Dear SN watchers, In [vsnet-alert 7494]: > The reported magnitudes suggest that it is in a rising phase. >Typical SN Ia at maximum would be mag about 14.1 for this galaxy. >Follow-up photometry and spectroscopic classification is urged. Spectroscopy at Bisei confirmed that SN 2002fk is really of type Ia. Following is a report submitted to IAU circular. SUPERNOVA 2002fk in NGC 1309 K. Ayani, Bisei Astronomical Observatory (BAO) and H. Yamaoka, Kyushu University, write: "A low-resolution spectrum (range 500-700 nm) of SN 2002fk (IAUC 7973), obtained with BAO 1.01-m telescope on Sept. 20.7 UT, indicates that it is a type-Ia supernova before maximum light. Adopting the NASA/IPAC Extragalactic Database recession velocity of 2135 km/s, the expansion velocity deduced from Si II (rest 635.5 nm) is about 10900 km/s. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp