Table 1
Integral contribution from our new γ-ray sources for different energy bins, compared to EGB and IGRB fluxes reported in (Ackermann et al. 2015a).
| Ebin (GeV) | I EGB | I IGRB |
|
%EGB | %IGRB |
|
%EGB | %IGRB |
|
|
||||||||
| 1.1−13 | 4.5 × 10-7 | 2.7 × 10-7 | 1.22 × 10-9 | 0.27% | 0.45% | 1.73 × 10-9 | 0.38% | 0.65% |
| 13−36 | 1.4 × 10-8 | 8.2 × 10-9 | 8.48 × 10-11 | 0.61% | 1.0% | 1.19 × 10-10 | 0.86% | 1.4% |
| 36−51 | 1.8 × 10-9 | 1.1 × 10-9 | 1.59 × 10-11 | 0.88% | 1.4% | 2.24 × 10-11 | 1.2% | 2.0% |
| 51−72 | 1.1 × 10-9 | 6.3 × 10-10 | 1.19 × 10-11 | 1.1% | 1.9% | 1.68 × 10-11 | 1.5% | 2.7% |
| 72−100 | 6.2 × 10-10 | 3.6 × 10-10 | 8.69 × 10-12 | 1.4% | 2.4% | 1.23 × 10-11 | 2.0% | 3.4% |
| 100−140 | 3.1 × 10-10 | 1.5 × 10-10 | 6.89 × 10-12 | 2.2% | 4.6% | 9.82 × 10-12 | 3.2% | 6.5% |
| 140−200 | 1.9 × 10-10 | 9.8 × 10-11 | 5.63 × 10-12 | 2.9% | 5.7% | 8.05 × 10-12 | 4.2% | 8.2% |
Notes.Columns headed %EGB show the significance of new detections with respect to the total EGB component, and columns headed %IGRB show the fraction of IGRB component we have solved in the present work. The superscripts TS identify the cases where we only consider our new detections at TS > 25 level, and the case considering all new detections at TS > 10 level. Here we take into account our detections at | b | > 10°, and all intensities reported are in units [ph/cm2/s/sr].
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.