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ALMA Lensing Cluster Survey: A strongly lensed multiply imaged dusty system at z ≥ 6

Laporte, N. (author)
University Of Cambridge
Zitrin, A. (author)
Ben-Gurion University of the Negev
Ellis, R. S. (author)
University College London (UCL)
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Fujimoto, S. (author)
Brammer, G. (author)
Richard, J. (author)
Centre national de la recherche scientifique (CNRS)
Oguri, M. (author)
University of Tokyo, Japan
Caminha, G. B. (author)
Rijksuniversiteit Groningen,University of Groningen
Kohno, K. (author)
University of Tokyo, Japan
Yoshimura, Y. (author)
University of Tokyo, Japan
Ao, Y. (author)
University of Science and Technology of China,Chinese Academy of Sciences
Bauer, F. E. (author)
Pontificia Universidad Catolica de Chile,Instituto Milenio de Astrofísica,Millennium Institute of Astrophysics
Caputi, Karina I. (author)
Rijksuniversiteit Groningen,University of Groningen
Egami, E. (author)
University of Arizona
Espada, D. (author)
National Astronomical Observatory of Japan,SKA Organisation,The Graduate University for Advanced Studies (SOKENDAI)
González-López, J. (author)
Las Campanas Observatory,Universidad Diego Portales,Diego Portales University
Hatsukade, B. (author)
University of Tokyo, Japan
Knudsen, Kirsten Kraiberg, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Lee, M. M. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Magdis, Georgios E. (author)
Ouchi, Masami (author)
University of Tokyo, Japan
Valentino, F. (author)
Wang, T. (author)
University of Tokyo, Japan,National Astronomical Observatory of Japan
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 (creator_code:org_t)
2021-01-28
2021
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 505:4, s. 4838-4846
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift z = 6.07 viewed through the cluster MACSJ0600.1–2008 (z = 0.46). A ≃ 4σ dust detection is seen at 1.2mm as part of the ALMA Lensing Cluster Survey (ALCS), an on-going ALMA Large programme, and the redshift is secured via [C II] 158 μm emission described in a companion paper. In addition, spectroscopic follow-up with GMOS/Gemini-North shows a break in the galaxy’s spectrum, consistent with the Lyman break at that redshift. We use a detailed mass model of the cluster and infer a magnification μ ≳ 30 for the most magnified image of this galaxy, which provides an unprecedented opportunity to probe the physical properties of a sub-luminous galaxy at the end of cosmic reionization. Based on the spectral energy distribution, we infer lensing-corrected stellar and dust masses of 2.9-2.3+115 × 109 and 4.8-3.4+45 × 106 M☉, respectively, a star formation rate of 9.7-6.6+220 M☉ yr−1, an intrinsic size of 0.54-0.14+026 kpc, and a luminosity-weighted age of 200 ± 100 Myr. Strikingly, the dust production rate in this relatively young galaxy appears to be larger than that observed for equivalent, lower redshift sources. We discuss if this implies that early supernovae are more efficient dust producers and the consequences for using dust mass as a probe of earlier star formation.

Subject headings

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
MEDICIN OCH HÄLSOVETENSKAP  -- Klinisk medicin -- Radiologi och bildbehandling (hsv//swe)
MEDICAL AND HEALTH SCIENCES  -- Clinical Medicine -- Radiology, Nuclear Medicine and Medical Imaging (hsv//eng)

Keyword

Galaxies: formation
Galaxies: high-redshift
Galaxies: evolution
Gravitational lensing: strong

Publication and Content Type

art (subject category)
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