Very high-energy gamma-ray detection and long-term multiwavelength view of the flaring blazar B2 1811+31

Open Access

Fig. 7.

Scatter plot of the PL spectral index Γ_γ and flux F_γ in the HE γ-ray data. In the top (bottom) panel, Γ_γ and F_γ derive from the Fermi-LAT lightcurve with 30-day bins (daily bins) shown in Figure 1 (Figure 3). The dotted lines mark the fits using Eq. (6).

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.