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= GSC 3096-00465 17h49m20s.96 +42o13'15".2 Error:0.2" Mag:14.44 Ma gError:0.41 Band:1 Class:0 Plate:02S0 Flag:T Epoch:23 MAY 1982 = GSC 3096-00465 17h49m20s.92 +42o13'15".2 Error:0.2" Mag:14.49 Ma gError:0.40 Band:1 Class:0 Plate:01H4 Flag:T Epoch:23 MAY 1982 = USNO-A2.0 1275.09590600 17h49m20s.933 +42o13'15".02 Mag(R):14.5 M ag(B):15.3
Seiichi Yoshida, MISAO Project; Nobuo Ohkura and Youichirou Nakashima, Okayama, Japan, discovered new variable stars MisV1432 - MisV1435.
They were picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura and Youichirou Nakashima. Their variations were confirmed by Ohkura and Nakashima (MisV1434), or by Yoshida, Ohkura and Nakashima (others).
Stefan Huemmerich reported the Catalina Sky Survey data revealed it is a W UMa-type (EW) eclipsing variable with a period of 0.32119 days, brightness range of 14.7-15.6 mag(V) (light curve).
Light curve by Catalina Sky Survey (Stefan Huemmerich)
Observations by MISAO Project