Home Page Updated on January 16, 2018
MisV0012 = V1265 Sco
= IRAS 17534-3103 R.A.=17 56 43.17 Decl.=-31 04 05.4 (22 x 5", p.a. =92) flux(12)=0.94 flux(25)=<3.02 flux(60)=1.93 flux(100)=<79.19 4% variable
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. No known variable stars are within 5 arcmin.
Research and Publication
Light Curve Analysis of MisV Stars Identified with Candidate Variable Stars from OGLE-II Bulge Data
Yoshida, S.; Greaves, J.
Observations by MISAO Project