We performed some follow-up measurements of this object, while it was still on the neocp. Stacking of 10 R-filtered exposures, 20-sec each, obtained remotely, from the Haleakala-Faulkes Telescope North on 2012, Jan.30.6, through a 2.0-m f/10.0 Ritchey-Chretien + CCD, under good seeing conditions, shows that this object appears "soft", compared to the nearby field stars of similar brightness (stellar FWHM of 1.2").
M.P.E.C. 2012-C23 assignes the following preliminary parabolic orbital elements to comet C/2012 B3: T 2011 Nov. 29.91; e= 1.00; Peri. = 49.22; q = 3.52 AU; Incl.= 106.85
by G. Sostero, K. Rochowicz, E. Guido, N. Howes & A. Tripp