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Table 2
List of sources significantly (≥5σ) detected on the sky mosaic (Fig. 1).
| Name | lon. | lat. | F25−60 keV | ||
| deg | deg | mCrab | |||
|
|
|||||
| 4U 0352+30a | 163.08 | –17.14 | 39.42 ± 0.69 | ||
| RX J0440.9+4431a | 159.82 | –1.26 | 26.12 ± 0.53 | ||
| 3C111b | 161.68 | –8.83 | 5.32 ± 0.60 | ||
| MCG 8-11-11b | 165.74 | 10.41 | 7.27 ± 0.86 | ||
| 4C 32.14c | 158.99 | –18.77 | 3.15 ± 0.56 | ||
| LEDA 168563b | 157.26 | 3.43 | 2.76 ± 0.49 | ||
| MRK 3b | 143.29 | 22.72 | 7.23 ± 1.33 | ||
| Perseus CLd | 150.58 | –13.25 | 3.06 ± 0.58 | ||
| IGR J01532+2612 | 139.82 | –34.64 | 20.31 ± 3.91 | ||
| IGR J08135+5655 | 160.75 | 33.53 | 7.09 ± 1.38 | ||
| GK Pere | 150.96 | –10.12 | 2.82 ± 0.56 | ||
Notes. The newly detected sources are highlighted in bold. The 68% confidence interval for estimated sky coordinates depends on source significance: 2.1′, 1.5′, and <0.8′ for 5–6, 10, and >20σ, respectively (Krivonos et al. 2007b).
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