Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.
citing papers explorer
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Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT
Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
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Can BLR line profile shape improve single-epoch black hole mass estimates?
Expanded sample yields marginal evidence that f correlates with log10(FWHM/σ) of the broad Hβ line, consistent with earlier results and potentially enabling empirical f estimates.