JPL Home NASA Home Caltech Home
Follow this link to skip to the main content
NASA Logo - Jet Propulsion Laboratory   + View the NASA Portal
Search JPL
JPL Home Earth Solar System Stars & Galaxies Technology
Science Visitor and Colloquium Program
SVCP Home
Meetings
Information for Visitors
Contact
Restricted
 
Astrophysics Colloquium

Optical Polarization Variability in Blazars
Presented by Vasiliki Pavlidou
University of Crete

Wednesday, September 2, 2015
2:00 P.M. in 169-336

Abstract
RoboPol is the first monitoring program of an unbiased sample of gamma-ray bright braziers, specifically designed for the effective detection and robust statistics of polarization swings in blazar synchrotron emission at optical wavelengths. Since the launch of the Fermi satellite, it has been suggested that such events may be physically connected with periods of high gamma-ray activity in blazars. Alternatively, the polarization variability in blazars may be erratic, and polarization swings may be produced by chance in an underlying random walk of the polarization vector. We discuss results of the first season of RoboPol monitoring, and how they weigh in on these questions. Some highlights from our findings are: 1 )It is highly unlikely (at the >4sigma level) that none of the rotations observed by RoboPol is physically connected with gamma ray flares. 2) We find indications that more than one mechanisms may be responsible for polarization swings. 3) Blazars with detected rotations have significantly different polarization variability properties than blazars that have never exhibited a rotation.

JPL Contact: Harold Yorke (4-5515)


SVCP Astrophysics


Privacy / Copyrights
  NASA Home Page
Site Manager:
Webmaster:

CL 08-3220