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Unified Models and Emission Mechanisms in Active Galactic Nuclei and Gamma-Ray Bursts

This work explores unified models for radio-loud Active Galactic Nuclei (AGN) and the structure of accretion disks as studied by notable researchers such as Urry, Padovani, and Shakura. It discusses the physics behind accretion disk spectra, black hole growth, and the relationship between black hole mass functions and relativistic phenomena, including iron lines. Additionally, it examines the highest redshift AGN, gamma-ray bursts, their emission mechanisms, and their importance as probes of high redshift galaxies, incorporating works from Madau, Fan, and Ghisellini.

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Unified Models and Emission Mechanisms in Active Galactic Nuclei and Gamma-Ray Bursts

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  1. Tesine AAE 2009 AGN: Unified models for radio loud AGN, Urry & Padovani 1995 Accretion disk structure, Shakura & Sunyaev 1976, Pringle 1981 Accretion disk spectra, Haardt & Maraschi 1991, 1993 BH growth, BH mass function, Marconi 2004, Merloni 2009 Relativistic iron lines Fabian2000, Fabian Miniutti 2005 etc The highest redshift AGN and the first BH, Madau 2001, Fan 2006, etc Panchromatic view of AGN Risaliti 2004 GRB: Emission mechanisms Piran 2004, Ghisellini 2001 GRB as probes of high redshift galaxies Ghisellini 2001, Savaglio 2009 Pulsars: Emission mechanisms, Energetics. Condon, Kujipers Population Condon, Kujipers

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