ARG0003k0q - a very strong radio source; host is not a boring elliptical (and may be green)
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by JeanTate
SDSS J231635.19+040518.3, a z_ph 0.195±0.0256/0.161±0.0604, um, object, is likely a merger (it may be a post-quenched/E+A galaxy, but without a spectrum we can't tell):
Question: does the radio emission extend well beyond the optical boundary, perhaps as nascent #nat or #wat? Or is it all artifacts?
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 J231635.19+040518.3; "z_ph" its SDSS photometric redshift.Posted