ARG0003d3f, two compact, NW overedge extended bent emission.
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by ChrisMolloy
Here's ARG0003d3f, what appears to be two separate #compact lobes. I've expanded this image out so that the #overedge lobe mentioned in the ARG comments left to the NW is included. This seems to be an #extended #bent lobe.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread.NED has NVSS references which seem to align near both the #compact lobes, the lobe to the WSW seems to be centred on SDSS J121121.79+062536.7 below, which is listed as a star,
and to the ENE, SDSS J121124.71+062610.4, again a star, which is more NW of this lobe.
Both the #compact lobes appear to be #noir, with no ALLWISE references.
As to whether this could be a #doublelobe with reference to the ARG comments left, in the centre of both lobes is SDSS J121123.22+062542.5, below, which is listed as a star and has an ALLWISE reference, ALLWISE J121123.22+062542.2.
To the SE of SDSS J121123.22+062542.5 is SDSS J121124.78+062531.9, below, a galaxy which has a z_ph=0.312 ± 0.1242. This galaxy has an ALLWISE reference also, ALLWISE J121124.79+062532.1, and does seem to have a #green-outflow to the NE. It does seem unlikely, however, that both these objects are possible hosts of a #doublelobe.
To the NW is what appears to be an #extended #bent lobe. The possible host in the centre of the emission appears to be SDSS J121118.60+062737.4, which has a z_sp=0.436 +/-0.00009, an NVSS reference in NED, and an ALLWISE reference, ALLWISE J121118.59+062737.6. If this is the host of the emission it is an extremely unusual looking galaxy, possibly #disturbed, and seems to have #red-outflows.
This lobe is quite visible in NVSS, below.
Comments, suggestions, welcome.
Posted