Electronic Telegram No. 3659 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 COMETS C/2012 V2 (LINEAR) AND C/2013 R1 (LOVEJOY) C. Opitom, E. Jehin, J. Manfroid, and M. Gillon, Liege University, report that they obtained narrowband photometry on Sept. 11 and 12 with the robotic TRAPPIST 0.6-m telescope at the European Southern Observatory of comets C/2012 V2 and C/2013 R1. Both comets display gaseous comae and are now visible in the morning sky from the southern hemisphere. The following production rates (Haser model with Vp = Vd = 1 km/s) were obtained for C/2012 V2 (when r = 1.50 AU, post-perihelion): log Q(OH) = 28.4; log Q(NH) = 26.4; log Q(CN) = 25.9; log Q(C_3) = 25.6; log Q(C_2) = 26.2; and Af(rho) at 526.0 nm = 2600 cm at 10000 km. A set of narrowband photometry was also collected on the new comet C/2013 R1 (when r = 1.94 AU, pre-perihelion), resulting in the following production rates: log Q(OH) = 27.9; log Q(CN) = 25.5; log Q(C_3) = 24.9; log Q(C_2) = 25.5; and Af(rho) at 526.0 nm = 160 cm. These values indicate that both comets have "typical" composition and that C/2013 R1 has a low dust-to-gas ratio. Visual total-magnitude and coma-diameter estimates for comet C/2012 V2: Aug. 9.82 UT, 8.9, 3' (M. Mattiazzo, Swan Hill, Vic., Australia, 25x100 binoculars); 12.80, 8.6, 4' (D. A. J. Seargent, The Entrance, NSW, Australia, 25x100 binoculars); 23.35, 8.7, 3' (W. Souza, Sao Paulo, Brazil, 0.10-m refractor); 29.35, 9.2, 4' (A. Amorim, Florianopolis, Brazil, 0.18-m reflector); Sept. 4.77, 8.9, 3' (Seargent); 27.32, 9.1, 2' (Amorim). K. Yoshimoto, Yamaguchi, Japan, reports total CCD mag 13.3 and coma diameter 1'.2 for comet C/2013 R1 on Sept. 19.79 UT. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2013 CBAT 2013 September 29 (CBET 3659) Daniel W. E. Green