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Table 2
Spectral characteristics and statistic test (TS) value of the GMC listed in Table 1 obtained from the LAT data.
| # | Region | TS | Flux at 3 GeV[10-9 GeV-1 cm-2 s-1] | Eb [GeV] | χ2/d.o.f. (BPL) | χ2/d.o.f. (KPL) | χ2/d.o.f. (TPL) |
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| 1 | ρ Oph | 11 648 | 7.7 ± 0.8 | 4.7 ± 2.3 | 10.7/9 (0.30) | 22.2/11 (0.024) | 13.9/11 (0.24) |
| 2 | Orion B | 6107 | 3.0 ± 0.6 | 3.6 ± 1.3 | 10.8/9 (0.29) | 27.9/11 (2.3 × 10-3) | 13.1/11 (0.29) |
| 3 | Orion A | 22 021 | 5.9 ± 0.7 | 4.3 ± 1.2 | 11.0/10 (0.35) | 40.1/12 (4.9 × 10-5) | 14.0/12 (0.30) |
| 4 | Mon R2 | 1607 | 1.3 ± 0.2 | 3.0 ± 0.7 | 10.5/10 (0.39) | 29.4/12 (3.4 × 10-3) | 13.4/12 (0.34) |
| 5 | Taurus | 5670 | 9.8 ± 1.5 | 4.7 ± 1.5 | 10.5/10 (0.39) | 36.9/12 (2.3 × 10-4) | 16.5/12 (0.17) |
| 6 | R CrA | 2315 | 1.2 ± 0.8 | 0.9 ± 0.8 | 5.1/9 (0.82) | 7.4/11 (0.76) | 15.0/11 (0.18) |
| 7 | Chamaeleon | 2917 | 2.0 ± 0.5 | 2.0 ± 0.9 | 9.2/9 (0.42) | 24.0/11 (0.01) | 12.0/11 (0.36) |
| 8 | Perseus OB2 | 6410 | 3.8 ± 0.3 | 4.9 ± 2.1 | 11.7/10 (0.30) | 20.8/12 (0.05) | 17.3/12 (0.14) |
Notes. The individual χ2/d.o.f. of the spectral representation tested are also quoted with the corresponding probabilities in brackets (see text for more details).
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