Dear colleagues, We submitted the following report of our spectroscopy of two supernovae to CBAT. SUPERNOVA IN NGC 4157 K. Ayani, Bisei Astronomical Observatory (BAO); T. Hashimoto and H. Yamaoka, Kyushu University, write: "A preliminary reduction of low-resolution spectrum (range 400-800 nm) of SN 2003? in NGC 4157, obtained with BAO 1.01-m telescope on Jan. 12.8 UT, shows a prominent H-alpha emission (FWHM about 10000 km/s) with a P-Cyg profile, which suggests that it is a normal type-II supernova." SUPERNOVA IN IC 1129 K. Ayani, Bisei Astronomical Observatory (BAO); and H. Yamaoka, Kyushu University, write: "A low-resolution spectrum (range 400-800 nm) of SN 2003? in IC 1129, obtained with BAO 1.01-m telescope on Jan. 12.9 UT, indicates that it is a type-Ia supernova several days before maximum light. Adopting the NASA/IPAC Extragalactic Database recession velocity of 6540 km/s, the expansion velocity deduced from Si II (rest 635.5 nm) is about 12100 km/s." Best ragards, Kazuya Ayani Bisei Astronomical Observatory