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[vsnet-campaign 820] DW Cnc



	An accurate sequence and chart are now available for this 
variable star thanks to field photometry acquired by Arne Henden. 

The chart, courtesy of Mike Simonsen, is available at:

    http://joevp.20m.com/cgi-bin/i/charts/hscharts/South_up/

The full field photometry file, including R&I measures, is at:

    http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/dwcnc.dat

Bruce Sumner
-----------------------
208  DW CANCRI   (UG)   Range: 14.1v-17.5p
     Position:   07 58 53.04  +16 16 45.5   (J2000, from .dat file)
     Magnitude:  V=14.915  B-V=0.023        (.dat file)

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

a) Comparison star sequence

1   07 59 12.1  +16 13 28   275 -197  2  12.331  0.019   0.506  0.031 
2   07 58 43.0  +16 17 24  -144   39  2  12.688  0.010   0.465  0.005 
3   07 59 06.8  +16 18 22   199   97  2  13.437  0.006   0.525  0.008 
4   07 58 35.6  +16 13 47  -251 -178  2  13.757  0.032   0.765  0.008 
5   07 59 04.6  +16 14 38   167 -127  2  14.074  0.008   0.528  0.002 
6   07 58 50.9  +16 14 45   -30 -120  2  14.539  0.012   0.916  0.008 
7   07 59 10.1  +16 15 42   247  -63  2  14.907  0.006   0.739  0.013 
8   07 59 00.5  +16 16 47   108    2  2  15.198  0.010   0.687  0.013 
9   07 58 38.5  +16 19 55  -209  190  2  15.495  0.017   0.781  0.013 
10  07 58 55.8  +16 17 11    40   26  2  16.093  0.008   0.944  0.019 
11  07 58 50.1  +16 16 50   -41    5  2  17.221  0.011   0.597  0.017 
12  07 58 54.4  +16 15 57    20  -48  2  18.701  0.055   0.704  0.151 

b) Wide-colour extension for CCD calibration

    07 58 38.9  +16 11 30  -203 -315  2  12.938  0.012   0.197  0.004 
    07 58 34.8  +16 11 11  -262 -334  2  15.703  0.016   1.374  0.020 

Notes:

1. This sequence is created from field photometry acquired by Arne 
Henden on two separate nights. Apart from the faintest star, this 
sequence is quite reliable and is not expected to change when extra 
nights are added to a later date to refine the errors. The star #4
has a large error and may be a low amplitude variable.

Bruce Sumner
22 March 2001

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