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• by meglon978

  3 in one shot. The bigger looks to have a decent spin/wobble going.

  Posted December 21, 2013 1:44 AM

• by JeanTate

  Other than z_ph 0.53 SDSS J003023.85+112112.5 as the likely host for the top (N) doublelobe, it's not clear which AGNs are creating the radio emission:

  

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  Boilerplate: SDSS image per http://skyservice.pha.jhu.edu/DR10/ImgCutout/getjpeg.aspx, FIRST contours derived from FITS files produced using SkyView with Python code described in this RGZ Talk thread. Image center per the ARG image (left; J2000).

  Posted July 1, 2014 11:06 PM