Dear SN watchers, IAUC 8013 informed classifications of three recent SNe. SN 2002gx: In [vsnet-obs 41955] (Oct. 20): >SN2002gx 20011223.0 <202C PAL >SN2002gx 20021013.41 190C PAL >SN2002gx 20021016.0 192C PAL > ># SN 2002gx (2:31:44.69, +40:16:39.5, J2000.0) is located about 6" ># east and 7" south of an apparent host anonymous galaxy (GSC2.2.1 red ># mag = 17.07). The UCB team (with Keck I 10-m) has revealed that it is SN Ia about 2 months after maximum on Nov. 8. The recession velocity of the host galaxy is about 24000 km/s. SN 2002hu: In [vsnet-campaign-sn 498]: >SN2002hu 20021004.0 <185C Bol >SN2002hu 20021107.09 170C Bol > ># MCG +06-6-12 = KUG 0215+372, a host galaxy of SN 2002hu (2:18:20.06, ># +37:27:58.8 (J2000.0), offset = 21"E, 7"N), is a small spiral galaxy ># with ultraviolet excess. The CfA team (with Mt. Hopkins 1.5-m on Nov. 8.80) and the UCB team (with Keck I 10-m on Nov. 9) revealed that it is of SN Ia a fer days before maximum. The recession velocity of the host galay is about 11000 km/s, so the discovery magnitude is roughly consistent with the expected maximum brightness. SN 2002hv: In [vsnet-campaign-sn 498]: >SN2002hv 20020428.2 <190:C KAI >SN2002hv 20021105.5 186C SCH >SN2002hv 20021107.5 189:C SCH > ># UGC 4974, a host galaxy of SN 2002hv (9:22:10.91, +33:50:10.8 ># (J2000.0), offset = 7"E, 43"S), is a lenticular (S0:) galaxy making ># a pair with KUG 0919+340. Such early (E-S0) galaxies produce SN Ia ># only, whose expected maximum is mag about 16.5. It is probably old ># SN Ia. The CfA team and the UCB team (with the same instruments as SN 2002hu) revealed that it is SN Ia some weeks after maximum. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp