Dear SN watchers, The KAIT discovered two new SNe, both are considerably nearby. The follow-up observations are encouraged. SN 2001P has discovered and confirmed on Jan. 31.4 UT and Feb. 1.3 UT, respectively. The discovery magnitude is reported as 17.5:C. The location is R.A. = 11h53m21s.56, Decl. = +20o44'53".3 (2000.0), which is about 17" east and 13" south of the nucleus of the barred-spiral ((R)SB(rs)b) galaxy NGC 3947. The new object is somewhat outside of the inner ring-like arm. There is a mag 14 foreground star GSC 1443-2559 (GSCmag=13.47, USNO_A2.0 rmag=14.4, bmag=16.1) about 50" east of the nucleus of the host galaxy. From the recession velocity of NGC 3947, the expected maximum for normal SN Ia is about mag 16. Note that NGC 3947 has produced SN 1972C, which was caught at m_p = 16. The Spectroscopy of SN 2001P has revealed that it is of type Ia about a week past maximum, and it seems to be subluminous. The follow-up photometry will reveal the decline rate, which is considered to be faster for subluminous SN Ia than a normal one. On the other hand, SN 2001Q was discovered on Jan 31.4 UT (mag 18.6:C) and confirmed on Feb. 1.3 (mag 18.3:C), which indicate that it is in rising. The position is R.A. = 11h25m19s.77, Decl. = +63o43'15".6 (2000.0), which is about 4" east and 30" south of the nucleus of the dim face-on spiral (SA(rs)c) galaxy UGC 6429. At the very neighbourhood, there is very dim (rmag 19.8, bmag 19.5) USNO_A2.0 object (position end figures 19s.64, 15".9), which seems to be an HII region. Another USNO_A2.0 object (position end figures 21s.89, 6".20) seems to be a companion galaxy or also an HII region. From the recession velocity of UGC 6429, the expected maximum for normal SN Ia is about mag 15. Photometric observation is encouraged for this rising SN. The spectrum of SN 2001Q shows that it is young type II SN. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp