Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2024-07-08T14:29:33Z
dc.date.available 2024-07-08T14:29:33Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167851
dc.description.abstract The High Energy Stereoscopic System (H.E.S.S.) is the world’s largest currently operating Atmospheric Cherenkov Telescope Array. This paper presents highlights of recent results from H.E.S.S. observations of extragalactic jet sources. It will focus on variability studies of the wellknown blazars Mrk 501 (discovering minute-scale variability at energies > 2 TeV) and PKS 2155-304, the multiwavelength analysis of the recently discovered blazar PKS 1440-389, and observations of the gravitationally lensed blazar PKS 1830-211, including a brief discussion of the implications of its non-detection by H.E.S.S. en
dc.format.extent 37-42 es
dc.language en es
dc.subject High Energy Stereoscopic System es
dc.subject extragalactic jet sources es
dc.title H.E.S.S. Observations of Extragalactic Jet Sources en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-3-4 es
sedici.creator.person Böttcher, Markus es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Objeto de conferencia es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.date.exposure 2015-10
sedici.relation.event High-Energy Phenomena tn Relativistic Outflows V (La Plata, 5 al 8 de octubre de 2015) es
sedici.description.peerReview peer-review es
sedici.relation.isRelatedWith https://sedici.unlp.edu.ar/handle/10915/167830 es
sedici.relation.bookTitle Proceedings of the High-Energy Phenomena in Relativistic Outflows V meeting es


Descargar archivos

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)