ARG0001xv8 - SDRAGN?
-
by Dolorous_Edd
What sort of morphology it is?
Usually ETGs are pretty straightforward
Posted
-
by JeanTate in response to Dolorous Edd's comment.
It's a 'not boring elliptical', so by my definition it is definitely an #SDRAGN candidate! 😃
Very nice find, well done!!
Posted
-
by ivywong scientist, admin
I think this requires an overlay for further clarification.
Posted
-
by Dolorous_Edd
FIRST (red) / NVSS (blue)
IMO SDSS J172107.89+262432.1 is clearly the host
But really what sort of morphology it is? disturbed ETG?
Posted
-
by JeanTate in response to Dolorous Edd's comment.
What sort of morphology it is?
Meert+(2015) is "a catalogue of 2D, point spread function-corrected de Vacouleurs, Sérsic, de Vacouleurs+Exponential, and Sérsic+Exponential fits of ˜7 × 105 spectroscopically selected galaxies drawn from the Sloan Digital Sky Survey (SDSS) Data Release 7."
This strange galaxy (ID# 119607 in their catalog) is one of those ~700k which they modeled. The 'elliptical/spiral/uncertain' flag is 'uncertain'. The estimated 'bulge/total' ratio is 0.41, quite typical for an early spiral. Their program had a tough time modelling the bulge: the estimated radius is 4.45±3.42", and the Sérsic index 8 (i.e. very extended). However, it's very close to 'spherical' (the b/a ratio is 0.97±0.04). The disk - modeled as an exponential - has an estimated radius of 5.02±0.15", with a b/a ratio of 0.63±0.02.
In short, it seems to be a disk galaxy with a large, somewhat unusual, bulge. So, one of the best SDRAGN candidates to date! 😃 Great discovery!! 😃 😃
Posted
-
by JeanTate
I started a thread on this - and one other object - over in GZ Talk, From RGZ, question about the morphology of two SDSS objects. It will be interesting to see what comments zooites there post ...
Posted
-
by Dolorous_Edd
Just FYI the area around SDSS J172107.89+262432.1 ( and even SDSS J172107.89+262432.1 itself ) seems to be imaged by Subaru telescope
Posted
-
by Dolorous_Edd
Here is an example of image cutout from Subaru
Link to download fits file ~49Mb
I hope you will have much more luck with it than I ( it does have SDSS J172107.89+262432.1 in FOV )
Posted
-
by Dolorous_Edd
As seen by Subaru
IMO doubtful improvement
Posted
-
by JeanTate in response to Dolorous Edd's comment.
Wow!
IMO doubtful improvement
IMO a big improvement ... to me it's clear this is a disturbed, early-type, spiral, possibly a merger.
Posted
-
by ivywong scientist, admin
Interesting, it's starting to look like an early-type that has ripped apart its companion galaxy into a stream so really, a merger system rather than spiral arms. I reckon that if one were to fit the galaxy with a elliptical galaxy's Sersic profile and subtract from the above Subaru image, you might find that it will fully take out the core of this galaxy.....
Posted
-
by Dolorous_Edd
cubehelix
inverted greyscale
HTH
Posted