On the origin of the soft photons of the high synchrotron peaked blazar : PKS 1424+240
Shiju Kang (LPSNU), Yong-Gang Zheng (YNNU), Qingwen Wu (HUST), Liang, Chen (SHAO)

TL;DR
This study re-examines the multi-wavelength spectral energy distributions of the blazar PKS 1424+240 using a one-zone leptonic model with a weak external Compton component, revealing a weaker external photon field than in luminous quasars.
Contribution
It demonstrates that a one-zone leptonic model with a weak external photon field can explain the SEDs of PKS 1424+240 without extreme parameters, suggesting a weaker BLR/torus in BL Lacs.
Findings
External photon field energy density is about 3 orders of magnitude less than in luminous quasars.
The magnetic field and Doppler factor are consistent with other BL Lacs.
External Compton scattering may still influence high synchrotron peaked blazars.
Abstract
PKS 1424+240 is a distant very high energy gamma-ray BL Lac object with redshift . It was found that pure synchrotron self-Compton (SSC) process normally need extreme input parameters (e.g., very low magnetic field intensity and extraordinarily large Doppler factor) to explain its multi-wavelength spectral energy distributions (SEDs). To avoid the extreme model parameters, different models have been proposed (e.g., two-zone SSC model or lepto-hadronic model). In this work, we employ the traditional one-zone leptonic model after including a weak external Compton component to re-explore the simultaneous multi-wavelength SEDs of PKS 1424+240 in both high (2009) and low (2013) states. We find that the input parameters of magnetic field and Doppler factor are roughly consistent with those of other BL Lacs if a weak external photon field from either broad line region (BLR) or the…
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