Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421

Blazars are highly variable and display complex characteristics. A key characteristic is the flux probability distribution function or flux PDF whose shape depends upon the form of the underlying physical process driving variability. The BL Lacertae Mrk 421 is one of the brightest and most variable...

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Main Author: Nachiketa Chakraborty
Format: Article
Language:English
Published: MDPI AG 2020-01-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/1/7
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author Nachiketa Chakraborty
author_facet Nachiketa Chakraborty
author_sort Nachiketa Chakraborty
collection DOAJ
description Blazars are highly variable and display complex characteristics. A key characteristic is the flux probability distribution function or flux PDF whose shape depends upon the form of the underlying physical process driving variability. The BL Lacertae Mrk 421 is one of the brightest and most variable blazars across the electromagnetic spectrum. It has been reported to show hints of lognormality across the spectrum from radio to gamma-ray histograms of observed fluxes. This would imply that the underlying mechanisms may not conform to the “standard” additive, multi-zone picture, but could potentially have multiplicative processes. This is investigated by testing the observed lightcurves at different wavelengths with time-series simulations. We find that the simulations reveal a more complex scenario, than a single lognormal distribution explaining the multiwavelength lightcurves of Mrk 421.
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spelling doaj.art-f481dfd7a3954afdb47eecffe15244582022-12-21T18:53:04ZengMDPI AGGalaxies2075-44342020-01-0181710.3390/galaxies8010007galaxies8010007Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421Nachiketa Chakraborty0Data Assimilation Research Centre, University of Reading, Whiteknights Rd., Reading RG6 6AH, UKBlazars are highly variable and display complex characteristics. A key characteristic is the flux probability distribution function or flux PDF whose shape depends upon the form of the underlying physical process driving variability. The BL Lacertae Mrk 421 is one of the brightest and most variable blazars across the electromagnetic spectrum. It has been reported to show hints of lognormality across the spectrum from radio to gamma-ray histograms of observed fluxes. This would imply that the underlying mechanisms may not conform to the “standard” additive, multi-zone picture, but could potentially have multiplicative processes. This is investigated by testing the observed lightcurves at different wavelengths with time-series simulations. We find that the simulations reveal a more complex scenario, than a single lognormal distribution explaining the multiwavelength lightcurves of Mrk 421.https://www.mdpi.com/2075-4434/8/1/7blazarsvariabilitylognormalitymrk 421
spellingShingle Nachiketa Chakraborty
Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
Galaxies
blazars
variability
lognormality
mrk 421
title Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
title_full Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
title_fullStr Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
title_full_unstemmed Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
title_short Investigating Multiwavelength Lognormality with Simulations—Case of Mrk 421
title_sort investigating multiwavelength lognormality with simulations case of mrk 421
topic blazars
variability
lognormality
mrk 421
url https://www.mdpi.com/2075-4434/8/1/7
work_keys_str_mv AT nachiketachakraborty investigatingmultiwavelengthlognormalitywithsimulationscaseofmrk421