194  V1208 TAURI   (UGSU)   Range: 15.2-18.4V
     Position:   04 59 44.04  +19 26 23.1  (J2000, from .dat file)
     Magnitude:  V=18.397  B-V=0.384       (.dat file, single night)
                                                            
ID     RA  (2000)   DEC       X    Y   N    V      ERR     B-V    ERR 

a) Comparison star sequence

1    04 59 41.0  +19 29 41   -42  198  4  12.181  0.066   0.597  0.067   
2    04 59 23.2  +19 32 36  -293  373  4  13.177  0.005   0.672  0.011   
3    04 59 31.8  +19 31 07  -172  284  4  14.099  0.000   0.726  0.012   
4    04 59 36.0  +19 28 01  -113   98  4  14.265  0.008   0.628  0.006   
5    04 59 39.4  +19 26 34   -64   11  4  14.466  0.008   0.846  0.012   
6    04 59 40.5  +19 24 31   -49 -112  4  14.747  0.006   0.686  0.008   
7    04 59 26.0  +19 29 19  -254  176  4  15.129  0.006   0.871  0.009   
8    04 59 35.8  +19 27 28  -116   65  4  15.451  0.010   0.698  0.012   
9    04 59 30.3  +19 26 49  -194   26  4  15.911  0.010   1.207  0.039   
10   04 59 46.1  +19 27 10    29   47  4  16.521  0.011   1.183  0.024   
11   04 59 44.7  +19 25 25    10  -58  4  17.596  0.019   0.865  0.027   


b) Wide-colour extension for CCD calibration

     04 59 22.3  +19 26 16  -308   -7  4  14.590  0.010   0.585  0.007   
     04 59 40.0  +19 22 23   -57 -240  4  14.249  0.019   1.373  0.010   


Notes:

1. This variable is also known as Tau3 in Downes, Webbink and Shara, 
PASP, 109, 734, April 1997. It was discovered to be a CV during the ROSAT
survey, where it was named RX J0459.7+1926 (Motch, A&A, 1996, 307, 459).

2. Superhumps were observed during the February 2000 superoutburst with 
a period of 0.7 days.

3. During the determination of this sequence this variable was observed 
as bright as V=15.218 and as faint as V=18.397 (Henden, private
communication, January 2001).


Bruce Sumner
26 January 2001