2006/06/29 by Brendon J. Brewer, B. J. Brewer, Geraint F. Lewis · 15 citations
Physics and Astronomy · #Adaptive optics and wavefront sensing #Artificial intelligence #Astrophysics #Bayesian inference #Bayesian probability #Computer science #Einstein ring #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gamma-ray bursts and supernovae #Gravitational lens #Lens (geology) #Optics #Physics #Pixel #Redshift #astro-ph
paper · pdf · doi:10.1086/507475
published in The Astrophysical Journal 651(1), 8-13 (IOP Publishing) · Accepted for publication in ApJ
arxiv created 2006/06/29 · openalex publication_date 2006/10/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In a previous paper, we outlined a new Bayesian method for inferring the properties of extended gravitational lenses given data in the form of resolved images. This method holds the most promise for optimally extracting information from the observed image, while providing reliable uncertainties in all parameters. Here, we apply the method to the well studied optical Einstein ring 0047-2808. Our results are in broad agreement with previous studies, showing that the density profile of the lensing galaxy is aligned within a few degrees of the light profile, and suggesting that the source galaxy (at redshift 3.6) is a binary system, although its size is only of order 1-2 kpc. We also find that the mass of the elliptical lensing galaxy enclosed by the image is (2.91 ± 0.01) × 10 11 M ☉ . Our method is able to achieve improved resolution for the source reconstructions, although we also find that some of the uncertainties are greater than has been found in previous analyses, due to the inclusion of extra pixels and a more general lens model.