activity
20082018
most citedThe extreme HBL behaviour of Markarian 501 during 2012

84 citations · 300 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2018★ 84 cited

The extreme HBL behaviour of Markarian 501 during 2012

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +276

A multiwavelength campaign was organized to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC,…

astro-ph.HE2016★ 62 cited

Multifrequency Photo-polarimetric WEBT Observation Campaign on the Blazar S5 0716+714: Source Microvariability and Search for Characteristic Timescales

G. Bhatta, Ł. Stawarz, M. Ostrowski +43

Here we report on the results of the WEBT photo-polarimetric campaign targeting the blazar S5~0716+71, organized in March 2014 to monitor the source simultaneously in BVRI and near…

astro-ph.HE2016★ 2 cited

Polarization angle swings in blazars: The case of 3C 279

S. Kiehlmann, T. Savolainen, S. G. Jorstad +61

Over the past few years, several occasions of large, continuous rotations of the electric vector position angle (EVPA) of linearly polarized optical emission from blazars have been…

astro-ph.HE2015

Flaring activity of Mrk 421 in 2012 and 2013: orphan flare and multiwavelength analysis

Nissim Fraija, José Ignacio Cabrera, Erika Benítez +1

The first one started in 2012 July 16 (MJD 56124) and the second one in 2013 April 9 (MJD 56391). The multiwavelength data analysis shows that the -ray flare observed in 2012 wa…

astro-ph.IM2014★ 16 cited

VAMOS: a Pathfinder for the HAWC Gamma-Ray Observatory

A. U. Abeysekara, R. Alfaro, C. Alvarez +133

VAMOS was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and…

astro-ph.HE2014★ 13 cited

Rotation of the optical polarization angle associated with the 2008 γ-ray flare of blazar w comae

Marco Sorcia, Erika Benítez, David Hiriart +3

An --band photopolarimetric variability analysis of the TeV bright blazar W Comae, between 2008 February 28 and 2013 May 17, is presented. The source showed a gradual tendency t…