cosmological parameters; cosmology: observations; dark energy; distance scale; galaxies: evolution; Compound lens; Cosmological parameters; Cosmology observations; Dark energy; Distance scale; Galaxy evolution; Light curves; Multiple image; Optical path; Red shift; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] We report the discovery of the first example of an Einstein zigzag lens, an extremely rare lensing configuration. In this system, J1721+8842, six images of the same background quasar are formed by two intervening galaxies, one at redshift z1 = 0.184 and another at z2 = 1.885. Two out of the six multiple images are deflected in opposite directions as they pass the first lens galaxy on one side and the second on the other side – the optical paths forming zigzags between the two deflectors. In this paper we demonstrate that J1721+8842, previously thought to be a lensed dual quasar, is in fact a compound lens, with the more distant lens galaxy also being distorted as an arc by the foreground galaxy. Evidence supporting this unusual lensing scenario includes: (1) identical light curves in all six lensed quasar images obtained from two years of monitoring at the Nordic Optical Telescope; (2) detection of the additional deflector at redshift z2 = 1.885 in JWST/NIRSpec integral field unit data; and (3) a multiple-plane lens model reproducing the observed image positions. This unique configuration offers the opportunity to combine two major lensing cosmological probes, time-delay cosmography and dual source-plane lensing, since J1721+8842 features multiple lensed sources that form two distinct Einstein radii of different sizes, one of which is a variable quasar. We expect to place tight constraints on H0 and w by combining these two probes of the same system. The z2 = 1.885 deflector, a quiescent galaxy, is also the highest-redshift strong galaxy-scale lens with a spectroscopic redshift measurement known to date.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Dux, F. ; European Southern Observatory, Santiago, Chile ; Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, Versoix, Switzerland
Millon, M. ; Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics, Stanford University, Stanford, United States ; Institute for Particle Physics and Astrophysics, ETH Zurich, Zurich, Switzerland
Lemon, C.; Oskar Klein Centre, Department of Physics, Stockholm University, Stockholm, Sweden
Schmidt, T.; UCLA Physics & Astronomy, Los Angeles, United States
Courbin, F.; Institut de Ciències del Cosmos, Universitat de Barcelona, Barcelona, Spain ; ICREA, Barcelona, Spain
Shajib, A.J. ; Department of Astronomy & Astrophysics, University of Chicago, Chicago, United States ; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, United States
Treu, T. ; UCLA Physics & Astronomy, Los Angeles, United States
Birrer, S. ; Department of Physics and Astronomy, Stony Brook University, Stony Brook, United States
Wong, K.C. ; Research Center for the Early Universe, Graduate School of Science, The University of Tokyo, Tokyo, Japan
Agnello, A.; DARK, Niels Bohr Institute, University of Copenhagen, Copenhagen N, Denmark ; STFC Hartree Centre, Sci-Tech Daresbury, Warrington, United Kingdom
Andrade, A.; European Southern Observatory, Santiago, Chile ; Universidad Andres Bellos, Santiago, Chile
Galan, A. ; Technical University of Munich, TUM School of Natural Sciences, Physics Department, Garching, Germany ; Max-Planck-Institut für Astrophysik, Garching, Germany
Hjorth, J.; DARK, Niels Bohr Institute, University of Copenhagen, Copenhagen N, Denmark
Paic, E. ; Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, Versoix, Switzerland
Schuldt, S.; Dipartimento di Fisica, Università degli Studi di Milano, Milano, Italy ; INAF, IASF Milano, Milano, Italy
Schweinfurth, A. ; Technical University of Munich, TUM School of Natural Sciences, Physics Department, Garching, Germany ; Max-Planck-Institut für Astrophysik, Garching, Germany
Sluse, Dominique ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO)
Smette, A. ; European Southern Observatory, Santiago, Chile
Suyu, S.H.; Technical University of Munich, TUM School of Natural Sciences, Physics Department, Garching, Germany ; Max-Planck-Institut für Astrophysik, Garching, Germany
SNF - Schweizerischer Nationalfonds zur Förderung der wissenschaftlichen Forschung ERC - European Research Council Marie Skłodowska-Curie Actions DFG - Deutsche Forschungsgemeinschaft JSPS - Japan Society for the Promotion of Science Villum Fonden European Union
Funding text :
The first two authors should be regarded as joint first authors. MM acknowledges support by the SNSF (Swiss National Science Foundation) through mobility grant P500PT_203114 and return CH grant P5R5PT_225598. FC acknowledges support from the SNSF and by the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (COSMICLENS: grant agreement No 787886). This project has received funding from the European Union\u2019s Horizon Europe research and innovation programme under the Marie Sklodovska-Curie grant agreement No 101105725. SS has received funding from the European Union\u2019s Horizon 2022 research and innovation programme under the Marie Sk\u0142odowska-Curie grant agreement No 101105167 \u2013 FASTIDIoUS. SHS thanks the Max Planck Society for support through the Max Planck Fellowship. This research is supported in part by the Excellence Cluster ORIGINS which is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany\u2019s Excellence Strategy \u2013 EXC-2094 \u2013 390783311. This work is supported by JSPS KAKENHI Grant Numbers JP24K07089, JP24H00221.AA has been partially supported by the Villum Experiment grant Cosmic Beacons (project number 36225; PIs Agnello, Izzo). This work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program #2974. Support for program #2974 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. This work was supported by research grants (VIL16599, VIL54489) from VILLUM FONDEN. The NOT light curves were extracted with lightcurver (Dux 2024).