He described that the comet showed a 5″ tail in PA 270°, and its FWHM was 6.4″ larger than stars nearby.
Its cometary nature was confirmed by other CCD astrometrists, including us.
The discovery was announced on Jan. 17 on IAUC 9193 (subscription required), and the astrometry appeared on MPEC 2011-B07, together with a very preliminary parabolic orbital elements (perihelion around 2011, Oct. 4).
The image above was taken on 2011, Jan. 16.22, in the last part of the night, after some passing high clouds and after the Moonset. Seeing and transparency were good.