Dear colleagues, New variable star discovery by the MISAO Project (MisV1003). MisV1003 R.A. 19h48m14s.63 Decl. +31o34'17".2 (2000.0) Mag. 13.1C-14.5C Type SR? = USNO-A2.0_1200.13281320 19 48 14.625 +31 34 17.21 15.9R 19.4B = 2MASS 194814.611 +313416.78 (2000.0) 9.205 8.040 7.551 http://vsnet.aerith.net/misao/data/MisV/MisV1003.gif MisV1003 19990803.63494 145C Mis image="KenIchi Kadota" MisV1003 19990803.63538 142C Mis image="KenIchi Kadota" MisV1003 19990803.63706 144C Mis image="KenIchi Kadota" MisV1003 19990803.63750 144C Mis image="KenIchi Kadota" MisV1003 20000708.55560 131C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1003. It was picked up by Yoshida from the candidates of new variable stars detected by the PIXY system from images taken by Ohkura comparing with images taken by Kadota. Kadota and Yoshida judged it as a real variable star. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis". The identification with the 2MASS data is by Taichi Kato and John Greaves. IRAS 19462+3127 is 31 arcsec from MisV1003, however, Taichi Kato and John Greaves pointed out IRAS 19462+3127 is not identified with MisV1003. Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/