Spectroscopy of high-energy BL Lacertae objects with X-shooter on the VLT
Résumé
Context. BL Lac objects detected in γ-rays and, particularly,
those detected at very high energies (E > 100 GeV) by Cherenkov
telescopes are extreme sources with most having redshifts lower than 0.2. Their study
gives insights on the acceleration mechanisms in play in such systems and is also a
valuable tool for putting constraints on the density of extragalactic background light,
especially if several objects are detected at different redshifts. As their spectra are
dominated by the non-thermal emission of the jet and the spectral features are weak and
narrow in the optical domain, measuring their redshift is challenging. However, such a
measure is fundamental as it allows a firm determination of the distance and luminosity of
the source, and, therefore, a consistent model of its emission.Aims. Measurement of the redshift of BL Lac objects detected in
γ-rays and
determination of global properties of their host galaxies is the aim of this study.Methods. We observed a sample of eight BL Lac objects with the X-shooter
spectrograph installed at the ESO Very Large Telescope (VLT) to take advantage of its
unprecedented wavelength coverage and its resolution, which is about five times higher
than generally used in such studies. We extracted UVB to NIR spectra that
we then corrected for telluric absorption and calibrated in flux. We systematically
searched for spectral features. When possible, we determined the contribution of the host
galaxy to the overall emission.Results. Of the eight BL Lac sources, we measured the redshift of five
of them and determined lower limits for two through the detection of intervening systems.
All seven of these objects have redshifts greater than 0.2. For the remaining one, we
estimated, using an indirect method, that its redshift is greater than 0.175. In two
cases, we refuted redshift values reported in other publications. Through careful
modelling, we determined the magnitude of the host galaxies. In two cases, the detection
of emission lines allowed to provide hints on the overall properties of the gas in the
host galaxies. Even though we warn that we are dealing with a very small sample, we remark
that the redshift determination efficiency of our campaign is higher than for previous
campaigns. We argue that it is mainly the result of the comparatively higher resolution of
X-shooter.
Origine : Publication financée par une institution
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