121  FBS 1735+825   (CV?)   Range: 14.0B
     Position:   17 29 34 +82 26 47  (J2000, from FBS precessed)
     Magnitude:  unknown

ID     RA  (2000)   DEC       X    Y   N    V      ERR     B-V    ERR   

a) Comparison star sequence
 
1    17 29 21.6  +82 30 45   -24  238  4  13.171  0.020   0.632  0.008   
2    17 31 14.3  +82 24 05   199 -162  4  13.548  0.017   0.854  0.011   
3    17 28 37.0  +82 24 59  -113 -108  4  14.136  0.018   1.135  0.008   
4    17 29 47.0  +82 25 10    26  -97  4  14.872  0.019   0.954  0.009   
5    17 29 24.9  +82 29 46   -18  179  4  15.556  0.010   0.681  0.012   
6    17 29 27.2  +82 25 23   -13  -84  4  16.047  0.022   0.728  0.014   
7    17 30 46.9  +82 28 33   143  106  4  16.232  0.018   0.756  0.008   
8    17 28 33.4  +82 26 21  -120  -26  4  16.531  0.014   0.950  0.026   
9    17 29 44.7  +82 28 25    21   98  4  17.425  0.014   0.984  0.060   
10   17 30 12.5  +82 24 54    76 -113  4  18.359  0.049   0.778  0.073   


b) Wide-colour extension for CCD calibration

     17 29 50.8  +82 24 27    33 -140  4  13.350  0.017   0.543  0.007   
     17 31 29.7  +82 26 32   228  -15  4  15.971  0.027   1.454  0.016   


Notes:

1. The position of this potential UG variable has not been identified. 
The offsets given here are relative to the nominal position quoted in 
FBS (First Byurakan Spectral Sky Survey).

2. An examination of fourteen images of pixel data from the US Naval
Observatory Precision Measuring Machine of images obtained between 
1953 and 1997 showed no image down to magnitude 20 in the region of 
this suspected dwarf nova.

3. There is a bright star in the northwest corner of this field that 
was not measured as part of this sequence. This star has an accurate 
Tycho-2 magnitude of V=9.56+/-0.03.


Bruce Sumner 
11 June 1999
Revised 14 December 2000