Dear SN watchers, IAUC 8023 informed the types of recent two SNe determined by the CfA team. SN 2002je: In [vsnet-obs 42363] (Nov. 22): >SN2002je 20021031.2 <190:C KAI >SN2002je 20021120.2 177:C KAI >SN2002je 20021121.1 175:C KAI > ># LEDA 212525 = 2MASXi J0027225+241055, a host galaxy of SN 2002je ># (0:27:22.42, +24:10:59.1 (J2000.0), offset = 2"W, 3"N), is a dim ># galaxy probably a companion of UGC 261. If it is the case, the ># expected maximum for typical SN Ia is mag about 16.7. It is type II SN near the maximum on Nov. 28. SN 2002jg: In [vsnet-obs 42396] (Nov. 25) >SN2002jg 20021118.2 <195:C KAI >SN2002jg 20021123.2 170:C KAI >SN2002jg 20021124.1 168:C SCH >SN2002jg 20021124.2 168:C KAI >SN2002jg 20021125.2 166:C KAI > ># NGC 7253 = Arp 278, a host galaxy of SN 2002jg (22:19:28.80, ># +29:23:04.5 (J2000.0)), is an interacting triple galaxies. A offset ># of SN 2002jg from the brightest nucleus of the southeastern galaxy ># (NGC 7253B = UGC 11985 = MCG +05-52-011) is 20"W and 13"S. There ># are several foreground stars and H II regions within the host, so be ># careful in the identification. The expected maximum for typical SN ># Ia is mag about 15.8, unless it would be reddened by the ># interstellar matter in the host galaxy. It is type Ia SN at the maximum light on Nov. 28, with a notable reddening. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp