Study of the variable broadband emission of Markarian 501 during the most extreme Swift X-ray activity

[Context] Markarian 501 (Mrk 501) is a very high-energy (VHE) gamma-ray blazar located at z = 0:034, which is regularly monitored by a wide range of multi-wavelength instruments, from radio to VHE gamma rays. During a period of almost two weeks in July 2014, the highest X-ray activity of Mrk 501 was...

Descripción completa

Detalles Bibliográficos
Autores: Acciari, Victor, Font, Lluís, Galindo, David, Gaug, Markus, Maggio, C., Molina, E., Moreno, Vicente, Munar-Adrover, P., Paredes, Josep M., Ribó, Marc, Torres-Albà, N., MAGIC Collaboration, FACT Collaboration
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/233660
Acceso en línea:http://hdl.handle.net/10261/233660
Access Level:acceso abierto
Palabra clave:BL Lacertae objects: individual: Mrk 501
Galaxies: active
Gamma rays: galaxies
X-ray galaxies
Descripción
Sumario:[Context] Markarian 501 (Mrk 501) is a very high-energy (VHE) gamma-ray blazar located at z = 0:034, which is regularly monitored by a wide range of multi-wavelength instruments, from radio to VHE gamma rays. During a period of almost two weeks in July 2014, the highest X-ray activity of Mrk 501 was observed in -14 years of operation of the Neil Gehrels Swift Gamma-ray Burst Observatory.

Similares en LA Referencia