In a previous paper, we proposed a new method to select low-power BL Lacs (LPBLs) based on mid-infrared emission and flux contrast through the Ca II spectral break; that study led to the selection of a complete sample formed by 34 LPBLs with 0.05 <z ≤ 0.15 and radio luminosities spanning the range log Lr = 39.2–41.5 [erg s-1]. We now assemble the broadband spectral energy distributions (SEDs) of these sources to investigate their nature and compare them with brighter BL Lacs. We find that the ratios between the X-ray and radio luminosities range from ~20 to ~30 000 and that the synchrotron peak frequencies span a wide energy interval, from log νpeak ~ 13.5 to ~20 [Hz]. This indicates a broad variety of SED shapes and a mixture of BL Lac fl...
This thesis is an analysis of the X-ray, optical, infrared and radio properties of a sample of c...
Context. The γ-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT det...
Context. BL Lacertae objects with an extremely low value of the peak frequency ($\nu_{\rm s}$ ≤ 1013...
We have collected a large amount of multifrequency data for the objects in the Metsahovi Radio Obser...
We analyse a group of radio sources, a subset of the 200 mJy sample, all of which have core-jet radi...
We have collected a large amount of multifrequency data for objects in the Metsähovi Radio Observat...
© Pleiades Publishing, Ltd., 2015. We study the synchrotron component of nonthermal radiation of bla...
Observations at millimetre wavelengths are presented for a representative sample of 22 X-ray-selecte...
We collect data at well-sampled frequencies from the radio to the gamma-ray range for the following ...
Among active galactic nuclei, BL Lac objects show extreme properties that have been interpreted as t...
This paper discusses the spectral energy distribution (SED) of all blazars with redshift detected by...
ROSAT data as well as archival radio and optical data are used for a broad band study of a large gro...
We discuss alternative interpretations of the differences in the spectral energy distributions (SEDs...
We present a spectral catalog for blazars based on the BeppoSAX archive. The sample includes 44 High...
Many properties of BL Lacs have become explicable in terms of the "relativistic beaming" hypothesis ...
This thesis is an analysis of the X-ray, optical, infrared and radio properties of a sample of c...
Context. The γ-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT det...
Context. BL Lacertae objects with an extremely low value of the peak frequency ($\nu_{\rm s}$ ≤ 1013...
We have collected a large amount of multifrequency data for the objects in the Metsahovi Radio Obser...
We analyse a group of radio sources, a subset of the 200 mJy sample, all of which have core-jet radi...
We have collected a large amount of multifrequency data for objects in the Metsähovi Radio Observat...
© Pleiades Publishing, Ltd., 2015. We study the synchrotron component of nonthermal radiation of bla...
Observations at millimetre wavelengths are presented for a representative sample of 22 X-ray-selecte...
We collect data at well-sampled frequencies from the radio to the gamma-ray range for the following ...
Among active galactic nuclei, BL Lac objects show extreme properties that have been interpreted as t...
This paper discusses the spectral energy distribution (SED) of all blazars with redshift detected by...
ROSAT data as well as archival radio and optical data are used for a broad band study of a large gro...
We discuss alternative interpretations of the differences in the spectral energy distributions (SEDs...
We present a spectral catalog for blazars based on the BeppoSAX archive. The sample includes 44 High...
Many properties of BL Lacs have become explicable in terms of the "relativistic beaming" hypothesis ...
This thesis is an analysis of the X-ray, optical, infrared and radio properties of a sample of c...
Context. The γ-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT det...
Context. BL Lacertae objects with an extremely low value of the peak frequency ($\nu_{\rm s}$ ≤ 1013...