The optical to near-infrared emission of BL Lac objects - Simultaneous observations

Astronomy and Astrophysics – Astronomy

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Bl Lacertae Objects, Blazars, Elliptical Galaxies, Infrared Astronomy, Near Infrared Radiation, Visual Observation, Active Galactic Nuclei, Energy Sources, Thermal Emission

Scientific paper

We present simultaneous optical to NIR observations of 34 blazars, most of which classical BL Lacertae objects, with repeated observations for 21 of them. The observations cover a period of three years with a typical time interval of six months. With the sole exception of PKS 2208-137, all observed optical to NIR flux distributions can be described either by a single power law or by a power law plus the contribution of a standard elliptical galaxy. The optical and NIR emission are strongly correlated and usually maintain the spectral index even under substantial flux variations. The average spectral index of the nonthermal emission, in the range 8 x 10 exp 13 to 7 x 10 exp 14 Hz, is 1.08 +/- 0.06 with significantly flatter spectra for the X-ray-selected subsample.

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