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Table · dataset · 2022

Multiwavelength cross-correlations in blazars

Listed in IVOA Registry (Virtual Observatory)

Blazars are known for their energetic multiwavelength flares from radio wavelengths to high-energy {gamma}-rays.

Description

In this work, we study radio, optical, and {gamma}-ray light curves of 145 bright blazars spanning up to 8 yr, to probe the flaring activity and interband correlations. Of these, 105 show >1{sigma} correlations between one or more wavebands, 26 of which have a >3{sigma} correlation in at least one wavelength pair, as measured by the discrete correlation function.

The most common and strongest correlations are found between the optical and {gamma}-ray bands, with fluctuations simultaneous within our ~30d resolution. The radio response is usually substantially delayed with respect to the other wavelengths with median time lags of ~100-160d. A systematic flare identification via Bayesian block analysis provides us with a first uniform sample of flares in the three bands, allowing us to characterize the relative rates of multiband and 'orphan' flares.

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Multiband flares tend to have higher amplitudes than 'orphan' flares.

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Stated by source
Gamma-Ray
Inferred from text
Astronomical sciences 72%
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/mnras/480/551712 d agoJSON v1
FieldAssertionExtractorEvidence
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concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (72%)
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concepts[modality].ivoa_waveband:gamma-raysource · IVOA Registryconnector:ivoa_registry@1.0.0
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