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| DOI | 10.1051/0004-6361/202452970 | ||||
| Año | 2025 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
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 z(1) = 0.184 and another at z(2) = 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 z(2) = 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 H-0 and w by combining these two probes of the same system. The z(2) = 1.885 deflector, a quiescent galaxy, is also the highest-redshift strong galaxy-scale lens with a spectroscopic redshift measurement known to date.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Dux, F. | - |
European Southern Observ - Chile
Ecole Polytech Fed Lausanne EPFL - Suiza European Southern Observatory Santiago - Chile Ecole Polytechnique Fédérale de Lausanne - Suiza |
| 2 | Millon, M. | Hombre |
Stanford Univ - Estados Unidos
Swiss Fed Inst Technol - Suiza Kavli Institute for Particle Astrophysics and Cosmology - Estados Unidos ETH Zurich - Suiza |
| 3 | Lemon, C. | - |
Stockholm Univ - Suecia
Oskar Klein Centre - Suecia |
| 4 | Schmidt, T. | - |
UCLA Phys & Astron - Estados Unidos
University of California, Los Angeles - Estados Unidos |
| 5 | Courbin, Fred | Hombre |
Univ Barcelona - España
ICREA - España Universitat de Barcelona - España Institució Catalana de Recerca i Estudis Avançats - España |
| 6 | Shajib, A. J. | - |
UNIV CHICAGO - Estados Unidos
The Department of Astronomy and Astrophysics, The University of Chicago - Estados Unidos The Kavli Institute for Cosmological Physics - Estados Unidos |
| 7 | Treu, Tommaso | Hombre |
UCLA Phys & Astron - Estados Unidos
University of California, Los Angeles - Estados Unidos |
| 8 | Birrer, Simon | Hombre |
SUNY Stony Brook - Estados Unidos
Stony Brook University - Estados Unidos |
| 9 | Wong, K. C. | - |
Univ Tokyo - Japón
Research Center for the Early Universe - Japón |
| 10 | Agnello, A. | Hombre |
Univ Copenhagen - Dinamarca
Scitech Daresbury - Reino Unido Niels Bohr Institutet - Dinamarca STFC Hartree Centre - Reino Unido |
| 11 | Andrade, A. | - |
European Southern Observ - Chile
Universidad Nacional Andrés Bello - Chile European Southern Observatory Santiago - Chile |
| 12 | Galan, A. | - |
TECH UNIV MUNICH - Alemania
Max Planck Inst Astrophys - Alemania Technische Universität München - Alemania Max Planck Institute for Astrophysics - Alemania |
| 13 | Hjorth, Jens | Hombre |
Univ Copenhagen - Dinamarca
Niels Bohr Institutet - Dinamarca |
| 14 | Paic, E. | - |
Ecole Polytech Fed Lausanne EPFL - Suiza
Ecole Polytechnique Fédérale de Lausanne - Suiza |
| 15 | Schuldt, S. | Hombre |
Univ Milan - Italia
INAF - Italia Università degli Studi di Milano - Italia INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia |
| 16 | Schweinfurth, A. | - |
TECH UNIV MUNICH - Alemania
Max Planck Inst Astrophys - Alemania Technische Universität München - Alemania Max Planck Institute for Astrophysics - Alemania |
| 17 | Sluse, Dominique | - |
STAR Inst - Bélgica
Universite de Liege - Bélgica |
| 18 | Smette, A. | - |
European Southern Observ - Chile
European Southern Observatory Santiago - Chile |
| 19 | Suyu, Sherry H. | Mujer |
TECH UNIV MUNICH - Alemania
Max Planck Inst Astrophys - Alemania Technische Universität München - Alemania Max Planck Institute for Astrophysics - Alemania |
| Fuente |
|---|
| European Union |
| Deutsche Forschungsgemeinschaft |
| JSPS KAKENHI |
| European Research Council |
| NASA |
| Japan Society for the Promotion of Science |
| National Aeronautics and Space Administration |
| Max-Planck-Gesellschaft |
| VILLUM FONDEN |
| SNSF |
| Space Telescope Science Institute |
| Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung |
| H2020 Marie Skłodowska-Curie Actions |
| Horizon 2020 |
| European Space Agency |
| Canadian Space Agency |
| European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme |
| Marie Sklodovska-Curie |
| Villum Experiment |
| NASA/ESA/CSA James Webb Space Telescope |
| Villum Experiment Grant Cosmic Beacons |
| European Union's Horizon Europe research and innovation programme |
| European Union’s Horizon Europe research and innovation programme |
| Schweizerischer Nationalfonds zur Frderung der Wissenschaftlichen Forschunghttp://dx.doi.org/10.13039/501100001711 |
| SNSF (Swiss National Science Foundation) |
| European Union’s Horizon 2022 research and innovation programme |
| Max Planck Society for support through the Max Planck Fellowship - Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) |
| Agradecimiento |
|---|
| 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's Horizon Europe research and innovation programme under the Marie Sklodovska-Curie grant agreement No 101105725. SS has received funding from the European Union's Horizon 2022 research and innovation programme under the Marie Sk & lstrok;odowska-Curie grant agreement No 101105167 - 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's Excellence Strategy - EXC-2094 - 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). |
| 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). |