
Minju M. Lee
  • Fonction : Auteur
Timothy Rawle
Daniel Espada
  • Fonction : Auteur

Résumé

We present bright [C ii] 158 μm line detections from a strongly magnified and multiply imaged (μ ∼ 20–160) sub–L * () Lyman-break galaxy (LBG) at z = 6.0719 ± 0.0004, drawn from the ALMA Lensing Cluster Survey (ALCS). Emission lines are identified at 268.7 GHz at ≥8σ exactly at the positions of two multiple images of the LBG, behind the massive galaxy cluster RXCJ0600−2007. Our lens models, updated with the latest spectroscopy from VLT/MUSE, indicate that a sub region of the LBG crosses the caustic, and is lensed into a long (∼6″) arc with a local magnification of μ ∼ 160, for which the [C ii] line is also significantly detected. The source plane reconstruction resolves the interstellar medium (ISM) structure, showing that the [C ii] line is co-spatial with the rest-frame UV continuum at a scale of ∼300 pc. The [C ii] line properties suggest that the LBG is a rotation-dominated system, whose velocity gradient explains a slight difference in redshifts between the whole LBG and its sub-region. The star formation rate (SFR)–L [CII] relations, for whole and sub-regions of the LBG, are consistent with those of local galaxies. We evaluate the lower limit of the faint-end of the [C ii] luminosity function at z = 6, finding it to be consistent with predictions from semi-analytical models and from the local SFR–L [CII] relation with a SFR function at z = 6. These results imply that the local SFR–L [CII] relation is universal for a wide range of scales, including the spatially resolved ISM, the whole region of the galaxy, and the cosmic scale, even in the epoch of reionization.

Dates et versions

hal-03129481 , version 1 (02-02-2021)

Identifiants

Citer

Seiji Fujimoto, Masamune Oguri, Gabriel Brammer, Yuki Yoshimura, Nicolas Laporte, et al.. ALMA Lensing Cluster Survey: Bright [CII] 158 $\mu$m Lines from a Multiply Imaged Sub-$L^{\star}$ Galaxy at $z=6.0719$. Astrophys.J., 2021, 911 (2), pp.99. ⟨10.3847/1538-4357/abd7ec⟩. ⟨hal-03129481⟩
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