Return to Home Page
(1993 Mar. 23)
subject: DI UMa
DI UMa
The star was observed between 22.660 and 22.753 UT using 60cn +
V-band CCD at Ouda. The variable had averaged magnitude of V=14.9 based
on GSC and no variation larger than 0.1 mag was detected.
The following is the V-band sequence.
frame DD55913 2400 DI UMa V
date 93 3 22.66306
6505 19960 1554 0
6824 3650 1140 0
11465 17284 1408 0
13156 23981 1498 0 DI UMa
13381 23025 1351 0
17430 19506 1514 0
X Y mag saturation name
V magnitude based on GSC V=11.4 star.
(X,Y): unit 0.01 pixel (=0.02 arcsec)
Mag 13.51 star is the close companion.
Regards,
Taichi Kato
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
