(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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