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The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796
dc.contributor.author | Díaz Sánchez, Anastasio | |
dc.contributor.author | Dannerbauer, Helmut | |
dc.contributor.author | Sulzenauer, Nikolaus | |
dc.contributor.author | Iglesias Groth, Susana | |
dc.contributor.author | Rebolo López, Rafael | |
dc.date.accessioned | 2021-10-01T12:22:08Z | |
dc.date.available | 2021-10-01T12:22:08Z | |
dc.date.issued | 2021-06 | |
dc.identifier.citation | Díaz-Sánchez, A., Dannerbauer, H., Sulzenauer, N., Iglesias-Groth, S., & Rebolo, R. (2021). The Einstein Ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z = 1.4796. The Astrophysical Journal, 919. | es_ES |
dc.identifier.issn | 0004-637X | |
dc.description.abstract | We report an ultra-bright lensed submillimeter galaxy at zspec = 1:4796, identi_ed as a result of a full-sky cross-correlation of the AllWISE and Planck compact source catalogs aimed to search for bright submillimeter galaxies at z _ 1:5 2:8. APEX/LABOCA observations of the candidate Galaxy reveal a source with ux (S870_m = 54_8 mJy). The position of the APEX source coincides with the position of the AllWISE mid-IR source, and with the Einstein ring GAL-CLUS-022058s, observed with the HST. Archival VLT/FORS observations reveal the redshift of this Einstein ring, zspec = 1:4796, and detection of the CO(5-4) line at zspec = 1:4802 with APEX/nFLASH230 con_rms the redshift of the submillimeter emission. The lensed source appears to be gravitationally magni_ed by a massive foreground galaxy cluster lens at z = 0:36. We use Lenstool to model the gravitational lensing, which is near to a \fold arc" con_guration for an elliptical mass distribution of the central halo, where four images of the lensed galaxy are seen; the mean magni_cation is _L = 18 _ 4. We have determined an intrinsic rest-frame infrared luminosity of LIR _ 1012L_ and a likely star formation rate of _ 70 170 M_ yr1. The molecular gas mass is Mmol _ 2:6 _ 1010M_ and the gas fraction is f = 0:34 _ 0:07. We also obtain a stellar mass log(M_=M_) = 10:7 _ 0:1 and a speci_c star formation rate log(sSFR=Gyr1) = 0:15 _ 0:03. This galaxy lies on the so-called main sequence of star-forming galaxies at this redshift. | es_ES |
dc.description.sponsorship | This publication is based on data acquired with the Atacama Path_nder Experiment (APEX) under programmes ID 105.20N6 and ID 0101.B-0560(A). APEX is a collaboration between the Max-Planck Institut fur Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. We thank Carlos De Breuck, and the APEX team for their support. Based on observations collected at the European Southern Observatory under ESO programme ID 081.A-0693(A). Based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (STECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). This publication makes use of data products from the Wide-_eld Infrared Survey Explorer. Based on observations obtained at the international Gemini Observatory program ID GS-2008A-Q-5. The scientic results reported in this article are based in part on data obtained from the Chandra Data Archive. This work has been partially funded by projects \Participation in the NISP instrument and preparation for the scientific exploitation of Euclid", PID2019-110614GB-C22/AEI/10.13039/501100011033, & PID2019-110614GB-C21 _nanced by the \Agencia Estatal de Investigaci_on" (AEI-MCINN). H.D. acknowledges financial support from the Spanish Ministry of Science, Innovation and Universities (MICIU) under the 2014 Ram_on y Cajal program RYC-2014-15686 and under the AYA2017-84061-P, coffinanced by FEDER (European Regional, Development Funds), and in addition, from the Agencia Estatal de Investigacion del Ministerio de Ciencia e Innovacion (AEI-MCINN) under grant (La evolución de los cúmulos de galaxias desde el amanecer hasta el mediodía cósmico) with reference (PID2019-105776GB-00/DOI:10.13039/501100011033). N.S. acknowledges a research stay at the Instituto de Astrofísica de Canarias, funded by \Short-term grant abroad" (KWA) programme of the University of Vienna. | es_ES |
dc.format | application/pdf | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | The University of Chicago Press | es_ES |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 España | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ | * |
dc.title | The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796 | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.subject.other | Física Aplicada | es_ES |
dc.subject | Ultraluminous infrared galaxies | es_ES |
dc.subject | Starburst galaxies | es_ES |
dc.subject | Strong gravitational lensing | es_ES |
dc.subject | Galaxy clusters | es_ES |
dc.subject | High-redshift galaxies | es_ES |
dc.subject | Submillimeter astronomy | es_ES |
dc.identifier.uri | http://hdl.handle.net/10317/9966 | |
dc.identifier.doi | 10.3847/1538-4357/ac0f75 | |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/ac0f75 | |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | es_ES |
dc.type.version | info:eu-repo/semantics/draft | es_ES |
dc.subject.unesco | 21 Astronomía y Astrofísica | es_ES |
dc.subject.unesco | 2101.04 Galaxias | es_ES |
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