ARG0001c1m, multiple emissions and hosts
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by ChrisMolloy
Here's ARG0001c1m, which has a number of emissions, including a possible #triple and #doublelobe, and a couple of #compact lobes.
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread. First in red.The host for the centre emission, which appears to be a #triple, seems to be SDSS J124826.97+364335.2. This galaxy has a z_ph=0.601 ± 0.0556, and radio references in NED and SIMBAD. Regarding the latter references, these are centred on different parts of the emission. This galaxy also has an ALLWISE reference, ALLWISE J124826.99+364335.1.
SW of the centre #triple there is a #diffuse #compact lobe which is positioned on SDSS J124825.96+364318.3. This object has a z_ph=0.693 ± 0.0454, recorded First flux emission, and radio references in NED and SIMBAD, with the latter reference positioned slightly west of the galaxy. There is also an ALLWISE reference, ALLWISE J124825.98+364318.3.
Further SW there is a lobe which could be related to either SDSS J124825.96+364318.3 or SDSS J124826.97+364335.2. This emission is #no-optical, #noir, although in the First contour overlay above, this lobe does seem related to either of these hosts and their emissions.
Furtherest south is a #compact lobe. There is a radio reference in NED for SDSS J124827.73+364248.2, which is listed as a star, and is east of this emission. However, there is a SIMBAD reference, which is positioned in the centre of the lobe, and an ALLWISE reference slightly west of the centre of the lobe, ALLWISE J124827.04+364243.3.
Centre west and WNW (especially in VLASS), there is an emission which could be a #bent or #s-shaped, #doublelobe. A host could be SDSS J124821.80+364336.2, which has a z_sp=0.606 +/-0.00012. This object has radio references in NED and SIMBAD and an ALLWISE reference, ALLWISE J124821.71+364336.5. Regarding the SIMBAD reference, this is slightly WSW of the galaxy.
Here's a VLASS contour overlay of the ARG field. The contours, especially the #diffuse #compact SW of the central emission, and possible #doublelobe to the WNW, seem to be more defined,
The contour overlay image in this post was created from sources, and using methods, described in this RGZ Talk
thread. VLASS contours in yellow.As always, comments, suggestions, welcome.
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by JeanTate
Very nice! 😃
The main source, which seems to be the NE lobe of the main host, would also be an #overlap ... a separate host ~in the center (dimple in VLASS contours ~encloses this), which may be a #triple.
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