Table 2
Fluxes of possible infrared counterparts to Srcs 3, 5, and 13.
| Band | I1 | I2 | I3 | I4 | M1 | J | H | K s |
| λ,μm | 3.6 | 4.5 | 5.8 | 8.0 | 24 | 1.2 | 1.7 | 2.2 |
|
|
||||||||
| Source | ||||||||
| o51 | 2.2 ± 0.1 | 1.5 ± 0.1 | <1.6 | <1.6 | <0.9 | ··· | ··· | ··· |
| o31 | 4.5 ± 0.1 | 2.4 ± 0.1 | <1.2 | <1.4 | <2.7 | ··· | 3.8 ± 0.4 | 4.5 ± 0.3 |
| o32 | 210 ± 0.9 | 120 ± 0.4 | 91.0 ± 0.8 | 54.1 ± 0.4 | 6.3 ± 0.1 | 6.3 ± 0.2 | 75 ± 1.6 | 140 ± 2.7 |
| o13 | 5.4 ± 0.4 | 2.9 ± 0.3 | 2.0 ± 0.3 | 1.5 ± 0.3 | ··· | 2.2 ± 0.2 | 6.6 ± 0.2 | <5.9 |
|
|
||||||||
| ext5 | 4.0 | 3.5 | 3.2 | 2.8 | 1.0 | 575 | 58 | 13 |
| ext3 | 2.5 | 2.4 | 2.2 | 2.0 | 1.0 | 76 | 16 | 5.8 |
Notes. Infrared fluxes of Src o51, o31, o32, and o13 are quoted for Spitzer IRAC bands I1, I2, I3, and I4, Spitzer MIPS band M1, and 2MASS bands J, H, and Ks (see Fig. 5). The flux units are 10-13 erg cm-2 s-1. Errors are at the 68% level. Estimates of extinction factors (i.e. the value 10Aband/2.5, AV is computed from the X-ray absorption) at positions of Srcs 3 and 5 are listed as ext5 and ext3.
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