Multi-wavelength behaviour of the radio galaxy SBS 1343+537: γ-ray flaring activity discovered by Fermi-LAT and coordinated Swift and SRT observations

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Table 2.

Energy flux, in the 100 MeV to 300 GeV range obtained by spectral fitting.

Period	${Flux}_{Power Law} (erg {cm}^{- 2} s^{- 1})$ $Mathematical equation: $ \mathrm{Flux}_{\mathrm{Power\ Law}}\,{\left(\mathrm{erg}\,\mathrm{cm}^{-2}\,\mathrm{s}^{-1}\right)} $$	${Flux}_{Log Parabola} (erg {cm}^{- 2} s^{- 1})$ $Mathematical equation: $ \mathrm{Flux}_{\mathrm{Log\ Parabola}}\,{\left(\mathrm{erg}\,\mathrm{cm}^{-2}\,\mathrm{s}^{-1}\right)} $$
Flare	(3.480±0.099) × 10⁻¹¹	(3.91±0.27) × 10⁻¹¹
Full period	(2.86±0.28) × 10⁻¹²	(2.75±0.32) × 10⁻¹²
4FGL-DR4	(3.14±0.31) × 10⁻¹²	–

Notes. We include, for reference, also the value reported in the 4FGL-DR4 catalogue (Ballet et al. 2024).

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