WFRF:(Caminha G.)
Sökning: WFRF:(Caminha G.) > ALMA Lensing Cluste...
LIBRIS Formathandbok (Information om MARC21)
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05947naa a2200697 4500 | |
| 001 | oai:research.chalmers.se:635714ac-b36f-4b6b-90cd-392fc2c6d44d | |
| 003 | SwePub | |
| 008 | 210304s2021 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://research.chalmers.se/publication/5226262 URI |
| 024 | 7 | a https://doi.org/10.3847/1538-4357/abd4d02 DOI |
| 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 Caputi, K. I.u Köpenhamns universitet,University of Copenhagen,Rijksuniversiteit Groningen,University of Groningen4 aut |
| 245 | 1 0 | a ALMA Lensing Cluster Survey: An ALMA Galaxy Signposting a MUSE Galaxy Group at z=4.3 Behind "El Gordo" |
| 264 | c 2021-02-19 | |
| 264 | 1 | b American Astronomical Society,c 2021 |
| 520 | a We report the discovery of a Multi Unit Spectroscopic Explorer (MUSE) galaxy group at z = 4.32 lensed by the massive galaxy cluster ACT-CL J0102-4915 (aka El Gordo) at z = 0.87, associated with a 1.2 mm source that is at a 2.07 0.88 kpc projected distance from one of the group galaxies. Three images of the whole system appear in the image plane. The 1.2 mm source has been detected within the Atacama Large Millimetre/submillimetre Array (ALMA) Lensing Cluster Survey (ALCS). As this ALMA source is undetected at wavelengths lambda < 2 mu m, its redshift cannot be independently determined, however, the three lensing components indicate that it belongs to the same galaxy group at z = 4.32. The four members of the MUSE galaxy group have low to intermediate stellar masses (similar to 10(7)-10(10) M) and star formation rates (SFRs) of 0.4-24 M yr(-1), resulting in high specific SFRs (sSFRs) for two of them, which suggest that these galaxies are growing fast (with stellar mass doubling times of only similar to 2 x 10(7) yr). This high incidence of starburst galaxies is likely a consequence of interactions within the galaxy group, which is compact and has high velocity dispersion. Based on the magnification-corrected sub-/millimeter continuum flux density and estimated stellar mass, we infer that the ALMA source is classified as an ordinary ultra-luminous infrared galaxy (with associated dust-obscured SFR similar to 200-300 M yr(-1)) and lies on the star formation main sequence. This reported case of an ALMA/MUSE group association suggests that some presumably isolated ALMA sources are in fact signposts of richer star-forming environments at high redshifts. | |
| 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 NATURVETENSKAPx Geovetenskap och miljövetenskapx Geofysik0 (SwePub)105052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Geophysics0 (SwePub)105052 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Data- och informationsvetenskapx Datorseende och robotik0 (SwePub)102072 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Computer and Information Sciencesx Computer Vision and Robotics0 (SwePub)102072 hsv//eng |
| 653 | a Starburst galaxies | |
| 653 | a Submillimeter astronomy | |
| 653 | a High-redshift galaxies | |
| 653 | a Galaxy groups | |
| 700 | 1 | a Caminha, G. B.u Rijksuniversiteit Groningen,University of Groningen4 aut |
| 700 | 1 | a Fujimoto, S.u Köpenhamns universitet,University of Copenhagen4 aut |
| 700 | 1 | a Kohno, K.u University of Tokyo, Japan4 aut |
| 700 | 1 | a Sun, F.u University of Arizona4 aut |
| 700 | 1 | a Egami, E.u University of Arizona4 aut |
| 700 | 1 | a Deshmukh, S.u Rijksuniversiteit Groningen,University of Groningen4 aut |
| 700 | 1 | a Tang, F.u Rijksuniversiteit Groningen,University of Groningen4 aut |
| 700 | 1 | a Ao, Y.u University of Science and Technology of China,Chinese Academy of Sciences4 aut |
| 700 | 1 | a Bradley, L.u Space Telescope Science Institute (STScI)4 aut |
| 700 | 1 | a Coe, D.u Space Telescope Science Institute (STScI)4 aut |
| 700 | 1 | a Espada, D.u SKA Organisation4 aut |
| 700 | 1 | a Grillo, C.u Istituto nazionale di astrofisica (INAF),Universita' degli Studi di Milano,University of Milan,Köpenhamns universitet,University of Copenhagen4 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, G. E.u Köpenhamns universitet,University of Copenhagen,Danmarks Tekniske Universitet,Technical University of Denmark4 aut |
| 700 | 1 | a Morokuma-Matsui, K.u University of Tokyo, Japan4 aut |
| 700 | 1 | a Oesch, P.u Université de Genève,University of Geneva4 aut |
| 700 | 1 | a Ouchi, M.u University of Tokyo, Japan,National Astronomical Observatory of Japan4 aut |
| 700 | 1 | a Rosati, P.u University of Ferrara,Istituto nazionale di astrofisica (INAF)4 aut |
| 700 | 1 | a Umehata, H.u University of Tokyo, Japan,RIKEN4 aut |
| 700 | 1 | a Valentino, F.u Köpenhamns universitet,University of Copenhagen4 aut |
| 700 | 1 | a Vanzella, E.u Istituto nazionale di astrofisica (INAF)4 aut |
| 700 | 1 | a Wang, W. -H.u Academia Sinica Taiwan4 aut |
| 700 | 1 | a Wu, J. F.u Space Telescope Science Institute (STScI)4 aut |
| 700 | 1 | a Zitrin, A.u Ben-Gurion University of the Negev4 aut |
| 710 | 2 | a Köpenhamns universitetb Rijksuniversiteit Groningen4 org |
| 773 | 0 | t Astrophysical Journald : American Astronomical Societyg 908:2q 908:2x 1538-4357x 0004-637X |
| 856 | 4 | u https://iopscience.iop.org/article/10.3847/1538-4357/abd4d0/pdf |
| 856 | 4 8 | u https://research.chalmers.se/publication/522626 |
| 856 | 4 8 | u https://doi.org/10.3847/1538-4357/abd4d0 |
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