ARG00034ii, doublelobe, SDRAGN candidate?
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by ChrisMolloy
Here's ARG00034ii, which appears to be a #doublelobe.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread.The host for the the emission appears to be SDSS J005027.57+092719.9, which has a z_ph=0.457 ± 0.0996, an NVSS reference in NED, and an ALLWISE reference, ALLWISE J005027.61+092719.7.
This galaxy is relatively faint, so as to whether this is an #SDRAGN candidate is hard to tell. For what it's worth, the galaxy has a fracDev_g, _r, of 0.168 and 0, and an expAB_g of 0.232 and expAB_r of 0.201 respectively. For c, the inverse concentration index, it has a figure of 0.320 for the g band and 0.516 for the r band.
Interestingly, there also appears to be an NVSS reference in NED for SDSS J005027.99+092717.4, which has a z_ph=0.468 ± 0.0895, and there is an ALLWISE reference ~6.5" ENE of SDSS J005027.57+092719.9, ALLWISE J005028.04+092722.3.
As always, comments, suggestions, welcome.
Posted