ARG00033ay - is the host a spiral?
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by JeanTate
SDSS J111049.36+095307.1, with a z_ph of 0.637±0.2009/0.378±0.2802 - which is, in plain English, "really have no clue" - is the likely host of the somewhat faint doublelobe radio structure. Is it a spiral?
Probably too faint to tell, really. But is it the likely host? And is the radio structure really a doublelobe?
Boilerplate: SDSS image per
http://skyservice.pha.jhu.edu/DR10/ImgCutout/getjpeg.aspx
, FIRST (red) contours derived from the FITS file produced using SkyView with Python code described in this RGZ Talk thread. Image center (J2000.0) is the galaxy SDSS J111049.36+095307.1; "z_ph" its SDSS photometric redshift.Posted