Table 1
Analysis of known gamma-ray novae with Pass 8.
| Nova | t start | t stop | Duration | TS | Index | Cutoff | Flux |
| [MET] | [MET] | [days] | [GeV] | [10-7 cm-2s-1] | |||
| V407 Cyg 2010 | 289872002 | 291772802 | 22 | 526.6 | 1.27 ± 0.18 | 2.0 ± 0.5 | 3.47 ± 0.44 |
| V1324 Sco 2012 | 361411202 | 362880003 | 17 | 185.8 | 1.92 ± 0.16 | 7.7 ± 4.7 | 4.40 ± 0.85 |
| V959 Mon 2012 | 361756802 | 363657603 | 22 | 193.7 | 1.50 ± 0.28 | 1.3 ± 0.5 | 2.64 ± 0.45 |
| V339 Del 2013 | 398304003 | 400636803 | 27 | 364.0 | 1.68 ± 0.22 | 3.0 ± 1.8 | 1.45 ± 0.19 |
| V1369 Cen 2013 | 407894403 | 411264003 | 39 | 129.3 | 2.00 ± 0.26 | 2.0 ± 1.0 | 2.51 ± 0.52 |
| V5668 Sgr 2015 | 448588803 | 453340803 | 55 | 87.5 | 2.11 ± 0.12 | – | 0.61 ± 0.13 |
| combined (all) | 1.71 ± 0.08 | 3.2 ± 0.6 | |||||
| combined (all, exc. V407 Cyg) | 1.90 ± 0.08 | 4.3 ± 1.2 | |||||
Notes. We adopted the time windows from previous analyses performed by Ackermann et al. (2014) and Cheung et al. (2016b), which differ from the 15 day time window used for the results presented in Appendix A. The energy cutoff for V5668 Sgr is not constrained by the fit. We therefore present the results of a simple power-law fit without a cutof,f for which we find that the TS value decreases only insignificantly from 89.0 to 87.5.
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