2006IAUC.8770....1P

Further to IAUC 8766, seven apparent supernovae have been reported from unfiltered CCD images: 2006le, 2006lf, 2006lg, 2006li, and 2006lu by R. R. Prasad, N. Joubert, M. Baek, and W. Li (LOSS/KAIT); and 2006lh and 2006lt by the "Nearby Supernova Factory" collaboration (details on CBETs 708 and 714). SN 2006 UT R.A. (2000.0) Decl. Mag. Offset 2006le Oct. 26.44 5 00 41.99 +62 15 19.0 18.0 12".4 W, 40".1 N 2006lf Oct. 26.43 4 38 29.49 +44 02 01.5 18.0 13".0 E, 12".1 S 2006lg Oct. 25.38 2 46 57.64 +39 00 40.0 18.8 0".6 W, 4".8 S 2006lh Oct. 24.2 23 26 51.60 + 9 19 57.6 19.4 – 2006li Oct. 28.49 7 05 33.33 +33 50 01.3 19.4 3".3 W, 20".4 N 2006lt Oct. 11.4 2 16 59.89 +30 41 57.4 19.1 – 2006lu Oct. 30.55 9 15 17.63 -25 36 00.3 17.6 6".0 E, 0".5 S Additional KAIT magnitudes for 2006le in UGC 3218: Oct. 19.44 UT, [19.1; 25.45, 18.5; 27.51, 17.6. SN 2006le is a type-Ia supernova, well before maximum light on Oct. 27 (details on CBET 702). Additional KAIT magnitudes for 2006lf in UGC 3108: Oct. 19.43, [19.3; 27.51, 17.6. SN 2006lf is a type-Ia supernova, around 1 week before maximum light on Oct. 28 (details on CBET 705). Additional KAIT magnitudes for 2006lg in UGC 2243: Oct. 1.38, [19.0; 26.36, 18.4; 28.34, 18.5. SN 2006lg is a type-II supernova (details on CBET 707). A spectrogram obtained on Oct. 28 showed 2006lh to be a young type-II supernova (details on CBET 708). Additional magnitudes for 2006li in UGC 3664: 1989 Oct. 28, [21.0 (Digitized Sky Survey red plate); 2003 Oct. 22.52, 19.8 (KAIT); 2006 Oct. 29.52, 19.4 (KAIT). A spectrogram obtained on Oct. 13 suggests that 2006lt was then already a late type-Ib supernova. Additional magnitudes for 2006lu: May 4.12, [18.8 (KAIT); Nov. 1.35, r = 17.51 ± 0.03 (W. Krzeminsky and C. Contreras, on behalf of the Carnegie Supernova Project; Las Campanas Observatory 1-m Swope telescope).