> Kato-san might consider recalibrating the vsnet V1830 Sgr chart using an > adjustment found from Henden's photometry for V4444 Sgr, which is about a > degree due west. How do these compare to 'Kato V' derived from USNO-A1.0? > Some of the brighter stars in the V1830 field might also be in Tycho-2, which > will give a hint as to whether the RASNZ chart has a zero-point problem. The star in question has already published photometry. 181350.7 -274200 (2000.0) UBV_V1830Sgr 12.56 0.01 -0.78 - - - - N=1 Nm=1 - Regards, Taichi Kato