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Plantilla para la elaboración del trabajo escrito del curso IE0499 - Proyecto Eléctrico. Incluye explicación sobre los contenidos del trabajo y sobre el uso de LaTeX en general.
Nota sobre esta versión: los contenidos del documento son solo de referencia y no están en su versión final, así que existen errores o inconsistencias. Para la elaboración de su proyecto puede borrar estos archivos.
Classe de documento padrão para a Dissertação do Mestrado Profissional em Computação Aplicada do Departamento de Ciência da Computação & Engenharia de Produção / Universidade de Brasília.
GitHub: https://github.com/UnB-CIC/Monografia
Versão: 28 de Dezembro de 2016.
Atualizado por: Eliézer H. Silva - Mestrando do Programa PPCA/MPCA.
Blazars are a type of Active Galactic Nucleus (AGN), characterized by the emission of a relativistic jet that points close to our line of sight. They are extremely powerful, variable emitters from radio to gamma-ray wavelengths. By cross-correlating light-curves from different energies, it is possible to determine the physical condition of the blazar emitting region, i.e. mechanism, morphology, distance from block hole to the actual emission, etc. In 2007, the 40m telescope at the Owens Valley Radio Observatory (OVRO) embarked on a new research campaign. In support of the Fermi Gamma-ray Space Telescope, the OVRO 40m telescope is monitoring more than 1800 blazars twice per week. In 2014, a new Ku-band spectropolarimeter receiver, KuPol, was installed on the 40m telescope with the aim of elucidating about potential spectral fluctuations that may arise during the flaring events. In this poster, we will present relevant information and preliminar results from KuPol and the actual status of its calibration, and also as well as the current state of the PSD analysis, where we are applying Fourier Transform to the signals.