Journal Article

Substructure in the lens HE 0435−1223

Ross Fadely and Charles R. Keeton

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 419, issue 2, pages 936-951
Published in print January 2012 | ISSN: 0035-8711
Published online December 2011 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2011.19729.x
Substructure in the lens HE 0435−1223

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics

GO

Show Summary Details

Preview

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−170 M). 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 0.000 77, assuming the total clump masses follow a mass function dN/dMM−1.9 over the range M= 107–1010 M. Few-clump and population models produce similar Bayesian evidence values, so neither type of model is objectively favoured.

Keywords: gravitational lensing: strong; methods: statistical; galaxies: haloes; dark matter

Journal Article.  11755 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.