SIMBAD references

Seven new apparent supernovae found on unfiltered CCD frames have been reported: 2006cl and 2006cn by the 'Nearby Supernova Factory' collaboration (cf. CBETs 520, 522); 2006cm and 2006cq by T. Puckett (with A. Langoussis for 2006cm, and with J. Newton and E. Briggs for 2006cq); 2006co by C. Colesanti, C. Jacques, E. Pimentel, and T. Napoleao (cf. IAUC 8658); 2006cp by H. Khandrika and W. Li (LOSS/KAIT; cf. IAUC 8710); and 2006cr by T. Boles (cf. IAUC 8699). SN 2006 UT R.A. (2000.0) Decl. Mag. Offset 2006cl May 20.4 16 19 48.80 -10 03 25.2 19.2 – 2006cm May 24.37 21 20 17.46 - 1 41 02.7 16.6 2".0 W, 1".0 N 2006cn May 25.2 13 21 49.14 -23 51 04.6 19.0 – 2006co May 27.10 12 52 40.93 -39 01 48.9 16.0 24".4 E, 7".7 S 2006cp May 28.23 12 19 14.89 +22 25 38.2 18.2 19".9 E, 15".3 S 2006cq May 29.18 13 24 25.10 +30 57 22.7 17.3 4".9 W, 10".3 S 2006cr May 29.95 13 07 12.51 +58 08 06.1 18.1 8".6 W Spectra show that 2006cl, 2006cn, and 2006co are type-II supernovae (details on CBETs 520, 522, and 529). Additional magnitudes for 2006cm in UGC 11723: 2005 Nov. 25, [19.3; 2006 May 25.37 UT, 16.4. A spectrum of 2006cm taken on May 29.47 showed it to be a reddened type-Ia supernova near maximum (details on CBET 526). Additional magnitudes for 2006co in ESO 323-G25: May 4.06, [18.5; 27.89, 15.9. Nothing was visible at the location of 2006co on a red Digitized Sky Survey (DSS) image from 1994. Additional magnitudes for 2006cp in UGC 7357: May 16.24, [19.0; 29.20, 17.8. A spectrum of 2006cp taken on May 30.26 showed it to be a type-Ia supernova around 1 week before maximum (details on CBET 528). Additional magnitudes for 2006cq in IC 4239: Jan. 20, [19.5 (Puckett); May 30.22, 17.3 (A. Sehgal, 0.50-m reflector, Osoyoos, BC). A spectrum of 2006cq obtained on May 31 showed it to be a type-Ia supernova close to maximum brightness (details on CBET 529). Additional magnitudes for 2006cr in UGC 8205: 1995 Apr. 23, [21.0 (DSS blue); 1997 June 25, [20.5 (DSS red); 2006 Apr. 5 and May 15, [19.5 (Boles). A spectrum of 2006cr taken on June 1 shows it to be a type-II supernova about 1 week past explosion (details on CBET 531).