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J1721+8842: The first Einstein zigzag lens

  • F. Dux
  • , M. Millon
  • , C. Lemon
  • , T. Schmidt
  • , F. Courbin
  • , A. J. Shajib
  • , T. Treu
  • , S. Birrer
  • , K. C. Wong
  • , A. Agnello
  • , A. Andrade
  • , A. Galan
  • , J. Hjorth
  • , E. Paic
  • , S. Schuldt
  • , A. Schweinfurth
  • , D. Sluse
  • , A. Smette
  • , S. H. Suyu
  • European Southern Observatory
  • Swiss Federal Institute of Technology Lausanne
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Swiss Federal Institute of Technology Zurich
  • Oskar Klein Centre
  • University of California at Los Angeles
  • University of Barcelona
  • ICREA
  • The University of Chicago
  • The University of Tokyo
  • University of Copenhagen
  • STFC Hartree Centre
  • Universidad Andrés Bello
  • Technical University of Munich
  • Max Planck Institute for Astrophysics
  • University of Milan
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • University of Liege

Research output: Contribution to journalArticlepeer-review

8 Scopus citations

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 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.

Original languageEnglish
Article numberA300
JournalAstronomy and Astrophysics
Volume694
DOIs
StatePublished - Feb 1 2025

Keywords

  • cosmological parameters
  • cosmology: observations
  • dark energy
  • distance scale
  • galaxies: evolution

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