ARG0001g1q - disk host?
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by JeanTate
SDSS J152955.47+344955.2, z_ph 0.308±0.0953/0.184±0.0921 (rather uncertain, eh?), certainly looks like a classic Eos (edge-on spiral)*
But is it the host of the strong doublelobe radio emission?
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 [); "z_ph" its SDSS photometric redshift.*what's the wispy red stuff?
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