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[vsnet-chat 6566] V Sequence for Liller's possible LMC nova

Re: Bill Liller's possible LMC nova, at (2000) 5h8.4m -68 26.2'.
I have compiled a comparison star sequence from published sources.

#         RA2000   DEC2000         V      B-V     Ref.        Id.
===================================================
1.    05:05:58.88  -68:24:59.8    8.16   0.57     1              HD 33617
2.    05:08:24.14  -68:28:34.9    9.49   0.35     1              HD 33970
3.    05:07:00.80  -68:28:35.1  10.24   0.96     1              HD 269035
4.    05:09:42.63  -68:26:11.6  11.05  1.13      1              HD 269095
5.    05:07:40.18  -68:15:36.8  11.12  0.56      1              P579
6.    05:08:02.43  -68:17:05.2  11.52  0.60      1              P589
7.    05:07:31.43  -68:21:24.5  11.71  0.46      1              HD 269049
8.    05:10:15.91  -68:23:52.9  12.15  0.56      1              P2121
9.    05:09:34.06  -68:24:41.6  12.54  0.02      2              Sk-68 56
10.  05:07:18.92  -68:25:37.6  12.79  0.28      2
C21=GSC9161.1314
11.  05:06:44.97  -68:20:47.0  13.11  0.24      2
G205=GSC9161.1156
12   05:07:08.62  -68:23:40.2  13.41 -0.11      2             Brunet 79
13.  05:07:43.35  -68:12:19.5  13.47 -0.16      2             Sk-68 54
14.  05:06:51.80  -68:25:48.0  14.1  -0.22       2             Brunet 74

Errors are available for most stars. In ref 1 they are of the order of 0.02
in V and B-V.
Ref:
1.  Gochermann, J. et al <Astron. Astrophys. Suppl. 99,591 (1993)>
     Grothues et al, <Astron. Astrophys. Suppl. 121,247 (1997)>
2.  Rousseau, J. et al <Astron. Astrophys. Suppl. 31, 243-260, 1978>

General Comments.  Stars from ref. 1 are foreground stars. Stars from ref. 2
are LMC  members.
On AAVSO prelim chart 030619, star 117 should be deleted, it is LMC V1111
(11.54-11.73V).

Regards,
Mati

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