Bingxiao Xu, Marc Postman, Massimo Meneghetti, Stella Seitz, Adi Zitrin, Julian Merten, Dani Maoz, Brenda Frye, Keiichi Umetsu, Wei Zheng, Larry Bradley, Jesus Vega, Anton Koekemoer

Research output: Contribution to journalArticlepeer-review


We developed an algorithm to find and characterize gravitationally lensed galaxies (arcs) to perform a comparison of the observed and simulated arc abundance. Observations are from the Cluster Lensing And Supernova survey with Hubble (CLASH). Simulated CLASH images are created using the MOKA package and also clusters selected from the high-resolution, hydrodynamical simulations, MUSIC, over the same mass and redshift range as the CLASH sample. The algorithm's arc elongation accuracy, completeness, and false positive rate are determined and used to compute an estimate of the true arc abundance. We derive a lensing efficiency of 4 ±1 arcs (with length ≥6″ and length-to-width ratio ≥7) per cluster for the X-ray-selected CLASH sample, 4 ±1 arcs per cluster for the MOKA-simulated sample, and 3 ±1 arcs per cluster for the MUSIC-simulated sample. The observed and simulated arc statistics are in full agreement. We measure the photometric redshifts of all detected arcs and find a median redshift zs = 1.9 with 33% of the detected arcs having zs>3. We find that the arc abundance does not depend strongly on the source redshift distribution but is sensitive to the mass distribution of the dark matter halos (e.g., the c-M relation). Our results show that consistency between the observed and simulated distributions of lensed arc sizes and axial ratios can be achieved by using cluster-lensing simulations that are carefully matched to the selection criteria used in the observations.

Original languageAmerican English
Article number85
JournalAstrophysical Journal
Issue number2
StatePublished - 1 Feb 2016


  • galaxies: clusters: general
  • gravitational lensing: strong
  • methods: Observational
  • methods: numerical
  • methods: statistical

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


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