Multiwavelength Intraday Variability of the BL Lac S5 0716+714

TL;DR

This study presents a multi-wavelength observational campaign of BL Lac S5 0716+714, revealing intraday variability, time lags, and possible quasi-periodic oscillations, with insights into the source's emission mechanisms and relativistic effects.

Contribution

First simultaneous multi-wavelength monitoring of S5 0716+714 capturing variability patterns and constraining jet physics and Doppler boosting factors.

Findings

Radio intra-day variability with time lags suggests intrinsic and scintillation contributions.

Optical large amplitude variations and possible quasi-periodic oscillations observed.

X-ray data show no significant short-term variability, favoring inverse-Compton processes.

Abstract

We report results from a 1 week multi-wavelength campaign to monitor the BL Lac object S5 0716+714 (on December 9-16, 2009). In the radio bands the source shows rapid (~ (0.5-1.5) day) intra-day variability with peak amplitudes of up to ~ 10 %. The variability at 2.8 cm leads by about 1 day the variability at 6 cm and 11 cm. This time lag and more rapid variations suggests an intrinsic contribution to the source's intraday variability at 2.8 cm, while at 6 cm and 11 cm interstellar scintillation (ISS) seems to predominate. Large and quasi-sinusoidal variations of ~ 0.8 mag were detected in the V, R and I-bands. The X-ray data (0.2-10 keV) do not reveal significant variability on a 4 day time scale, favoring reprocessed inverse-Compton over synchrotron radiation in this band. The characteristic variability time scales in radio and optical bands are similar. A quasi-periodic variation (QPO) of 0.9 - 1.1 days in the optical data may be present, but if so it is marginal and limited to 2.2 cycles. Cross-correlations between radio and optical are discussed. The lack of a strong radio-optical correlation indicates different physical causes of variability (ISS at long radio wavelengths, source intrinsic origin in the optical), and is consistent with a high jet opacity and a compact synchrotron component peaking at ~= 100 GHz in an ongoing very prominent flux density outburst. For the campaign period, we construct a quasi-simultaneous spectral energy distribution (SED), including gamma-ray data from the FERMI satellite. We obtain lower limits for the relativistic Doppler-boosting of delta >= 12-26, which for a BL\,Lac type object, is remarkably high.