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dc.contributor.authorAngelakis, Emmanouil
dc.contributor.authorBöttcher, Markus
dc.contributor.authorHovatta, Talvikki
dc.contributor.authorKiehlmann, Sebastian
dc.contributor.authorMyserlis, Ioannis
dc.date.accessioned2017-11-02T08:44:55Z
dc.date.available2017-11-02T08:44:55Z
dc.date.issued2016
dc.identifier.citationAngelakis, E. et al. 2016. Robopol: optical polarisation monitoring of blazars. 4th Annual Conference on High Energy Astrophysics in Southern Africa, 25-26 Aug 2016, Cape Town, South Africa. Proceedings of science: Article no 022. [https://pos.sissa.it/275/022/]en_US
dc.identifier.issn1824-8039 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/26008
dc.identifier.urihttps://pos.sissa.it/275/022/
dc.identifier.urihttps://pos.sissa.it/275/022/pdf
dc.description.abstractThe RoboPol program has been monitoring the R-band linear polarisation parameters of an unbiased sample of 60 gamma-ray-loud blazars and a “control” sample of 15 gamma-ray-quite ones. The prime drive for the program has been the systematic study of the temporal behaviour of the optical polarisation and particularly the potential association of smooth and long rotations of the linear polarisation position angle with flaring activity at high energies. Here we present the program and discuss a list of selected topics from our studies of the first three observing seasons (2013–2015) both in the angle and in the amplitude domainen_US
dc.language.isoenen_US
dc.publisherHEASAen_US
dc.titleRobopol: optical polarisation monitoring of blazarsen_US
dc.typePresentationen_US
dc.contributor.researchID24420530 - Böttcher, Markus


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