Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.
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Stacked blazar data show strongest gamma-ray to radio correlation at a 180-day delay, with some sources displaying 1-3 year lags between activity in the two bands.
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Locating the Production Sites of High-Energy Neutrinos in Blazar Jets
Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.
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Characterizing Gamma-Radio Delayed Flaring Activity from Blazars
Stacked blazar data show strongest gamma-ray to radio correlation at a 180-day delay, with some sources displaying 1-3 year lags between activity in the two bands.