Testing the blazar sequence with the least luminous BL Lacs
Claudia M. Raiteri, Alessandro Capetti

TL;DR
This study investigates the spectral energy distributions of low-power BL Lac objects, revealing a broad variety of shapes and challenging the traditional blazar sequence, especially at low radio luminosities.
Contribution
The paper presents a new method for selecting low-power BL Lacs and provides the first comprehensive SED analysis of these sources, questioning the role of radio power in their properties.
Findings
Wide range of synchrotron peak frequencies (log(nu_peak)~13.5 to ~20 Hz).
Majority are high-energy peaked BL Lacs, but a significant fraction are LBLs.
Disagreement with the blazar sequence at low radio luminosities.
Abstract
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(L_r) = 39.2-41.5 [erg/s]. 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 ~30000 and that the synchrotron peak frequencies span a wide energy interval, from log(nu_peak)~13.5 to ~20 [Hz]. This indicates a broad variety of SED shapes and a mixture of BL Lac flavors. Indeed, although the majority of our LPBLs are high-energy peaked BL Lacs (HBLs), we find that a quarter of them are low-energy peaked BL Lacs…
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