Dear SN watchers, IAUC 7566 informed that KAIT discovered an bright SN Ia. It can have a broad maximum, which indicate it would be an overluminous SN Ia. The discovery made by the image taken on Jan 18.4 UT when the new object was mag about 15.4. It was confirmed on an earlier image taken on 2000 Dec. 31.4, when it was mag about 15.7. The location is: R.A. = 11h36m48s.83, Decl. = -8 35'07".0 (equinox 2000.0), which is about 4" north of the nucleus of nearly edge-on spiral (SAb: sp) galaxy MCG -01-30-11. It is almost overimposed on the bulge region. The spectrum has taken by CfA team on Jan 19.46 UT, which reveals that SN 2000L is SN Ia about 1 week after maximum. The recession velocity of the host galaxy (4567 km/s) suggest that the typical SN Ia would have the maximum brightness of mag 15.7. Reported magnitude is somewhat brighter, and the peak of the light curve seems to be broader than the typical one. So, it can be an overluminous SN Ia like SN 1991T. The follow-up photometry of this bright example is very important for the confirmation of "bright SN Ia will decline slowly" relation. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp