Substructure in the lens HE 0435-1223

Ross Fadely, Charles R. Keeton

Research output: Contribution to journalArticlepeer-review

53 Scopus citations

Abstract

We investigate the properties of dark matter substructure in the gravitational lens HE 0435-1223 (zl=0.455) via its effects on the positions and flux ratios of the quadruply imaged background quasar (zs= 1.689). We start with a smooth mass model, add individual, truncated isothermal clumps near the lensed images and use the Bayesian evidence to compare the quality of different models. Compared with smooth models, models with at least one clump near image A are strongly favoured. The mass of this clump within its Einstein radius is log10(MAEin) = 7.65+0.87- 0.84 (in units of h-170M). The Bayesian evidence provides weaker support for a second clump near image B, with log10(MBEin) = 6.55+1.01- 1.51. We also examine models with a full population of substructure, and find the mass fraction in substructure at the Einstein radius to be fsub>rsim 0.00077, assuming the total clump masses follow a mass function dN/dM∝M-1.9 over the range M= 107-1010M. Few-clump and population models produce similar Bayesian evidence values, so neither type of model is objectively favoured.

Original languageEnglish (US)
Pages (from-to)936-951
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume419
Issue number2
DOIs
StatePublished - Jan 2012

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Dark matter
  • Galaxies: haloes
  • Gravitational lensing: strong
  • Methods: statistical

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