[LTS2006] J071317.37-514154.0 , the SIMBAD biblio

Two apparent supernovae have been reported: 2006Y by P. Luckas, O. Trondal, and M. Schwartz (cf. IAUC 8655; unfiltered CCD frames, 0.35-m Tenagra telescope at Perth) and 2006Z by the SDSS collaboration (found in spectra; communicated by M. SubbaRao, University of Chicago and Adler Planetarium; cf. IAUC 8513; r-band magnitude given below). SN 2006 UT R.A. (2000.0) Decl. Mag. Offset 2006Y Feb. 3.58 7 13 17.19 -51 41 18.8 17.7 1".7 W, 5".2 N 2006Z Feb. 1.51 13 44 58.07 +26 18 25.7 20.4 – Additional unfiltered magnitudes of 2006Y: Jan. 27.59 UT, [18.5; Feb. 7.60, 17.3. SN 2006Z, which appears to be a type-Ia supernova with an age of approximately -7 ± 4 days after maximum light, is coincident with the center of the host galaxy (r = 17.0 from an image taken on 2004 June 12; z = 0.1232).