From samus@lnfm1.sai.msu.ru Wed Feb 27 17:34:50 2002 Delivered-To: tkato@kusastro.kyoto-u.ac.jp Date: Wed, 27 Feb 2002 11:34:44 +0300 (MSK) From: "Nikolai N. Samus" <samus@sai.msu.ru> To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> Subject: Re: [vsnet-gcvs 174] Re: [vsnet-chat 5136] GCVS errors MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by AMaViS perl-11 Content-Length: 1334 Dear Taichi, In March, a paper will appear in Astronomy Letters introducing the results of our work on systematic improvement of coordinates for GCVS Volume I stars. We are continuing the work for Vol. II stars. The particular case of V728 Her has been noticed and will be corrected. I think the corrected version of Vol. II will be added to the files at our web site within a year (if we are through with the very difficult constellation of Ophiuchus). Best regards Kolya On Wed, 27 Feb 2002, Taichi Kato wrote: > Re: [vsnet-chat 5136] GCVS errors > > Example of V728 Her: > > GSC3081.676 171804.29 +415038.8 (2000.0) 10.38 1 > GSC3081.676 171804.32 +415038.9 (2000.0) 10.94 1 > USNO1275.09394448 171804.320 +415039.13 (2000.0) 10.1 11.1 > 2MASS 171804.305 +415038.82 (2000.0) 10.031 9.893 9.870 > 171804.3 +415039 (2000.0) ROTSE1_J171804.31+415039.3 11.11 (0.400) ew 0.471 > 171804.3 +415038 (2000.0) 1084V > 171804.2 +415038 (2000.0) 1062 0.60 TYC2-3081.676.1 (10.68 0.05) (11.39 0.07) > 171804.3 +415038 (2000.0) HERV728 * EW/KW 10.9 11.5 P 41571.273 0.4462587 - R0/PZP15A > > The object was already correctly identified on the discovery paper. > It was apparent that Hipparcos team noticed this identification. > ROTSE team also independely detected the variablilty of the correct star. > > Regards, > Taichi Kato >