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[vsnet-campaign 867] Re: [vsnet-alert 5828] Re: New Haseda variable (HadV82) = WR104
Together with Brian Skiff's reference stars, you should
be able to calibrate the UCAC1 magnitudes for this field
well enough to serve as a sequence down to 16th magnitude
or so; an excellent stop-gap until someone gets
quality photometry for the field.
Arne
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
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