PS J2107-1611: A new wide-separation, quadruply imaged lensed quasar with flux ratio anomalies
dc.contributor.author | Dux, Frédéric | |
dc.contributor.author | Lemon, Cameron | |
dc.contributor.author | Courbin, Frédéric | |
dc.contributor.author | Sluse, Dominique | |
dc.contributor.author | Smette, Alain | |
dc.contributor.author | Anguita, Timo | |
dc.contributor.author | Neira, Favio | |
dc.date.accessioned | 2025-01-27T19:01:46Z | |
dc.date.available | 2025-01-27T19:01:46Z | |
dc.date.issued | 2023-11 | |
dc.description | Indexación: Scopus | |
dc.description.abstract | We report the discovery of PS J2107-1611, a fold-configuration 4.3′′-separation quadruply lensed quasar with a bright lensed arc. It was discovered using a convolutional neural network on Pan-STARRS gri images of pre-selected quasar candidates with multiple nearby Pan-STARRS detections. Spectroscopic follow-up with EFOSC2 on the ESO 3.58 m New Technology Telescope reveals the source to be a quasar at z = 2.673, with the blended fold image pair showing deformed broad lines relative to the other images. The flux ratios measured from optical to near-infrared imaging in the Canada-France-Hawaii Telescope Legacy Survey, Pan-STARRS, the Legacy Surveys, and the Vista Hemisphere Survey are inconsistent with a smooth mass model as the fold pair images are ∼15 times too faint. Variability, time delay effects, and reddening are ruled out through multiple-epoch imaging and color information. The system is marginally resolved in the radio in the Very Large Array Sky Survey S-band, where it has a 10 mJy detection. The radio flux ratios are compatible with the smooth mass macromodel. This system offers a unique tool for future studies of quasar structure with strong and microlensing. A more detailed analysis of follow-up with JWST/MIRI, VLT/MUSE, VLT/ERIS, and data from the European Very Long Baseline Interferometer will be presented in a forthcoming paper. © 2023 EDP Sciences. All rights reserved. | |
dc.description.uri | https://www.aanda.org/articles/aa/full_html/2023/11/aa48227-23/aa48227-23.html | |
dc.identifier.citation | Astronomy and Astrophysics. Volume 679. 1 November 2023. Article number L4 | |
dc.identifier.doi | 10.1051/0004-6361/202348227 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.uri | https://repositorio.unab.cl/handle/ria/63307 | |
dc.language.iso | en | |
dc.publisher | EDP Sciences | |
dc.rights.license | Attribution 4.0 International Deed (CC BY 4.0) | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.subject | Galaxies: Active | |
dc.subject | Gravitational lensing: strong | |
dc.title | PS J2107-1611: A new wide-separation, quadruply imaged lensed quasar with flux ratio anomalies | |
dc.type | Artículo |
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