Dear SN watchers, IAUC 7920-22 reported some spectra of recent SNe. SN 2002di: In [vsnet-obs 40219]: ># The host galaxy of SN 2002di is MCG +05-40-2, which is a distant ># interacting galaxy. The expected maximum for typical SN Ia is mag ># about 17.6. It is of peculiar (subluminous) SN Ia, roughly 1 week after maximum on June 17 (the UCB team, IAUC 7920). SN 2002dk: In [vsnet-obs 40238]: ># NGC 6616 = the host galaxy of SN 2002dk is a spiral (Sab) galaxy ># somewhat near to the Galactic plane (b = 17o). The position is: ># R.A. = 18h17m43s.52, Decl. = +22o14'53".4 (2000.0), which is about ># 34" east and 35" north of the nucleus of NGC 6616. The expected ># maximum for typical SN Ia is mag about 16.5. It is also of peculiar SN Ia near maximum on June 17 (ibid). SN 2002dg: In [vsnet-campaign-sn 434]: ># This SN was discovered during the course of the NEAT survey. The ># apparent host galaxy is quite dim and unnamed. The Padova team took a spectrum of SN 2002dg with ESO NTT at La silla on June 15.13, which reveals that it is type Ib SN, 2-3 weeks after maximum. The recession velocity of the host galaxy is measured as 14000 km/s. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp