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MisV0696     Profile MisV0696 R.A. 19h02m36s.04 Decl. -01o06'17".0 (2000.0) Mag. 12.6-14.2C = USNO-A2.0_0825.14163260 19 02 36.036 -01 06 17.02 13.0R 16.3B Digitized Sky Survey GIF image (15 x 15 arcmin) SIMBAD Query AAVSO VSX Database ASAS-3 Light Curve NSVS Light Curve (NSVS 13974371) Discovery Information It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida. NSV 11675 is 2.7 arcmin from MisV0696. No star brighter than 14.2 mag was detected at the catalogued position on our unfiltered CCD images. However, considering the large distance, MisV0696 is probably another new variable object. HS 1411, one of the variable stars discovered by FASTT, Flagstaff Astrometric Scanning Transit Telescope, is 1.2 arcmin from MisV0696. HS 1411 was detected as another variable star between 10.8 and 11.4 mag. Therefore, MisV0696 is another new variable star. Research and Publication MisV Stars in the TASS Tenxcat Database Yoshida, S.; Richmond, M. Light Curve 12.5 +--------------------------------------------------------+ | * | | | | | | | | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | * | 14.3 +--------------------------------------------------------+ 2451278 2451389 1999 Apr. 9 1999 July 29 Observations by MISAO Project Date Mag Filter Observer 1999 Apr. 14.75911 12.6 C Ken-ichi Kadota 1999 Apr. 14.75954 12.6 C Ken-ichi Kadota 1999 May 8.71193 12.9 C Ken-ichi Kadota 1999 May 8.71236 13.0 C Ken-ichi Kadota 1999 July 24.51391 14.1 C Ken-ichi Kadota 1999 July 24.51481 14.2 C Ken-ichi Kadota