Speaker
Jose Rodrigo Sacahui Reyes
(Universidad de San Carlos de Guatemala)
Description
Blazars are the most luminous extrgalactic gamma ray sources. They are a type of Active Galactic Nuclei which are powered by material falling onto a supermassive black hole at the center of the host galaxy. They show sporadic bursts of activity with different time range. In this talk we present a 10 year data analysis of a sample of bright blazars detected by Fermi-LAT (0.1-300 GeV), in particular we present the Duty Cycle -the fraction of time that the source spends in active phase- for the sample. Also we present the consistence of this sample with the so called "blazar sequence" and how this analysis constrains possible counterpart of neutrino emission.
Authors
Jose Rodrigo Sacahui Reyes
(Universidad de San Carlos de Guatemala)
Dr
Antonio Marinelli
(Instituto Nazionale di Fisica Nucleare, Sezione di Napoli, Italy)
Dr
Ana Penacchioni
(Instituto de Física de La Plata (IFLP), La Plata, Argentina.)
Dr
Ankur Sharma
(Dept. of Physics and Astronomy, Uppsala University, Sweden)
Dr
Manuel Castro
(Instituto Nacional de Pesquisas Espaciais (INPE)- Divisão de Astrofı́sica, Brazil.)
Mrs
Osorio Mabel
(Instituto de Astronomía, UNAM. México)
Mr
Marco Antonio Morales
(Instituto Balseiro, Universidad Nacional de Cuyo, Argentina)
