Table B.1
Point sources fitted in the analysis.
| Source | l | b | TS | k | Γ | Photon flux | Energy flux |
|---|---|---|---|---|---|---|---|
| PKS 1830–210 | 12.17 | −5.71 | 24.4 | 3.2±0.9 | 2.2±0.2 | 1.0±0.4 | 3.8±1.1 |
| LS 5039 | 16.88 | −1.29 | 85.2 | 7.3±0.9 | 1.5±0.1 | 1.3±0.2 | 10.4±1.2 |
| Cyg X-1 | 71.33 | 3.07 | 252.8 | 6.8±1.0 | 2.5±0.1 | 2.9±0.6 | 8.9±1.4 |
| Vela pulsar | 263.55 | −2.79 | 31.6 | 5.3±1.0 | 1.5±0.2 | 1.0±0.2 | 7.4±1.4 |
| PKS 0506–612 | 270.55 | −36.07 | 16.4 | 2.0±1.1 | 2.5±0.4 | 0.9±0.6 | 2.7±1.5 |
| 3C 273 | 289.95 | 64.36 | 85.3 | 7.1±0.8 | 1.8±0.1 | 1.6±0.2 | 8.7±1.0 |
| 3C 279 | 305.10 | 57.06 | 32.8 | 4.1±0.7 | 1.8±0.2 | 0.9±0.2 | 5.1±0.9 |
| Cen A | 309.52 | 19.42 | 164.8 | 8.1±1.0 | 2.1±0.1 | 2.4±0.4 | 9.7±1.2 |
| GRO J1411–64 | 311.50 | −2.50 | 38.3 | 2.2±1.2 | 2.7±0.4 | 1.3±0.9 | 3.4±2.1 |
| PSR J1513–5908 | 320.32 | −1.16 | 49.3 | 6.8±1.0 | 1.6±0.1 | 1.3±0.2 | 9.0±1.3 |
Notes. l and b specify the Galactic longitudes and latitudes of the point sources in degrees, TS gives the test statistic of the source detection, k are the power-law prefactors, and Γ are the spectral indices. Power-law prefactors are in units of 10−6 ph cm−2 s−1 MeV−1 and specified for a pivot energy of 4.5 MeV. Photon and energy fluxes are specified for the 0.75–30 MeV energy band, with photon fluxes in units of 10−4 ph cm−2 s−1 and energy fluxes in units of 10−10 erg cm−2 s−1.
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