Dear SN watchers, IAUC 8014 informed the spectra of recent two SNe by the UCB team: both spectra were taken on Nov. 9 UT with Keck II 10-m. SN 2002gz: In [vsnet-obs 41955] (Oct. 20): >SN2002gz 20020922.0 <202C PAL >SN2002gz 20021015.49 183C PAL >SN2002gz 20021018.0 182C PAL > ># SN 2002gz (2:34:10.36, -0:53:18.2, J2000.0) is located at about 4" ># east and 1" south of an apparent host dim galaxy. It is indeed a SN with a blue continuum and very broad undulations, but the classification is uncertain. It can be of type IIb because of possible H-alpha emission and He I absorption. The recession velocity is measured as about 25000 km/s. SN 2002ho: In [vsnet-campaign-sn 498] (Nov. 9): >SN2002ho 20020403.0 <185C Bol >SN2002ho 20021105.130 170C Bol >SN2002ho 20021107.528 168C SCH > ># NGC 4210, a host galaxy of SN 2002ho (12:15:17.97 +65:58:55.1 ># (J2000.0), offset = 13"E, 12"S), is a barred-spiral (SB(r)b) galaxy. ># SN is superimposed on the southern arm. Typical SN Ia in this ># galaxy would have a maximum of mag about 14.5, but it seems not the ># case for this SN. It is of type Ic within a few weeks after maximum. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp