Home Page Updated on November 1, 2017
MisV0476 = V5161 Sgr
= IRAS 17539-2405 R.A.=17 56 58.41 Decl.=-24 06 11.9 (24 x 4", p.a. =91) flux(12)=25.15 flux(25)=8.91 flux(60)=<20.48 flux(100)=<254 .90 96% 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.
Taichi Kato pointed out this is identified with a carbon star CS3906.
Research and Publication
Light Curve Analysis of MisV Stars Identified with ASAS Variables
Yoshida, S.; Greaves, J.
Observations by MISAO Project