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Table of contents
1 Introduction
2 Active Galactic Nuclei
2.1 The AGN zoo
2.2 Unied scheme of AGN phenomenon
2.2.1 What denes the observed luminosity?
2.2.2 Radio-loud or radio-quiet?
2.2.3 Orientation eects
2.3 AGN jets
2.3.1 Imaging of jets
2.3.2 Kinematics and structure
2.3.3 High-energy particles in jets
2.3.4 Energy dissipation
2.3.5 Relativistic motions in jets
2.4 Blazars
2.4.1 Doppler boosting
2.4.2 Blazar emission
2.4.3 Blazar sequence
2.4.4 Probing the Universe with blazars
3 Cherenkov gamma-ray astronomy and H.E.S.S. data analysis
3.1 VHE gamma-ray astronomy
3.1.1 Detection of VHE gamma-rays with an IACT
3.1.2 Presently operating IACTs
3.2 H.E.S.S. experiment
3.2.1 Overview
3.2.2 The optical system
3.2.3 The cameras
3.2.4 The trigger system
3.2.5 Data analysis and reconstruction
3.3 Analysis of H.E.S.S. data of 3C 279
3.3.1 The studied source: 3C 279
3.3.2 VHE
3.3.4 Analysis of H.E.S.S. 3C 279 data : June 2018
3.4 Discussion and perspective
4 Modeling of AGN emission: stationary models
4.1 Origin of blazar broad-band emission
4.1.1 Leptonic (SSC and EC) and hadronic models
4.1.2 Blob-in-jet model
4.1.3 Synchrotron emission
4.1.4 Inverse Compton emission
4.1.5 Gamma-gamma pair production
4.1.6 Transformation to observer’s frame
4.2 EBL absorption
5 Modeling of AGN emission: time-dependent approach
5.1 General approach and the kinetic equation
5.1.1 Particle injection
5.1.2 Particle radiative cooling
5.1.3 Particle acceleration
5.1.4 Particle escape
5.2 EMBLEM code
5.2.1 Numerical implementation
5.2.2 Input parameters
5.2.3 Code architecture
5.2.4 Examples of simulated
5.3 Physical modeling of AGN
5.3.1 What causes the observed variability in the VHE-ray regime ?
5.3.2 One-zone models
5.3.3 Multiple-zone models
6 Modeling of a MWL are of Mrk 421
6.1 The studied source: Mrk 421
6.2 Modeling of the low state of the source
6.2.1 Mrk 421 low-state emission: archival data
6.2.2 Mrk 421 low-state emission: physical modeling and discussion
6.3 Observational data set of the February 2010 are of Mrk 421
6.3.1 Archival data
6.3.2 Analysis of Fermi-LAT gamma-ray data
6.4 A general criterion to test one-zone
6.5 Physical modeling of Mrk 421 February 2010
6.5.1 One-zone model
6.5.2 Two-zone model
6.6 Discussion and perspective
7 Preparation of Cherenkov Telescope Array
7.1 CTA project
7.1.1 Overview
7.1.2 Future science with CTA
7.2 Gamma-Ray Cherenkov Telescope: overview and prototyping
7.2.1 Overview
7.2.2 Prototyping
7.3 Gamma-Ray Cherenkov Telescope: performance
7.3.1 Ideal optical performance
7.3.2 Non-ideal optical performance
7.3.3 Modeling of the PSF of the pGCT
7.4 Discussion and perspective
8 Conclusion and perspective
