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* 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

* Light Curve

    12.5  +--------------------------------------------------------+
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    14.3  +--------------------------------------------------------+
       2451278                                                  2451389
     1999 Apr. 9                                              1999 July 29

* Observations by MISAO Project

DateMagFilterObserver
1999 Apr. 14.7591112.6CKen-ichi Kadota
1999 Apr. 14.7595412.6CKen-ichi Kadota
1999 May 8.7119312.9CKen-ichi Kadota
1999 May 8.7123613.0CKen-ichi Kadota
1999 July 24.5139114.1CKen-ichi Kadota
1999 July 24.5148114.2CKen-ichi Kadota

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