2000/08/31 by J. D. Cohn, C. S. Kochanek, B. A. McLeod +2 · 4 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Radio Astronomy Observations and Technology #astro-ph
paper · pdf · doi:10.1086/321412
24 pages, 10 figures, final version to appear in ApJ. Some minor corrections (e.g. constraint on central unseen image was stronger than intended earlier, now agrees with text, conventions on angles fixed in text/plots). Resulting model fits have some change in chi squareds and best parameters (e.g. cores, flatness of rotation curve) have some changes. Properties of model families and trends for best fitting models very close to earlier results; general conclusions the same
arxiv created 2001/02/22 · openalex publication_date 2001/06/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
We consider a wide range of parametric mass models for B1933+503, a 10-image radio lens, and identify shared properties of the models with the best fits. The approximate rotation curves vary by less than 8.5% from the average value between the innermost and the outermost image (1.5-4.1 h -1 kpc) for models within 1 σ of the best fit, and the radial dependence of the shear strength and angle also have common behavior for the best models. The time delay between images 1 and 6, the longest delay between the radio cores, is Δ t = 10.6 h -1 days (Ω 0 = 0.3, λ 0 = 0.7), including all the modeling uncertainties. Deeper infrared observations, to more precisely register the lens galaxy with the radio images and to measure the properties of the Einstein ring image of the radio source's host galaxy, would significantly improve the model constraints and further reduce the uncertainties in the mass distribution and time delay.