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Hi Scott et al.,
This is my first mail in this group, so I hope it works right away. :-) Scott, we seem to have very similar observing projects!
Indeed, the definition of a quasar seems to be subjective. Physically, they are very luminous examples of Seyfert galaxies, but the question is where to draw the limit between a quasar and an "ordinary" Seyfert galaxy.
In this catalog there is a list of quasars: https://ui.adsabs.harvard.edu/abs/2010A&A...518A..10V/abstract
They define a quasar as a starlike object or object with a starlike nucleus with broad emission lines that is brighter than -22.25 Mag absolute blue magnitude.
Interestingly, many objects listed in this catalog don't fulfill their magnitude criterion based on Simbad data, although they referenced Simbad data in their catalog.
Within the last couple of years I observed some of those objects. At least I Zw 1 (PGC 3151) and VII Zw 118 = PGC 20174 fulfill their criterion. With my 20" Dobsonian I was able to discern non-stellar galaxy bodies from their stellar cores when observing them.
At Deep Sky Meting in March 2026 in southern Germany I will give
a presentation on this topic. So for readers who will attend
(there certainly are a few...) I will discuss this quasar catalog
and observations I did based on this source.
Clear skies,
Robin