PDRS is an O(N) algorithm for identifying high-activity regions in time series by seeding at local maxima and using gradient-aware search, achieving performance comparable to Bayesian Blocks.
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5 Pith papers cite this work, alongside 123 external citations. Polarity classification is still indexing.
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UNVERDICTED 5representative citing papers
Reevaluation of 610 FSRQ candidates shows most radio spectra are flat within per-source uncertainties but 60% of well-covered sources exhibit restarted-peaked morphologies, indicating the flat-spectrum label is insufficient and BZQ better captures the diversity.
Systematic search of ZTF DR23 data yields catalogs of 28,504 coarse and 1,984 refined AGN flares with public release.
Multi-wavelength monitoring of a gamma-ray flare in 1H 0323+342 reveals sub-hour variability, jet-corona transition, and ~10^46 erg/s jet power via external Compton modeling of disk and BLR photons.
Estimates based on 17 years of Fermi LAT data indicate COSI may detect MeV polarization in a small number of blazar flares, with flat-spectrum radio quasars as the top targets.
citing papers explorer
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PDRS : A Linear $\mathcal{O}(N)$ Algorithm for Segmentation of High-Activity Regions in Irregularly Sampled Time Series
PDRS is an O(N) algorithm for identifying high-activity regions in time series by seeding at local maxima and using gradient-aware search, achieving performance comparable to Bayesian Blocks.
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The Phenomenological Nature of Quasar-type Blazars (BZQ). I. Revisiting the Flat-Spectrum Paradigm
Reevaluation of 610 FSRQ candidates shows most radio spectra are flat within per-source uncertainties but 60% of well-covered sources exhibit restarted-peaked morphologies, indicating the flat-spectrum label is insufficient and BZQ better captures the diversity.
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A Systematic Search for Active Galactic Nucleus Flares in ZTF Data Release 23
Systematic search of ZTF DR23 data yields catalogs of 28,504 coarse and 1,984 refined AGN flares with public release.
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A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342
Multi-wavelength monitoring of a gamma-ray flare in 1H 0323+342 reveals sub-hour variability, jet-corona transition, and ~10^46 erg/s jet power via external Compton modeling of disk and BLR photons.
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Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI
Estimates based on 17 years of Fermi LAT data indicate COSI may detect MeV polarization in a small number of blazar flares, with flat-spectrum radio quasars as the top targets.