A catalog of 7918 blazars and candidates with nightly optical light curves, quantified variability, and Bayesian blocks-derived flaring periods from three all-sky surveys.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Only one of 87 LMC blue supergiants shows S Dor-like variability, implying the S Dor phase lasts at most ~1000 years and can occur at low luminosities due to Eddington-limit physics.
Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.
citing papers explorer
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The incidence of LBV variability in the LMC
Only one of 87 LMC blue supergiants shows S Dor-like variability, implying the S Dor phase lasts at most ~1000 years and can occur at low luminosities due to Eddington-limit physics.
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Association of the IceCube neutrinos with CAZ blazar light curves
Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.