Dear SN watchers, In addition of two discovery, IAUC 8031 informed the spectroscopic classifications of two recent SNe by the UCB team. SN 2002jj: In [vsnet-campaign-sn 513] (Dec. 5): >SN2002jj 20020814.5 <190:C KAI >SN2002jj 20021001.4 <180:C KAI >SN2002jj 20021024.4 165:C KAI >SN2002jj 20021103.4 165:C KAI >SN2002jj 20021203.4 165:C KAI > ># IC 340, a host galaxy of SN 2002jj (3:39:29:55, -13:06:55.8 ># (J2000.0), offset = 7"E, 2"S), is a lenticular (S0^0^:) galaxy. ># There is a bright (mag about 14) foreground star about 15" east of ># the nucleus of IC 340. SN is located between the nucleus and this ># foreground star. The KAIT discovery image can be seen at: ># http://astron.berkeley.edu/~bait/2002/sn2002jj.gif . The expected ># maximum for typical SN Ia is mag about 15.6. ># ># Lenticular galaxies are believed to produce SNe Ia only. On the ># other hand, the reported magnitudes suggest that it does not like SN ># Ia but it can be of type IIP in the plateau phase, though it seems ># somewhat brighter than typical SNe II. It is urged to determine ># whether it is genuine SN. This SN was turned out to be a type Ic SN, about one month after maximum on Dec. 12. Such a slow evolution of the light curve is quite exceptional for type Ic SN. The follow-up magnitude estimates is very urged. SN 2002jm: In [vsnet-campaign-sn 517] (Dec. 11): >SN2002jm 20021123.5 <185:C KAI >SN2002jm 20021207.5 175:C KAI >SN2002jm 20021209.5 175:C SCH > ># IC 603, a host galaxy of SN 2002jm (10:19:25.20, -5:39:14.5 ># (J2000.0), offset = 3"E, 7"N), is a disk ((R)SB(r)A:) galaxy. The ># SN is superimposed on the bright bulge region. The expected maximum ># for typical unreddened SN Ia is mag about 16.1, which seems not the ># case. It seems to be a subluminous SN Ia about 3 weeks after maximum. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp