Sökning: onr:"swepub:oai:research.chalmers.se:4a5ff42d-638d-4f54-8127-dd1ae2e41e3b" > ALMA Lensing Cluste...
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000 | 05472naa a2200697 4500 | |
001 | oai:research.chalmers.se:4a5ff42d-638d-4f54-8127-dd1ae2e41e3b | |
003 | SwePub | |
008 | 210718s2021 | |||||||||||000 ||eng| | |
024 | 7 | a https://research.chalmers.se/publication/5249512 URI |
024 | 7 | a https://doi.org/10.1093/mnras/stab1912 DOI |
024 | 7 | a https://research.chalmers.se/publication/5249472 URI |
040 | a (SwePub)cth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a art2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Laporte, N.u University Of Cambridge4 aut |
245 | 1 0 | a ALMA Lensing Cluster Survey: A strongly lensed multiply imaged dusty system at z ≥ 6 |
264 | c 2021-01-28 | |
264 | 1 | b Oxford University Press (OUP),c 2021 |
338 | a electronic2 rdacarrier | |
520 | a 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. | |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
650 | 7 | a MEDICIN OCH HÄLSOVETENSKAPx Klinisk medicinx Radiologi och bildbehandling0 (SwePub)302082 hsv//swe |
650 | 7 | a MEDICAL AND HEALTH SCIENCESx Clinical Medicinex Radiology, Nuclear Medicine and Medical Imaging0 (SwePub)302082 hsv//eng |
653 | a Galaxies: formation | |
653 | a Galaxies: high-redshift | |
653 | a Galaxies: evolution | |
653 | a Gravitational lensing: strong | |
700 | 1 | a Zitrin, A.u Ben-Gurion University of the Negev4 aut |
700 | 1 | a Ellis, R. S.u University College London (UCL)4 aut |
700 | 1 | a Fujimoto, S.4 aut |
700 | 1 | a Brammer, G.4 aut |
700 | 1 | a Richard, J.u Centre national de la recherche scientifique (CNRS)4 aut |
700 | 1 | a Oguri, M.u University of Tokyo, Japan4 aut |
700 | 1 | a Caminha, G. B.u Rijksuniversiteit Groningen,University of Groningen4 aut |
700 | 1 | a Kohno, K.u University of Tokyo, Japan4 aut |
700 | 1 | a Yoshimura, Y.u University of Tokyo, Japan4 aut |
700 | 1 | a Ao, Y.u University of Science and Technology of China,Chinese Academy of Sciences4 aut |
700 | 1 | a Bauer, F. E.u Pontificia Universidad Catolica de Chile,Instituto Milenio de Astrofísica,Millennium Institute of Astrophysics4 aut |
700 | 1 | a Caputi, Karina I.u Rijksuniversiteit Groningen,University of Groningen4 aut |
700 | 1 | a Egami, E.u University of Arizona4 aut |
700 | 1 | a Espada, D.u National Astronomical Observatory of Japan,SKA Organisation,The Graduate University for Advanced Studies (SOKENDAI)4 aut |
700 | 1 | a González-López, J.u Las Campanas Observatory,Universidad Diego Portales,Diego Portales University4 aut |
700 | 1 | a Hatsukade, B.u University of Tokyo, Japan4 aut |
700 | 1 | a Knudsen, Kirsten Kraiberg,d 1976u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)kraiberg |
700 | 1 | a Lee, M. M.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut |
700 | 1 | a Magdis, Georgios E.4 aut |
700 | 1 | a Ouchi, Masamiu University of Tokyo, Japan4 aut |
700 | 1 | a Valentino, F.4 aut |
700 | 1 | a Wang, T.u University of Tokyo, Japan,National Astronomical Observatory of Japan4 aut |
710 | 2 | a University Of Cambridgeb Ben-Gurion University of the Negev4 org |
773 | 0 | t Monthly Notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 505:4, s. 4838-4846q 505:4<4838-4846x 0035-8711x 1365-2966 |
856 | 4 | u https://research.chalmers.se/publication/524951/file/524951_Fulltext.pdfx primaryx freey FULLTEXT |
856 | 4 | u https://discovery.ucl.ac.uk/10119895/1/2101.01740.pdf |
856 | 4 8 | u https://research.chalmers.se/publication/524951 |
856 | 4 8 | u https://doi.org/10.1093/mnras/stab191 |
856 | 4 8 | u https://research.chalmers.se/publication/524947 |
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