[vsnet-obs 56570] GSC3656.1328 revised

Hiroyuki Maehara mira at cetus-net.org
Mon Nov 20 02:57:40 JST 2006


I recalibrated the brightness of GSC3656.1328 by using sequence 
by A. Henden (ftp://ftp.aavso.org/public/calib/varcas06.dat).

Please delete following data in previous report.

> GSC3656.1328   20061103.69438 10.42Ic  Mhh.VSOLJ
> GSC3656.1328   20061103.69543 10.44Rc  Mhh.VSOLJ
> GSC3656.1328   20061103.69682 10.51V   Mhh.VSOLJ
> GSC3656.1328   20061103.69924 10.64B   Mhh.VSOLJ
> GSC3656.1328   20061104.69022 10.65Ic  Mhh.VSOLJ
> GSC3656.1328   20061104.69125 10.68Rc  Mhh.VSOLJ
> GSC3656.1328   20061104.69263 10.71V   Mhh.VSOLJ
> GSC3656.1328   20061104.69506 10.89B   Mhh.VSOLJ
> GSC3656.1328   20061105.36861 10.88V   Mhh.VSOLJ
> GSC3656.1328   20061105.58370 10.80Ic  Mhh.VSOLJ
> GSC3656.1328   20061105.58473 10.83Rc  Mhh.VSOLJ
> GSC3656.1328   20061105.58611 10.88V   Mhh.VSOLJ
> GSC3656.1328   20061105.58855 11.01B   Mhh.VSOLJ
> GSC3656.1328   20061107.66539 11.03Ic  Mhh.VSOLJ
> GSC3656.1328   20061107.66642 11.01Rc  Mhh.VSOLJ
> GSC3656.1328   20061107.66781 11.10V   Mhh.VSOLJ
> GSC3656.1328   20061107.67025 11.23B   Mhh.VSOLJ

Revised data are as follows:

GSC3656.1328   20061103.69438 10.34Ic  Mhh.VSOLJ
GSC3656.1328   20061103.69543 10.38Rc  Mhh.VSOLJ
GSC3656.1328   20061103.69682 10.47V   Mhh.VSOLJ
GSC3656.1328   20061103.69924 10.63B   Mhh.VSOLJ
GSC3656.1328   20061104.69022 10.57Ic  Mhh.VSOLJ
GSC3656.1328   20061104.69125 10.62Rc  Mhh.VSOLJ
GSC3656.1328   20061104.69263 10.67V   Mhh.VSOLJ
GSC3656.1328   20061104.69506 10.89B   Mhh.VSOLJ
GSC3656.1328   20061105.36861 10.84V   Mhh.VSOLJ
GSC3656.1328   20061105.58370 10.72Ic  Mhh.VSOLJ
GSC3656.1328   20061105.58473 10.77Rc  Mhh.VSOLJ
GSC3656.1328   20061105.58611 10.84V   Mhh.VSOLJ
GSC3656.1328   20061105.58855 11.00B   Mhh.VSOLJ
GSC3656.1328   20061107.66539 10.95Ic  Mhh.VSOLJ
GSC3656.1328   20061107.66642 11.00Rc  Mhh.VSOLJ
GSC3656.1328   20061107.66781 11.07V   Mhh.VSOLJ
GSC3656.1328   20061107.67025 11.22B   Mhh.VSOLJ

My data in vsnet-obs 56557, 56558, 56559, 56567 and 56569
were measured by using Henden's sequence.

Best regards,
Hiroyuki Maehara



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