Dear SN watchers, The Cfa team has taken spectra of recent two SNe, which can be seen at: http://cfa-www.harvard.edu/cfa/oir/Research/supernova/RecentSN.html . SN 2002es: In [vsnet-campaign-sn 466] (Aug. 27): >SN2002es 20020215.2 <190:C KAI >SN2002es 20020812.5 185:C KAI >SN2002es 20020823.5 164:C KAI >SN2002es 20020824.5 163:C KAI > ># UGC 2708, the host galaxy of SN 2002es (offset 19"W, 25"N), is a ># lenticular (S0) galaxy, which produce SN Ia only. The reported ># magnitude is consistent with the expected maximum for typical SN Ia. It is a peculiar (subluminous) type Ia SN near maximum on Sept. 3 UT. SN 2002eu: In [vsnet-obs 41120] (Sept. 1): >SN2002eu 20020820.4 <190:C KAI >SN2002eu 20020825.4 188:C KAI >SN2002eu 20020830.4 174:C KAI > ># The host galaxy of SN 2002eu is LEDA 212843 = 2MASXi J0149427+323730. ># The recession velocity of the host galaxy is 11280 km/s, so the ># discovery magniture (174:C) is consistent to the expected maximum ># for typical SN Ia. It is type Ia SN several days after maximum on Sept. 3 UT. The recession velocity is roughly estimated to be about 10000 km/s. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp