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>High resolution images from Tanabe-san are subject to further
>astrometric analysis by Yamaoka-san.
The position derived from Tanabe-san's images is:
11:31:22.401 +43:22:38.27
About 10 GSC-2.2 stars are used for reference, the mean error among
10 measurements is about 0".3.
cf. from [vsnet-campaign-dn 2160]
Kyoto image 11:31:22.426 +43:22:38.51
2MASS 11:31:22.39 +43:22:38.4 (the north star of a pair)
GSC2.2 11:31:22.423 +43:22:38.11 (the north star of a pair)
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
