Table 2.
Fermi/LAT results.
| Name | Flux | Energy flux | Liso | Eiso |
|---|---|---|---|---|
| (cm−2 s−1) | (erg cm−2 s−1) | (erg s−1) | (erg) | |
| GRB 180128A | < 1.9 × 10−6 | < 2.3 × 10−10 | < 3.7 × 1041 | < 1.8 × 1044 |
| GRB 200415A | (4.1 ± 2.2)×10−6 | (4.8 ± 2.7)×10−9 | (7.4 ± 4.2)×1042 | (3.6 ± 2.1)×1045 |
| GRB 150101B | < 4.9 × 10−6 | < 1.9 × 10−9 | < 9.4 × 1046 | < 2.8 × 1050 |
Notes. Comparison between the LAT detection of GRB 200415A and the upper limit on GRB 180128A and GRB 150101B. For the latter, we assumed z = 0.134 for the associated host galaxy (D = 0.65 Gpc) Fong et al. (2016), and we used the same analysis setup as for GRB 180128A (see the main text). All fluxes and energy fluxes measured from 0.1 to 10 GeV.
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.