184  KZ GEMINORUM   (UG)   Range: 14.7-<18.5p
     Position:   06 53 02.8   +16 39 52    (J2000, from DWS)
     Magnitude:  unknown
                                                            
ID     RA  (2000)   DEC       X    Y   N    V      ERR     B-V    ERR

a) Comparison star sequence

1   06 53 22.4  +16 37 32   283 -142  3  11.267  0.249   0.309  0.058   
2   06 53 05.1  +16 37 20    34 -154  3  12.131  0.081   0.379  0.037   
3   06 53 17.2  +16 40 11   208   17  3  12.480  0.026   0.817  0.024   
4   06 53 15.0  +16 38 44   177  -71  3  13.081  0.017   0.415  0.004   
5   06 52 46.0  +16 40 55  -240   61  3  13.558  0.012   0.580  0.004   
6   06 52 45.8  +16 43 59  -243  245  3  14.143  0.023   0.418  0.004   
7   06 53 05.7  +16 40 24    43   30  3  14.390  0.010   1.165  0.017   
8   06 53 02.5  +16 40 06    -3   12  3  14.699  0.062   0.554  0.007   
9   06 52 58.6  +16 43 24   -59  210  3  15.047  0.016   0.556  0.003   
10  06 53 03.7  +16 40 34    15   40  4  15.537  0.012   0.663  0.009   
11  06 53 01.2  +16 39 40   -22  -14  4  16.378  0.024   0.879  0.011   
12  06 53 00.3  +16 40 11   -34   17  4  17.075  0.026   0.781  0.015   
13  06 53 02.6  +16 39 34    -1  -20  3  17.875  0.083   0.733  0.073   
14  06 53 03.4  +16 39 09    11  -45  1  19.025  0.017   1.266  0.034   


b) Wide-colour extension for CCD calibration

     06 53 18.7  +16 38 12   230 -102  3  14.932  0.014   0.194  0.008   
     06 52 50.0  +16 44 34  -183  280  3  13.918  0.019   0.338  0.006   
     06 52 56.2  +16 38 32   -94  -82  3  12.397  0.053   1.312  0.031   
     06 52 42.1  +16 45 29  -297  335  3  12.183  0.081   1.335  0.068   


Notes:

1. Star #1 is saturated and its magnitude and colour are very approximate.
It should be used for guidance only until an accurate magnitude is
determined. This star also has an approximate Tycho-2 magnitude of
V=11.04+/-0.09, but even this magnitude needs to be treated with care.

2. The accurate position of KZ Gem is unknown. The position used for 
the derivation of this sequence is from Downes, Webbink and Shara,
PASP,100,734,1997, which places the variable within a tight grouping of
faint stars, the brightest of which is the V=14.7 star #8.

3. The very faint star #14 is included for guidance only. This single 
night measurement is probably only accurate to about 0.2 magnitude.


Bruce Sumner
3 January 2001