Table 3
Spitzer photometry.
| ID | [3.6] | [4.5] | [5.8] | [8.0] | [24] |
|
|
|||||
| Foreground stars | |||||
| #2 | 13.31 | ... | 13.01 | ... | ... |
| #10a | ... | ... | 13.15 | ... | ... |
| #11 | 11.67 | 11.68 | 11.35 | 10.97 | 8.43 ± 0.30 |
| #15 | 13.64 | 13.55 | 13.57 | 13.15 | ... |
| #16a | 12.94 | 12.87 | 12.55 | ... | ... |
|
|
|||||
| IC 10 | |||||
| #3 | 13.32 | ...b | 12.59 | ...b | ... |
| #4 | 13.29 | 13.16 | 12.83 | 12.47 | ... |
| #6 | 13.05 | 13.04 | 12.82 | 12.55 | ... |
| #7 | 13.29 | ...b | 12.98 | ...b | ... |
| #8 | 13.21 | 12.65 | 12.15 | 11.13 | 7.62 ± 0.30 |
| #12 | 13.74 | 12.96 | 12.23 | 10.77 | 5.90 ± 0.10 |
| #13 | 13.20 | ... | 12.40 | ... | ... |
| #14 | 13.12 | 13.16 | 12.37 | ... | ... |
|
|
|||||
| Unknown membership | |||||
| #17 | 14.99 | 13.81 | 12.90 | 12.07 | ... |
Notes. Magnitudes calculated assuming zero-magnitude fluxes from the instrument handbooks. The uncertainties are ≈0.01, ≈0.01, ≈0.02, and ≈0.03 for [3.6], [4.5], [5.8], and [8.0] respectively. Bands with no data correspond to sources that were not found by the MOPEX algorithm to detect point sources, unless otherwise noted. Membership is based on the color diagnostics discussed in Sect. 4.4.
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