(1992 Nov. 24) subject: VS observations + sequences Visual magnitude estimates by VSOLJ members object YYMMDD(UT) mag code RX And 921123.590 143 Mkn DX And 921123.433 <143 Mkn FO And 921123.507 <143 Mkn HT Cas 921123.506 <143 Mkn SS Cyg 921122.410 123 Mkn 921123.409 124 Mkn TY Psc 921123.510 138 Mkn GROJ0422+32 921123.594 137 Mkn Observer's code: Mkn: N. Makiguchi (Kanagawa, Japan) CCD(V) sequence for GRO J0422+32 N *111 *160 *130 *149 *145 *148 *160 *148 *160 126 * o Nova * 112 *142 *152 *150 *132 *153 *144 (field size 7') V band, Ouda station, Kyoto university 921121 based on (112) : V = 11.15 (Dodaira photometry) CCD (V) sequence for FG Sge N *117 *119 *121 o *131 FG + comp *118 *137 *133 *136 *126 * *130 *124 125 *130 # 85 * (relative magnitudes based on 11.8 star = GSC) field size 7', V filter enlargement *121 .159 | *144 comp--*o FG | .159 *147 *140 .155 *118 *137 .156 *149 .156 *136 image on Nov. 22, FG Sge is slightly fainter than the companion, approximately V=12.6 in this scale (not yet measured inidividually) The combined magnitudes is V=11.5 in this scale. Do you have recent (in November) estimates of AX Per?
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