FS Scuti
18 58 16.84  -05 24 05.8 (from dat file)
NA:
10.1p - 19.3B
Sequence: CCD(V) A. Henden  and  M. Simonsen

#	RA (2000)	Dec (2000)	Obs	V	Err	B-V	Err.
1	18 58 18.83	- 05 26 42.8	2	10.753  0.033	+0.441  0.005
2	18 58 03.21	- 05 21 02.1	2	12.135  0.000	+0.729  0.003
3	18 58 23.75	- 05 28 44.7	2	12.781  0.008	+0.959  0.006
4	18 58 25.52	- 05 21 28.8	2	13.108  0.006	+0.776  0.005
5	18 58 04.44	- 05 25 18.8	2	13.470  0.008	+0.796  0.001
6	18 58 31.52	- 05 24 39.4	2	13.663  0.006	+0.623  0.002
7	18 58 29.66	- 05 28 54.9	2	13.979  0.014	+0.791  0.013
8	18 58 13.94	- 05 27 19.8	2	14.306  0.000	+0.896  0.004
9	18 58 14.50	- 05 20 28.5	2	14.637  0.006	+0.970  0.004
10	18 58 22.23	- 05 24 55.7	2	14.878  0.006	+0.937  0.004
11	18 58 24.07	- 05 26 09.5	2	15.179  0.000	+1.030  0.011
12	18 58 07.18	- 05 26 29.7	2	15.514  0.017	+0.916  0.020
13	18 58 16.62	- 05 24 10.5	2	15.833  0.010	+0.956  0.005
14	18 58 19.21	- 05 23 50.9	2	16.078  0.008	+1.107  0.017
15	18 58 09.02	- 05 24 50.5	2	16.348  0.000	+1.083  0.029


Note: The position stated above has not been positively identified as the variable.
It is the nearest star to the position given in Downes et al. The actual variable may 
be a faint companion close by.


M. Simonsen  
October 24, 2002