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dc.date.accessioned 2024-07-22T17:23:22Z
dc.date.available 2024-07-22T17:23:22Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/168052
dc.description.abstract We present results from an optical polarimetric study of blazars that have been detected at very high-energy (VHE) -γ rays. We look for short time-scale fluctuations (i.e., microvariability) either/both in their polarisation percent or position angle in the B and R optical bands. Spurious effects introduced by light contamination from the host galaxy, especially due to seeing FWHM variations, are quantitatively analysed. en
dc.format.extent 129-132 es
dc.language en es
dc.subject blazars es
dc.subject optical polarimetric study es
dc.title Optical polarimetry of blazars detected at TeV γ-rays en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-3-4 es
sedici.creator.person Cellone, Sergio Aldo es
sedici.creator.person Combi, Jorge Ariel es
sedici.creator.person Andruchow, Ileana es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Martí, Javier Guillermo 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


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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)