SS Aurigae
(2000) 06 13 22.44 +47 44 25.6
Type:UGSS 
Range:10.5-15.8v*
Sequence CCD(V) A. Henden and M. Simonsen


#	RA		Dec		n	V	Err	B-V	Err
1	06 13 44.84	+47 33 55.1	2	10.666	0.031	0.558	0.071
2	06 13 41.74	+47 41 02.2	2	10.921	0.030	0.521	0.045
3	06 13 23.18	+47 46 31.5	2	11.013	0.004	0.265	0.037
4	06 13 02.65	+47 36 18.3	2	11.172	0.003	0.771	0.000
5	06 12 49.23	+47 47 02.6	2	12.061	0.003	1.036	0.001
6	06 13 44.37	+47 44 53.8	2	12.517	0.006	0.433	0.004
7	06 13 01.26	+47 42 53.3	2	13.142	0.005	1.021	0.005
8	06 13 41.47	+47 39 52.7	2	13.298	0.003	0.947	0.004
9	06 13 12.96	+47 45 00.0	2	13.902	0.004	0.871	0.001
10	06 13 46.47	+47 43 23.0	2	14.086	0.004	0.692	0.005
11	06 13 29.36	+47 44 26.8	2	14.570	0.006	0.740	0.001
12	06 13 31.94	+47 44 06.2	2	15.157	0.011	0.524	0.003
13	06 13 29.61	+47 44 02.2	2	15.299	0.004	0.689	0.012
14	06 13 26.91	+47 45 27.2	2	15.632	0.005	0.713	0.001
15	06 13 11.13	+47 43 54.8	2	15.936	0.003	0.998	0.009
16	06 13 21.03	+47 43 57.0	2	16.290	0.016	0.595	0.035
17	06 13 22.65	+47 42 58.4	2	16.934	0.013	0.640	0.026
	

Notes:
1. There are two bright Tycho 2 stars that can fill in the bright end of this sequence.
 
06 12 30.83 +47 33 08.4   V=9.61,  B-V=0.670
06 12 56.16 +47 54 18.0   V=10.46, B-V=1.041

2. Additional photometry was performed by Doug West for GSC 3379:0020.
(2000) 06 14 40.83 +47 48 09.8  V=11.47+/-0.04, B=12.05+/-0.05

3. * The actual quiescent magnitude is probably fainter than this.


Mike Simonsen
March 27, 2003