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[vsnet-sequence 194] MisV1147 in Cepheus



ID:  MisV1147 Cep  Range: 12.3-13.8C
Position:  22 54 03.80  +58 54 01.6 (J2000, from .dat file)
Magnitude:  V=13.365  B-V:+0.814
Sequence:  CCD(V) A. Henden & M. Simonsen

a) Comparison star sequence

ID   RA            DEC         N    V      ERR    B-V     ERR    U-B     ERR
V-R     ERR    R-I     ERR

1    22 53 59.41  +58 53 40.8  1  10.805  0.001  +0.229  0.001  +0.117
0.001  +0.111  0.001  +0.165  0.001
2    22 53 49.19  +58 52 40.6  1  11.380  0.001  +0.335  0.001  +0.114
0.001  +0.214  0.001  +0.243  0.001
3    22 53 54.37  +58 58 13.7  1  11.805  0.001  +0.442  0.001  +0.155
0.001  +0.278  0.001  +0.310  0.001
4    22 54 53.96  +58 54 09.2  1  12.091  0.001  +1.049  0.001  +0.525
0.003  +0.708  0.001  +0.776  0.001
5    22 53 40.10  +58 59 56.9  1  12.605  0.001  +0.486  0.001  -0.061
0.002  +0.352  0.001  +0.319  0.002
6    22 53 21.96  +58 58 51.1  1  12.807  0.001  +0.855  0.002  +0.515
0.004  +0.494  0.001  +0.386  0.002
7    22 54 07.81  +58 57 39.3  1  13.191  0.002  +0.434  0.003  -0.018
0.004  +0.303  0.003  +0.330  0.003
8    22 53 55.50  +58 55 44.4  1  13.496  0.002  +0.782  0.003  +0.263
0.004  +0.482  0.003  +0.480  0.004
9    22 54 11.03  +58 57 03.7  1  13.768  0.002  +0.700  0.004  +0.179
0.006  +0.423  0.003  +0.416  0.004
10   22 54 18.05  +58 51 16.3  1  14.099  0.003  +0.633  0.004  +0.341
0.007  +0.372  0.004  +0.429  0.005
11   22 53 50.47  +58 50 36.0  1  14.301  0.003  +0.761  0.005  +0.347
0.009  +0.471  0.004  +0.478  0.005
12   22 54 48.81  +58 55 27.5  1  14.716  0.004  +0.723  0.006  -0.009
0.009  +0.461  0.006  +0.470  0.006
13   22 54 16.31  +58 56 39.2  1  15.018  0.005  +0.796  0.008  +0.436
0.015  +0.499  0.007  +0.531  0.008
14   22 54 40.08  +58 56 41.8  1  15.266  0.006  +0.666  0.008  +0.386
0.015  +0.408  0.008  +0.441  0.010
15   22 54 11.95  +58 54 00.5  1  15.600  0.008  +0.900  0.013  +0.328
0.031  +0.548  0.011  +0.576  0.013

Notes:

a)  Note that labeled comparison stars above magnitude 12.5 may be in error
due to camera saturation.
Consider these stars suspect until further photometry can be done.

b)  The star labelled 14.1 has a close 17th magnitude companion.

Vance Petriew
Revised 09 November 2002


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