2006IAUC.8697....2H

Four additional apparent supernova have been reported from unfiltered CCD images: 2006bg and 2006bi by R. Holmes, Charleston, IL (cf. IAUC 8677; 2006bg with V. Hoette, and 2006bi with H. Devore and P. Miller); 2006bh by L. A. G. Monard (cf. IAUC 8693); and 2006bj by R. Quimby (cf. IAUC 8680). SN 2006 UT R.A. (2000.0) Decl. Mag. Offset 2006bg Mar. 27.28 11 35 25.17 +54 57 37.4 18.4 16".5 W, 2".3 N 2006bh Apr. 2.12 22 40 16.10 -66 29 06.3 14.8 48" W, 22" S 2006bi Mar. 25.39 13 59 11.52 +27 52 17.5 18.1 0".2 W, 2".6 N 2006bj Mar. 26.19 12 22 19.16 + 7 37 25.3 17.3 1".1 E, 1".1 N Additional approximate magnitudes for 2006bg: 1993 Apr. 25, [21.0 (Palomar Sky Survey, red); 2006 Jan. 26.38 UT, [20.4 (Holmes); Apr. 2.18, 18.3 (Holmes). Additional magnitudes for 2006bh in NGC 7329: Jan. 17.751, [17.5; Apr. 3.086, 14.6 ± 0.1. Nothing is visible at the location of 2006bh on the Digitized Sky Survey (limiting red mag 20.5). Additional magnitudes for 2006bi: 1996 July 8, [21.0 (PSS, red); 2006 Feb. 19 and 24, [20.2 (Holmes); Mar. 27.31, 18.2 (Holmes). Additional approximate magnitudes for 2006bj: 2005 May 9, [19.0; 2006 Apr. 2.17, 17.2. A spectrum of 2006bj taken on Mar. 3.34 by S. C. Odewahn and F. Deglman shows it to be a young type-II supernova (details on CBET 460).