Multifrequency monitoring of the blazar 0716+714 during the GASP-WEBT-AGILE campaign of 2007

TL;DR

This paper presents multiwavelength optical, radio, and UV observations of blazar 0716+714 during 2007, highlighting a rare optical-radio outburst and providing data to explore correlations with gamma-ray emissions.

Contribution

It offers the first detailed multiwavelength monitoring of 0716+714 during a gamma-ray detection period, including spectral energy distributions and flare analysis.

Findings

Detected a contemporaneous optical-radio outburst.

Observed a peculiarly wavy spectral energy distribution during the outburst.

Captured prominent and sharp optical flares during AGILE pointings.

Abstract

Since the CGRO operation in 1991-2000, one of the primary unresolved questions about the blazar gamma-ray emission has been its possible correlation with the low-energy (in particular optical) emission. To help answer this problem, the Whole Earth Blazar Telescope (WEBT) consortium has organized the GLAST-AGILE Support Program (GASP) to provide the optical-to-radio monitoring data to be compared with the gamma-ray detections by the AGILE and GLAST satellites. This new WEBT project started in early September 2007, just before a strong gamma-ray detection of 0716+714 by AGILE. We present the GASP-WEBT optical and radio light curves of this blazar obtained in July-November 2007, about various AGILE pointings at the source. We construct NIR-to-UV spectral energy distributions (SEDs), by assembling GASP-WEBT data together with UV data from the Swift ToO observations of late October. We observe a contemporaneous optical-radio outburst, which is a rare and interesting phenomenon in blazars. The shape of the SEDs during the outburst appears peculiarly wavy because of an optical excess and a UV drop-and-rise. The optical light curve is well sampled during the AGILE pointings, showing prominent and sharp flares. A future cross-correlation analysis of the optical and AGILE data will shed light on the expected relationship between these flares and the gamma-ray events.