papers

Publications (18)

astro-ph.HE2021

GeV-radio correlation in Markarian 421

Vitalii Sliusar, Roland Walter, Matteo Balbo

Markarian 421 (Mrk 421) is a high-synchrotron-peaked blazar showing relentless variability across the electromagnetic spectrum from radio to gamma-rays. We use over 7-years of radi…

astro-ph.HE2021

Long-term multi-band photometric monitoring of Mrk 501

Axel Arbet-Engels, Dominik Baack, Matteo Balbo +18

Radio-to-TeV observations of the bright nearby (z=0.034) blazar Markarian 501 (Mrk 501), performed from December 2012 to April 2018, are used to study the emission mechanisms in it…

astro-ph.HE2021

Radioray response in blazars as a signature of adiabatic blob expansion

Andrea Tramacere, Vitalii Sliusar, Roland Walter +2

Multiwavelength light curves in long-term campaigns have shown that, for several blazars, the radio emission occurs with a significant delay w.r.t. to -ray band, with timescale…

astro-ph.HE2022

Rapid X-ray Variability in Mkn 421 during a Multiwavelength Campaign

Alex G. Markowitz, Krzysztof Nalewajko, Gopal Bhatta +47

The study of short-term variability properties in AGN jets has the potential to shed light on their particle acceleration and emission mechanisms. We report results from a four-day…

astro-ph.HE2019

5.5 years multi-wavelength variability of Mrk 421: evidences of leptonic emission from the radio to TeV

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +25

Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use the longest and densest ongoing unbiased observing campaign obtained at TeV…

astro-ph.HE2016

First Study of Combined Blazar Light Curves with FACT and HAWC

Daniela Dorner, Robert J. Lauer, : +28

For studying variable sources like blazars, it is crucial to achieve unbiased monitoring, either with dedicated telescopes in pointing mode or survey instruments. At TeV energies,…

astro-ph.HE2017

Fermi acceleration under control: Carinae

Roland Walter, Matteo Balbo, Christos Panagiotou

We used data from the Fermi Large Area Telescope obtained during the last 7 years and spanning two passages of Carinae at periastron and compared them with the predictions of…

astro-ph.HE2021

Relentless multi-wavelength variability of Mrk 421 and Mrk 501

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +18

Mrk 421 and Mrk 501 are two close, bright and well-studied high-synchrotron-peaked blazars, which feature bright and persistent GeV and TeV emission. We use the longest and densest…

astro-ph.HE2017

Fermi acceleration along the orbit of η Carinae

Matteo Balbo, Roland Walter

The η Carinae binary system hosts the most massive stars with the highest known mass-loss rate. Its dense wind encounters the faster wind expelled by the companion, dissipating me…

astro-ph.HE2022

Observation of the galactic PeVatron candidate LHAASO J2108+5157 with the Large-Sized Telescope for Cherenkov Telescope Array

Jakub Juryšek, Matteo Balbo, Dominique Eckert +3

The Cherenkov Telescope Array (CTA) Observatory will be the next-generation ground-based very-high-energy gamma-ray observatory, sensitive from 20 GeV up to 300 TeV. The Large-Size…

astro-ph.IM2019

Calibration and operation of SiPM-based cameras for gamma-ray astronomy in presence of high night-sky light

Imen Al Samarai, Cyril Martin Alispach, Matteo Balbo +56

The next generation of Cherenkov telescope cameras feature Silicon Photo Multipliers (SiPM), which can guarantee excellent performance and allow for observation also under moonligh…

astro-ph.HE2021

Statistical properties of flux variations in blazar light curves at GeV and TeV energies

Sarah M. Wagner, Paul R. Burd, Daniela Dorner +23

Despite numerous detections of individual flares, the physical origin of the rapid variability observed from blazars remains uncertain. Using Bayesian blocks and the Eisenstein-Hut…

astro-ph.HE2018

Carinae: particle acceleration and multi-messenger aspects

Roland Walter, Matteo Balbo

Carinae is composed of two very massive stars orbiting each other in 5.5 years. The primary star features the densest known stellar wind, colliding with that expelled by its c…

astro-ph.HE2019

Gamma-rays and positrons from Colliding Wind Binaries

Matteo Balbo, Roland Walter

The Carinae binary system is the first -ray binary ever observed which does not contain a compact object. The dense wind of the primary star shocks against the fast light…

astro-ph.HE2024

Chasing Gravitational Waves with the Cherenkov Telescope Array

Jarred Gershon Green, Alessandro Carosi, Lara Nava +563

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts…

astro-ph.HE2021

The relentless variability of Mrk 421 from the TeV to the radio

Axel Arbet-Engels, Dominik Baack, Matteo Balbo +22

The origin of the gamma-ray emission of the blazar Mrk 421 is still a matter of debate. We used 5.5 years of unbiased observing campaign data, obtained using the FACT telescope and…

astro-ph.HE2019

FACT -- Multi-wavelength analysis of more than 30 flares of Mrk 421

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +22

Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use multi-wavelength light curves of Mrk 421 spanning 5.5 years with FACT (TeV)…

astro-ph.HE2019

Monte Carlo study of a single SST-1M prototype for the Cherenkov Telescope Array

Jakub Jurysek, Imen Al Samarai, Cyril Alispach +56

The SST-1M telescope was developed as a prototype of a Small-Size-Telescope for the Cherenkov Telescope Array observatory and it has been extensively tested in Krakow since 2017. I…