Image Details

Choose export citation format:

SDSS J024634.11−082536.2: A New Gravitationally Lensed Quasar from the Sloan Digital Sky Survey

  • Authors: Naohisa Inada, Scott Burles, Michael D. Gregg, Robert H. Becker, Paul L. Schechter, Daniel J. Eisenstein, Masamune Oguri, Francisco J. Castander, Patrick B. Hall, David E. Johnston, Bartosz Pindor, Gordon T. Richards, Donald P. Schneider, Richard L. White, J. Brinkmann, Alexander S. Szalay, and Donald G. York

Inada et al. 2005 The Astronomical Journal 130 1967.

  • Provider: AAS Journals

Caption: Fig. 12.

Comparison of the "ring" with the critical curve of the best‐fit model. The solid line represents the critical curve predicted by the two SIS lens model with ﹩\alpha _{\mathrm{E}\,}( \mathrm{G}\,\prime ) =0\farcs 07﹩. The deep gray squares represent the pixels with higher count rate, after subtracting the central lensing galaxy and excluding the pixels around components A and B. The red dot‐dashed line connects the pixels that have the maximum count rate in each column. The ring is in good agreement with the critical curve; this fact supports the idea that the ring is the lensed host galaxy of the source quasar.

Other Images in This Article

Show More

Copyright and Terms & Conditions