SwePub
Sök i LIBRIS databas

  Utökad sökning

WFRF:(Caminha G.)
 

Sökning: WFRF:(Caminha G.) > ALMA Lensing Cluste...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005472naa a2200697 4500
001oai:research.chalmers.se:4a5ff42d-638d-4f54-8127-dd1ae2e41e3b
003SwePub
008210718s2021 | |||||||||||000 ||eng|
0247 a https://research.chalmers.se/publication/5249512 URI
0247 a https://doi.org/10.1093/mnras/stab1912 DOI
0247 a https://research.chalmers.se/publication/5249472 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
1001 a Laporte, N.u University Of Cambridge4 aut
2451 0a ALMA Lensing Cluster Survey: A strongly lensed multiply imaged dusty system at z ≥ 6
264 c 2021-01-28
264 1b 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 7a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a MEDICIN OCH HÄLSOVETENSKAPx Klinisk medicinx Radiologi och bildbehandling0 (SwePub)302082 hsv//swe
650 7a 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
7001 a Zitrin, A.u Ben-Gurion University of the Negev4 aut
7001 a Ellis, R. S.u University College London (UCL)4 aut
7001 a Fujimoto, S.4 aut
7001 a Brammer, G.4 aut
7001 a Richard, J.u Centre national de la recherche scientifique (CNRS)4 aut
7001 a Oguri, M.u University of Tokyo, Japan4 aut
7001 a Caminha, G. B.u Rijksuniversiteit Groningen,University of Groningen4 aut
7001 a Kohno, K.u University of Tokyo, Japan4 aut
7001 a Yoshimura, Y.u University of Tokyo, Japan4 aut
7001 a Ao, Y.u University of Science and Technology of China,Chinese Academy of Sciences4 aut
7001 a Bauer, F. E.u Pontificia Universidad Catolica de Chile,Instituto Milenio de Astrofísica,Millennium Institute of Astrophysics4 aut
7001 a Caputi, Karina I.u Rijksuniversiteit Groningen,University of Groningen4 aut
7001 a Egami, E.u University of Arizona4 aut
7001 a Espada, D.u National Astronomical Observatory of Japan,SKA Organisation,The Graduate University for Advanced Studies (SOKENDAI)4 aut
7001 a González-López, J.u Las Campanas Observatory,Universidad Diego Portales,Diego Portales University4 aut
7001 a Hatsukade, B.u University of Tokyo, Japan4 aut
7001 a Knudsen, Kirsten Kraiberg,d 1976u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)kraiberg
7001 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
7001 a Magdis, Georgios E.4 aut
7001 a Ouchi, Masamiu University of Tokyo, Japan4 aut
7001 a Valentino, F.4 aut
7001 a Wang, T.u University of Tokyo, Japan,National Astronomical Observatory of Japan4 aut
7102 a University Of Cambridgeb Ben-Gurion University of the Negev4 org
7730 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
8564 u https://research.chalmers.se/publication/524951/file/524951_Fulltext.pdfx primaryx freey FULLTEXT
8564 u https://discovery.ucl.ac.uk/10119895/1/2101.01740.pdf
8564 8u https://research.chalmers.se/publication/524951
8564 8u https://doi.org/10.1093/mnras/stab191
8564 8u https://research.chalmers.se/publication/524947

Hitta via bibliotek

Till lärosätets databas

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Stäng

Kopiera och spara länken för att återkomma till aktuell vy