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Dear Mike, Taichi and All, Yes, I have been monitoring V2552 Oph on a regular basis since Mike produced his chart. I continue to use his initial comparison sequence as this does the job well. I understand this is being reviewed. Attached is a text listing of my observations in JD format from the VSSOBS program of the VSS RASNZ. I am a few days behind in the data entry but this gives a good idea of what this star is doing. I have not reported any observations of this star to the vsnet simply because it has remained at maximum and I am still concerned about duplication of my observations in the various international data bases. All of my observations are sent on a monthly basis to both the VSS RASNZ and the AAVSO. Reports of unusual activity are sent through the vsnet. Trust this is of interest. Best wishes. Peter Williams Heathcote NSW ----- Original Message ----- From: "Mike Simonsen" <mikesimonsen@mindspring.com> To: "Taichi Kato" <tkato@kusastro.kyoto-u.ac.jp>; <vsnet-campaign-rcb@ooruri.kusastro.kyoto-u.ac.jp>; <vsnet-rcb@ooruri.kusastro.kyoto-u.ac.jp> Sent: Sunday, September 21, 2003 9:14 PM Subject: [vsnet-rcb 612] Re: V2552 Oph? > Peter Williams has been monitoring it for some time now. > I prepared a preliminary chart and sequence for him a while back. > > http://joevp.20m.com/cgi-bin/i/charts/provisional/HadV98_C_northup.jpg > > I've been meaning to update it with better photometry from ASAS-3 but AAVSO > is keeping me pretty busy at the moment. > > Peter wrote August 10, 2003- > "V2552 Oph has shown variations of several points since I commenced > monitoring, ranging between 10.8 and 11.0." > > Mike Simonsen > >
-171722 V2552 OPH 2452788.9674 11.00 11= HadV098 Wy -171722 V2552 OPH 2452789.9417 11.00 11= HadV098 Wy -171722 V2552 OPH 2452795.9063 11.00 11 Wy -171722 V2552 OPH 2452797.0181 11.00 11 Wy -171722 V2552 OPH 2452798.9444 11.00 11 Wy -171722 V2552 OPH 2452805.9868 11.00 11 Wy -171722 V2552 OPH 2452806.9965 11.00 11 Wy -171722 V2552 OPH 2452808.9646 10.90 11 Wy -171722 V2552 OPH 2452814.0694 11.00 11 Wy -171722 V2552 OPH 2452824.0215 10.70 11 Wy -171722 V2552 OPH 2452825.0083 10.90 11 Wy -171722 V2552 OPH 2452825.9236 10.90 11 Wy -171722 V2552 OPH 2452826.9611 10.90 11 Wy -171722 V2552 OPH 2452832.9722 11.00 11 Wy -171722 V2552 OPH 2452835.9708 11.00 11 Wy -171722 V2552 OPH 2452836.9271 11.00 11 Wy -171722 V2552 OPH 2452838.0181 11.00 11 Wy -171722 V2552 OPH 2452838.9819 10.90 11 Wy -171722 V2552 OPH 2452842.9792 10.80 11 Wy -171722 V2552 OPH 2452843.9618 10.80 11 Wy -171722 V2552 OPH 2452844.9736 10.80 11 Wy -171722 V2552 OPH 2452847.9354 10.80 11 Wy -171722 V2552 OPH 2452848.9278 10.90 11 Wy -171722 V2552 OPH 2452853.9389 10.80 11 Wy -171722 V2552 OPH 2452854.9424 10.90 11 Wy -171722 V2552 OPH 2452855.9743 10.80 11 Wy -171722 V2552 OPH 2452857.9611 10.80 11 Wy -171722 V2552 OPH 2452877.0118 11.00 11 Wy -171722 V2552 OPH 2452878.9292 10.90 11 Wy -171722 V2552 OPH 2452881.9819 10.90 11 Wy -171722 V2552 OPH 2452882.9208 10.80 11 Wy -171722 V2552 OPH 2452884.9243 10.80 11 Wy -171722 V2552 OPH 2452894.9556 10.90 11 Wy -171722 V2552 OPH 2452895.9174 10.90 11 Wy -171722 V2552 OPH 2452898.9438 10.80 11 Wy -171722 V2552 OPH 2452899.9361 10.80 11 Wy
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