{
  "id": "astro-ph/0110099",
  "version": "v2",
  "published": "2001-10-04T15:03:35.000Z",
  "updated": "2001-10-05T00:18:40.000Z",
  "title": "High resolution observations and mass modelling of the CLASS gravitational lens B1152+199",
  "authors": [
    "D. Rusin",
    "M. Norbury",
    "A. D. Biggs",
    "D. R. Marlow",
    "N. J. Jackson",
    "I. W. A. Browne",
    "P. N. Wilkinson",
    "S. T. Myers"
  ],
  "comment": "7 pages, post-referee revision for MNRAS",
  "journal": "Mon.Not.Roy.Astron.Soc. 330 (2002) 205",
  "doi": "10.1046/j.1365-8711.2002.05043.x",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We present a series of high resolution radio and optical observations of the CLASS gravitational lens system B1152+199 obtained with the Multi-Element Radio-Linked Interferometer Network (MERLIN), Very Long Baseline Array (VLBA) and Hubble Space Telescope (HST). Based on the milliarcsecond-scale substructure of the lensed radio components and precise optical astrometry for the lensing galaxy, we construct models for the system and place constraints on the galaxy mass profile. For a single galaxy model with surface mass density Sigma(r) propto r^-beta, we find that 0.95 < beta < 1.21 at 2-sigma confidence. Including a second deflector to represent a possible satellite galaxy of the primary lens leads to slightly steeper mass profiles.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2001-10-05T00:18:40.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "high resolution observations",
      "mass modelling",
      "class gravitational lens system",
      "surface mass density sigma",
      "slightly steeper mass profiles"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 577162
    }
  }
}