Table 3
Change in gamma-ray flux of the first three molecular clouds for different background models.
| Name | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| RCrA | 0.13 | 0.06 | 0.15 | 0.07 | 0.11 | 0.03 | 0.14 | 0.04 | 0.11 | 0.03 | 0.13 | 0.04 | 0.09 | –0.01 | 0.12 | 0.01 |
| Oph | 0.05 | 0.05 | 0.05 | 0.06 | 0.05 | 0.06 | 0.06 | 0.07 | 0.05 | 0.06 | 0.06 | 0.07 | 0.05 | 0.08 | 0.07 | 0.08 |
| Perseus | 0.07 | 0.02 | 0.08 | 0.05 | 0.07 | 0.06 | 0.09 | 0.05 | 0.06 | 0.02 | 0.08 | 0.04 | 0.07 | 0.02 | 0.08 | 0.05 |
Notes. Thevalues represent the ratio between (F2 – F1) and F1, where F1 is derived using the method in the second paragraph of Sect. 2, and F2 is derived using the method in the third paragraph of Sect. 2. 1: Lorimer, 4 kpc, 150 K, and 2 mag; 2: Lorimer, 4 kpc, 150 K, and 5 mag; 3: Lorimer, 4 kpc, 105 K, and 2 mag; 4: Lorimer, 4 kpc, 105 K, and 5 mag; 5: Lorimer, 10 kpc, 150 K, and 2 mag; 6: Lorimer, 10 kpc, 150 K, and 5 mag; 7: Lorimer, 10 kpc, 105 K, and 2 mag; 8: Lorimer, 10 kpc, 105 K, and 5 mag; 9: SNR, 4 kpc, 150 K, and 2 mag; 10: SNR, 4 kpc, 150 K, and 5 mag; 11: SNR, 4 kpc, 105 K, and 2 mag; 12: SNR, 4 kpc, 105 K, and 5 mag; 13: SNR, 10 kpc, 150 K, and 2 mag; 14: SNR, 10 kpc, 150 K, and 5 mag; 15: SNR, 10 kpc, 105 K, and 2 mag; 16: SNR, 10 kpc, 105 K, and 5 mag.
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