Below we include a set of useful calibrators for DSLR photometry on epsilon Aurigae. These values come from Homogeneous Means in the UBV System (Mermilliod 1991). Values were obtained through VizieR using the II/168 catalog.
Variable Stars:
| Star | HD | RA | DEC | (B-V) Cat |
| eps Aur | 31964 | 75.49223 | 43.82331 | 0.540 |
Comparision Stars (see chart below for AAVSO ID references).
| Star | AAVSO | HD | RA | DEC | V Cat | (B-V) Cat |
|
eta Aur |
32 |
32630 |
76.62872 |
41.23447 |
3.172 |
-0.178 |
|
zet Aur * |
38 |
32068 |
75.61953 |
41.07584 |
3.755 |
1.224 |
|
lam Aur |
47 |
34411 |
79.78531 |
40.09905 |
4.705 |
0.624 |
|
5 Aur |
60 |
31761 |
75.07641 |
39.39470 |
5.960 |
0.410 |
|
ome Aur |
50 |
31647 |
74.81421 |
37.89024 |
4.952 |
0.040 |
|
rho Aur |
|
34759 |
80.45173 |
41.80457 |
5.218 |
-0.149 |
|
mu Aur |
|
33641 |
78.35716 |
38.4845 |
4.851 |
0.187 |
|
sig Aur |
50 |
35186 |
81.16309 |
37.38535 |
5.010 |
1.416 |
|
58 Per |
43 |
29095 |
69.17262 |
41.26481 |
4.255 |
1.225 |
|
the Aur |
26** |
40312 |
89.93028
|
37.21258
|
2.645 |
-0.081 |
* NOTE: Zeta Aur is itself an eclipsing binary star. Be aware of it's eclipses or use it with two or more comparison stars.
** NOTE: The Aur is a preferred standard for visual observers. Please see this reference chart for it's location.
To assist you in finding the stars in the images, you may either use the AAVSO star chart (image below), or a downloadable PDF document that uses a real DSLR image.
DSLR Chart:
This document was created by bikeman as part of the DSLR Documentation and Reduction team. Download the PDF copy from here.
AAVSO Chart:
