papers

Publications (32)

astro-ph.HE2021

The Blazar Hadronic Code Comparison Project

Matteo Cerruti, Michael Kreter, Maria Petropoulou +15

Blazar hadronic models have been developed in the past decades as an alternative to leptonic ones. In hadronic models the gamma-ray emission is associated with synchrotron emission…

astro-ph2006

Recent results from the Pierre Auger Observatory

Andreas Zech

The goal of the Pierre Auger Observatory is to determine the still unknown nature and origin of ultra-high energy cosmic rays. The study of these elusive particles probes astrophys…

astro-ph.HE2017

Gammapy: high level data analysis for extragalactic science cases with the Cherenkov Telescope Array

Julien Lefaucheur, Catherine Boisson, Zeljka Bosnjak +5

The Cherenkov Telescope Array (CTA) observatory will probe the non-thermal universe above 20 GeV up to several hundreds of TeV with a significant improvement in sensitivity and ang…

astro-ph.HE2026

Blazar flares from plasma blobs crossing the broad-line region

Sébastien Le Bihan, Anton Dmytriiev, Andreas Zech

The blazar 3C 279 is well known for its rapid and large-amplitude variability. On 20 December 2013, the source exhibited an orphan γ-ray flare characterized by a flux-doubling tim…

astro-ph.HE2025

An orphan flare from a plasma blob crossing the broad-line region ?

Sébastien Le Bihan, Anton Dmytriiev, Andreas Zech

The blazar 3C 279 is well known for its prolific emission of rapid flares. A particular event occurred on 12/20/2013, exhibiting a large flux increase with a doubling time scale of…

astro-ph.HE2023

The variety of extreme blazars in the AstroSat view

Pranjupriya Goswami, Michael Zacharias, Andreas Zech +3

Extreme blazars have exceptionally hard intrinsic X-ray/TeV spectra and extreme peak energies in their spectral energy distribution (SED). Observational evidence suggests that the…

astro-ph.HE2023

ExHaLe-jet: Modeling blazar jets with an extended hadro-leptonic radiation code

Michael Zacharias, Anita Reimer, Catherine Boisson +1

Blazars emit across all electromagnetic wavelengths. While the so-called one-zone model has described well both quiescent and flaring states, it cannot explain the radio emission a…

astro-ph.HE2012

A mixed lepto-hadronic scenario for PKS 2155-304

Matteo Cerruti, Andreas Zech, Catherine Boisson +1

The models developed to describe the spectral energy distribution (SED) of blazars can be divided into leptonic or hadronic scenarios, according to the particles responsible for th…

astro-ph.HE2026

Particle acceleration signatures in the time-dependent one-zone synchrotron self-Compton model of blazar flares

Paloma Thevenet, Andreas Zech, Catherine Boisson +1

The study of multiwavelength flux and spectral variations during rapid flares from blazars provides strong constraints on the physical parameters of the compact emission regions re…

astro-ph.HE2019

H.E.S.S. searches for TeV gamma rays associated to high-energy neutrinos

Fabian Schüssler, Halim Ashkar, Michael Backes +12

The detection of an astrophysical flux of high-energy neutrinos by IceCube is a major step forward in the search for the origin of cosmic rays, as this emission is expected to orig…

astro-ph.HE2019

The Giant Radio Array for Neutrino Detection (GRAND): Science and Design

GRAND Collaboration, Jaime Alvarez-Muniz, Rafael Alves Batista +48

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10^8 GeV. Its goal is…

astro-ph.HE2017

Expected signatures from hadronic emission processes in the TeV spectra of BL Lac objects

Andreas Zech, Matteo Cerruti, Daniel Mazin

The wealth of recent data from imaging air Cherenkov telescopes (IACTs), ultra-high energy cosmic-ray experiments and neutrino telescopes have fuelled a renewed interest in hadroni…

astro-ph.HE2014

Equipartition Gamma-Ray Blazars and the Location of the Gamma-Ray Emission Site in 3C 279

Charles D. Dermer, Matteo Cerruti, Benoit Lott +2

Blazar spectral models generally have numerous unconstrained parameters, leading to ambiguous values for physical properties like Doppler factor delta or fluid magnetic field B'. T…

astro-ph.HE2023

Modelling the variable emission states of -ray emitting Narrow-Line Seyfert 1 galaxies

Anna Luashvili, Catherine Boisson, Andreas Zech +2

-ray-emitting narrow-line Seyfert 1 galaxies (-NLS1) constitute an intriguing small population of Active Galactic Nuclei with -ray emission resembling low power flat-sp…

astro-ph.GA2017

The relativistic jet of the gamma-ray emitting narrow-line Seyfert 1 galaxy 1H 0323+342

Daniel Kynoch, Hermine Landt, Martin J. Ward +7

The detection of several radio-loud narrow-line Seyfert 1 (NLS1) galaxies by the Fermi Gamma-Ray Space Telescope hints at the existence of a rare, new class of gamma-ray emitting a…

astro-ph.IM2015

Monte Carlo Studies of the GCT Telescope for the Cherenkov Telescope Array

Thomas Armstrong, Heide Costantini, Cameron Rulten +2

The GCT is an innovative dual-mirror solution proposed for the small-size telescopes for CTA, capable of imaging primary cosmic gamma-rays from below a TeV to hundreds of TeV. The…

astro-ph.HE2021

Flux variability from ejectas in structured relativistic jets with large-scale magnetic fields

Gaëtan Fichet de Clairfontaine, Zakaria Meliani, Andreas Zech +1

Using the relativistic MHD code MPI-AMRVAC and a radiative transfer code in post-processing, we explore the influence of the magnetic-field configuration and transverse stratificat…

astro-ph.HE2020

Progress in unveiling extreme particle acceleration in persistent astrophysical jets

Jonathan Biteau, Elisa Prandini, Luigi Costamante +7

The most powerful persistent accelerators in the Universe are jetted active galaxies. Blazars, galaxies whose jets are directed towards Earth, dominate the extragalactic gamma-ray…

astro-ph.HE2019

News from the very-high-energy sky seen with H.E.S.S

Andreas Zech, H. E. S. S. Collaboration

The H.E.S.S. experiment, the largest Cherenkov telescope array to date, has been observing the sky at TeV energies for the past 16 years. Its location in the Southern hemisphere pr…

astro-ph2005

Studies of Systematic Uncertainties in the HiRes-II Measurement of the UHECR Spectrum

Andreas Zech

We present studies of systematic uncertainties in the measurement of the ultra-high energy cosmic ray (UHECR) spectrum with the FADC detector of the High Resolution Fly's Eye exper…

astro-ph.HE2013

Constraining the parameter space of the one-zone synchrotron-self-Compton model for GeV-TeV detected BL Lac objects

Matteo Cerruti, Catherine Boisson, Andreas Zech

The one-zone synchrotron-self-Compton (SSC) model aims to describe the spectral energy distribution (SED) of BL Lac objects via synchrotron emission by a non-thermal population of…

astro-ph2004

A Measurement of the UHECR Spectrum with the HiRes FADC Detector

Andreas Zech

We have measured the energy spectrum of ultra-high energy cosmic rays (UHECR) with the HiRes FADC detector (HiRes-2) in monocular mode. A detailed Monte Carlo simulation of the det…

astro-ph.HE2021

Electron-proton co-acceleration on relativistic shocks in extreme-TeV blazars

Andreas Zech, Martin Lemoine

The multi-wavelength emission from a newly identified population of `extreme-TeV' blazars, with Compton peak frequencies around 1 TeV, is difficult to interpret with standard one-z…

astro-ph.HE2013

Gamma-ray blazars near equipartition and the origin of the GeV spectral break in 3C 454.3

Matteo Cerruti, Charles D. Dermer, Benoit Lott +2

Observations performed with the Fermi-LAT telescope have revealed the presence of a spectral break in the GeV spectrum of flat-spectrum radio quasars (FSRQs) and other low- and int…

astro-ph.HE2022

Flare echos from relaxation shocks in perturbed relativistic jets

Gaëtan Fichet de Clairfontaine, Zakaria Meliani, Andreas Zech

One of the main scenarios to account for the multi-wavelength flux variability observed in relativistic jets of AGNs is based on diffusive shock acceleration of a population of rel…

astro-ph.IM2017

The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives

Ke Fang, Jaime Álvarez-Muñiz, Rafael Alves Batista +33

The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau lepton…

astro-ph.HE2022

ExHaLe-jet: An extended hadro-leptonic jet model for blazars. I. Code description and initial results

Michael Zacharias, Anita Reimer, Catherine Boisson +1

The processes operating in blazar jets are still an open question. Modeling the radiation emanating from an extended part of the jet allows one to capture these processes on all sc…

astro-ph.HE2021

The imprint of protons on the emission of extended blazar jets

Michael Zacharias, Anita Reimer, Andreas Zech

Blazars - active galaxies with the jet pointing at Earth - emit across all electromagnetic wavelengths. The so-called one-zone model has described well both quiescent and flaring s…

astro-ph.HE2022

Blazars at Very High Energies: Emission Modelling

Hélène Sol, Andreas Zech

Blazars are very broadband cosmic sources with spectra spanning over twenty orders of magnitude in frequency, down to the 100 MHz regime in the radio range, up to VHE at several te…

astro-ph.CO2011

Lepto-hadronic modelling of blazar emission

Matteo Cerruti, Andreas Zech, Catherine Boisson +1

The characteristic double-bumped spectral energy distribution (SED) of blazars is explained by either leptonic or hadronic models. In the former, Inverse Compton emission dominates…

astro-ph.HE2025

A Comprehensive Hadronic Code Comparison for Active Galactic Nuclei

Matteo Cerruti, Annika Rudolph, Maria Petropoulou +14

We perform the first dedicated comparison of five hadronic codes (AM, ATHEA, B13, LeHa-Paris, and LeHaMoC) that have been extensively used in modeling of the spectral energ…

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…