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[vsnet-campaign-dn 2179] Re: 1RXP J113123+4322.5: superhumps still prominent

>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

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