112  U SCORPII   (NR)   Range: 8.0-18.5V
     Position:   16 22 30.80  -17 52 42.9 (J2000, from .dat file)
     Magnitude:  V=18.510  B-V=0.459      (in .dat file)

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

1    16 22 09.4  -17 53 15  -306  -32  3  12.565  0.015   0.906  0.010  
2    16 22 45.8  -17 51 52   214   51  3  12.588  0.005   1.238  0.003  
3    16 22 08.1  -17 52 57  -325  -14  3  12.730  0.006   0.927  0.006  
4    16 22 27.7  -17 48 57   -45  226  3  12.764  0.005   1.511  0.007  
5    16 22 46.5  -17 57 01   224 -258  3  12.783  0.000   0.795  0.007  
6    16 22 44.4  -17 47 32   194  311  3  13.167  0.005   0.641  0.008  
7    16 22 11.9  -17 57 33  -270 -290  3  14.286  0.009   0.870  0.014  
8    16 22 22.3  -17 54 10  -121  -87  3  14.489  0.006   1.174  0.003  
9    16 22 29.2  -17 54 50   -23 -127  3  14.628  0.005   1.168  0.002  
10   16 22 38.9  -17 56 51   115 -248  3  14.751  0.005   0.967  0.009  
11   16 22 36.8  -17 51 55    86   48  3  15.098  0.006   0.837  0.006  
12   16 22 27.5  -17 54 15   -47  -92  3  15.494  0.016   0.818  0.015  
13   16 22 25.6  -17 51 34   -75   69  3  15.863  0.006   1.120  0.015  
14   16 22 22.2  -17 52 40  -123    3  3  16.090  0.006   0.806  0.023  
15   16 22 36.2  -17 51 22    77   81  3  16.383  0.016   0.863  0.020  
16   16 22 31.8  -17 53 52    14  -69  3  16.635  0.023   0.822  0.032  
17   16 22 29.2  -17 52 19   -22   24  3  16.697  0.019   0.856  0.038  
18   16 22 27.9  -17 51 32   -41   71  3  16.918  0.009   0.791  0.009  
19   16 22 27.1  -17 53 57   -53  -74  3  17.293  0.033   0.827  0.019   
20   16 22 32.5  -17 54 23    24 -100  3  17.481  0.058   0.841  0.072  
21   16 22 37.3  -17 53 03    92  -20  3  17.978  0.039   1.273  0.017   
22   16 22 30.2  -17 53 01    -9  -18  3  18.491  0.103   0.620  0.135  
23   16 22 31.1  -17 52 39     4    4  2  19.035  0.073   0.535  0.556   


The two faintest stars have large errors, and are included only for
guidance. They should not be used for comparison purposes.  

There is another sequence for U Scorpii, determined many years ago by PEP
photometry by Barry Menzies (Menzies, Circ. 171, VSS RASNZ, 1971). However
only V measured were taken. The sequence is shown below, with the three
common stars between it and Henden also indicated:

                                        Menzies   Henden
     16 23 16.1  -17 50 15   648  150    10.61                          
     16 22 25.8  -18 02 59   -72 -616    10.94                          
     16 22 54.0  -17 45 08   332  454    11.53                          
     16 22 45.8  -17 51 52   214   51    12.63    12.588
     16 22 09.4  -17 53 15  -306  -32    12.65    12.565 
     16 22 27.7  -17 48 57   -45  226    12.84    12.764
     16 22 31.7  -18 01 13    14 -510    13.74                          



Bruce Sumner
14 April 1999