ARG0002i2c possibly fading, asymmetrical doublelobe, SDRAGN candidate?
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by ChrisMolloy
Here we have ARG0002i2c, which appears to be a possibly #fading, #asymmetrical, #doublelobe.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread.The host for this emission seems to be SDSS J154220.23+173754.0, a very red galaxy, which has a z_ph=0.656 ± 0.0634. In terms of radio references, there is an NVSS reference in NED, and an ALLWISE reference, ALLWISE J154220.23+173754.2. Furthermore, this emission is cited on page 6 of the How to describe the radio morphology? thread, with the following observation:
Can the morphology of the radio emission be described as #fading?
And here's the First cutout.
As per the classification comments left, and whether this galaxy is an #SDRAGN candidate, it has a fracDev_g, _r, of 0, and 0.839, and an expAB_g of 0.05 and expAB_r of 0.750 respectively. For c, the inverse concentration index, it has a figure of 0.492 for the g band and 0.478 for the r band. On the above parameters, it could be, but it is a very faint galaxy, so hard to say.
Here's a zoomed in image without the gridlines.
Comments, suggestions, welcome.
Posted