Electronic Telegram No. 3972 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network COMET C/2014 R3 (PANSTARRS) R. Wainscoat reports the discovery of a comet on i-band CCD images obtained with the Pan-STARRS 1.8-m Ritchey-Chretien reflector (discovery observations tabulated below), the object appearing having a slightly extended point-spread function (FWHM = 1".33, vs. about 1" for nearby stars). 2014 UT R.A. (2000) Decl. Mag. Sept. 6.32856 19 30 58.41 +56 02 46.4 20.1 6.34132 19 30 57.80 +56 02 44.0 20.2 6.35409 19 30 57.18 +56 02 41.3 20.0 6.36684 19 30 56.59 +56 02 38.6 20.1 After the object was posted on the Minor Planet Center's PCCP webpage, H. Sato (Tokyo, Japan) found the object to be diffuse with a moderately condensed coma of size 6" and w-band magnitude 20.1 as measured within a circular aperture of radius 3".8 in ten stacked 60-s exposures taken on Sept. 12.2 UT with an iTelescope 0.61-m f/6.5 astrograph (+ luminance filter) located at Auberry, CA, U.S.A. The available astrometry, the following preliminary parabolic orbital elements by G. V. Williams, and an ephemeris appear on MPEC 2014-S05. T = 2016 July 8.0264 TT Peri. = 110.3780 Node = 334.9057 2000.0 q = 7.476449 AU Incl. = 91.1528 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 September 16 (CBET 3972) Daniel W. E. Green