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J1721+8842: The first Einstein zigzag lens
Indexado
WoS WOS:001426864800007
Scopus SCOPUS_ID:85219586477
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


Abstract



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.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



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

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Financiamiento



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)

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



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).

Muestra la fuente de financiamiento declarada en la publicación.