Table 2
Parameters and gamma-ray fluxes of Galactic molecular clouds.
| Name |  , ) |
 |
 , |
Flux0.1−100GeV | Error | Flux1−500GeV | Error |
|---|---|---|---|---|---|---|---|
| RCrA | (0.56,–19.63) | 3 | (6.94,–19.63) | 0.91 | 2.24 | 0.87 | 0.15 |
| Oph | (355.81,16.63) | 5 | (34.94,16.63) | 11.3 | 0.56 | 12.1 | 2.80 |
| Perseus | (159.31,–20.25) | 4 | (148.44,–19.88) | 4.72 | 0.29 | 4.82 | 0.76 |
| Taurus | (173.19,–14.75) | 6 | (143.94,–19.50) | 16.4 | 6.69 | 15.4 | 1.27 |
| Orion A | (212.19,–19.13) | 4 | (233.69,–19.13) | 9.35 | 4.06 | 9.10 | 9.34 |
| Orion B | (204.56,–13.75) | 4 | (233.69,–19.13) | 9.26 | 10.2 | 8.70 | 14.3 |
| Chamaeleon | (300.43,–16.13) | 5.5 | (283.81,–16.13) | 4.56 | 1.21 | 4.46 | 3.53 |
| Mon R2 | (213.81,–12.63) | 1.5 | (233.81,–18.75) | 1.91 | 1.17 | 1.81 | 9.47 |
| RCrA | (0.56,–19.63) | 3 | (6.94,–19.63) | 0.73 | 1.80 | 0.33 | 0.06 |
| Oph | (355.81,16.63) | 5 | (34.94,16.63) | 10.2 | 0.51 | 5.46 | 1.27 |
| Perseus | (159.31,–20.25) | 4 | (148.44,–19.88) | 4.02 | 0.24 | 2.01 | 0.32 |
| Taurus | (173.19,–14.75) | 6 | (143.94,–19.50) | 13.6 | 5.56 | 6.32 | 0.52 |
| Orion A | (212.19,–19.13) | 4 | (233.69,–19.13) | 7.75 | 3.37 | 3.73 | 3.83 |
| Orion B | (204.56,–13.75) | 4 | (233.69,–19.13) | 7.56 | 8.32 | 3.55 | 5.83 |
| Chamaeleon | (300.43,–16.13) | 5.5 | (283.81,–16.13) | 3.78 | 1.00 | 1.86 | 1.47 |
| Mon R2 | (213.81,–12.63) | 1.5 | (233.81,–18.75) | 1.56 | 0.95 | 0.75 | 3.93 |
Notes. The second and third columns are the position and size of the source region. The forth column is the position of the background estimation region, whose size is the same as the source region. The fluxes and errors above the double horizontal lines in 0.1–100 GeV are in units of 10−7 ph cm−2 s−1 and 10−9ph cm−2 s−1, respectively.The fluxes and errors above the double horizontal lines in 1–500 GeV are in units of 10−8 ph cm−2s−1 and 10−10 ph cm−2 s−1, respectively.The fluxes and errors below the double horizontal lines are in units of 10−10 erg cm−2s−1 and 10−12 erg cm−2s−1, respectively.
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