Multiband optical polarimetry of the BL Lac object PKS 2155--304. Intranight and long term variability

Abstract

The polarized and total flux of the BL Lac object PKS 2155-304 were monitored intensively and simultaneously in the optical UBVRI bands with the Turin photopolarimeter at the CASLEO 2.15 m telescope during 4 campaigns in June, August, November 1998 and August 1999. The effective observation time amounted to ~47 hours. PKS 2155-304 showed a linear polarization percentage (P) usually ranging between 3% and 7% and a polarization position angle (PA) mainly between 70 and 120 deg. The highest temporal resolution of our observations, 15 minutes, is unprecedented for polarimetric monitoring of this source, and has allowed us to detect amplitude variations of the linear polarization percentage from 6 to 7.5% in time scales of hours. In some nights the polarization percentage seems to increase toward shorter wavelengths, however the polarized spectrum does not vary significantly with time. The most remarkable variability event occurred on 1998 June 18, when the degree of linear polarization decreased by more than a factor 2 in one day in all bands, while the PA rotated by 90 deg. This is consistent with the presence of two emission components, of different polarization degree and position angle. Intranight variability of P and PA can be interpreted with small amplitude physical or geometrical changes within the jet. Measurements of the circular polarization over time intervals of days set upper limits of 0.2%. Simultaneous photometry taken with the Turin Photopolarimeter and with a CCD camera at Cordoba Astronomical Observatory did not show light variations correlated with those of the linearly polarized flux.

21 pages, 6 eps figures. Accepted for The Astrophysical Journal Supplement Series

References in corpus (4)

• Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray-Burst Sources
• Polarization lightcurves and position angle variation of beamed gamma-ray bursts
• The discovery of polarization in the afterglow of GRB 990510 with the ESO Very Large Telescope
• GRB990712: First Indication of Polarization Variability in a Gamma-ray Burst Afterglow

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