ARG0003gq3, SDRAGN candidate?
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by ChrisMolloy
Here's ARG0003gq3, possibly a #doublelobe, #SDRAGN candidate.
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 is SDSS J144528.33+051459.6, which appears to be a faint, #clumpy, #green, galaxy, and which NED lists as having a redshift of z_sp=0.895880 +/- 0.000300. There are PMN and NVSS radio references in NED for this galaxy, and there is an ALLWISE reference, ALLWISE J144528.32+051459.5.
As per the classification comments left, this could be an #SDRAGN candidate, but the galaxy is very faint. It has a fracDev_g, _r, of 0, and 1, and an expAB_g of 0.508 and expAB_r of 0.499 respectively. For c, the inverse concentration index, it has a figure of 0.455 for the g band and 0.326 for the r band. On the above parameters, it could possibly be an #SDRAGN candidate, or more likely, a #disk galaxy.
As always, comments, suggestions, welcome.
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by ivywong scientist, admin
maybe I have terrible eyesight but I really cannot tell that this fuzzy galaxy is a spiral...
Posted
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by ChrisMolloy in response to ivywong's comment.
Agree. Very faint, and does appear clumpy.
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