Optimizing the hunt for extraterrestrial high-energy neutrino counterparts

Open Access

Fig. 3.

CAZ optical light curve of the blazar J0509+0541 (also known as TXS 0506+056). Top: CAZ light curve. Bottom: Corresponding median-normalized flux density ( $S / \tilde{S}$ $S/\widetilde{S}$ ) distribution and its best-fit lognormal distribution (shown as the red curve with the parameters μ_LN ≈ 10⁻¹⁸ and σ_LN = 0.33).

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