TY - JOUR
T1 - X-Ray Polarization of the High-synchrotron-peaked BL Lac H 1426+428
AU - Hu, Xin Ke
AU - Li, Jia Xuan
AU - Yu, Yu Wei
AU - Lian, Ji Shun
AU - Deng, Wei
AU - Zhang, Hai Ming
AU - Zhang, Jin
N1 - Publisher Copyright:
© 2025. The Author(s). Published by the American Astronomical Society.
PY - 2025/6/20
Y1 - 2025/6/20
N2 - We report the X-ray polarization properties of the high-synchrotron-peaked BL Lac H 1426+428, based on two-epoch observational data from the Imaging X-ray Polarimetry Explorer (IXPE). For the first observation, only an upper limit of polarization degree (ΠX), ΠX < 19.5%, at the 99% confidence level (CL) is determined. In contrast, for the second observation, we derive ΠX = 20.6% ± 2.9% with a polarization angle (ψX) of ψX = 116 . ° 1 ± 4 . ° 1 at a CL of 7.1σ. The time-resolved and energy-resolved polarization analysis reveals no significant variation in ψX and no detectable polarization within narrower energy bins for the first observation, while the polarization during the second observation is dominated by low-energy photons. Furthermore, the X-rays during the second observation are found to be in a higher flux state with a harder spectrum compared to that observed during the first observation, consistent with a harder-when-brighter behavior. We propose that the enhanced X-ray emission observed during the second observation is produced by shock-accelerated electrons within an ordered magnetic field region via synchrotron radiation. Nonetheless, no significant detection of polarization during the first IXPE observation may be due to the limited number of detected photons.
AB - We report the X-ray polarization properties of the high-synchrotron-peaked BL Lac H 1426+428, based on two-epoch observational data from the Imaging X-ray Polarimetry Explorer (IXPE). For the first observation, only an upper limit of polarization degree (ΠX), ΠX < 19.5%, at the 99% confidence level (CL) is determined. In contrast, for the second observation, we derive ΠX = 20.6% ± 2.9% with a polarization angle (ψX) of ψX = 116 . ° 1 ± 4 . ° 1 at a CL of 7.1σ. The time-resolved and energy-resolved polarization analysis reveals no significant variation in ψX and no detectable polarization within narrower energy bins for the first observation, while the polarization during the second observation is dominated by low-energy photons. Furthermore, the X-rays during the second observation are found to be in a higher flux state with a harder spectrum compared to that observed during the first observation, consistent with a harder-when-brighter behavior. We propose that the enhanced X-ray emission observed during the second observation is produced by shock-accelerated electrons within an ordered magnetic field region via synchrotron radiation. Nonetheless, no significant detection of polarization during the first IXPE observation may be due to the limited number of detected photons.
UR - https://www.scopus.com/pages/publications/105009291943
U2 - 10.3847/1538-4357/add87d
DO - 10.3847/1538-4357/add87d
M3 - Article
AN - SCOPUS:105009291943
SN - 0004-637X
VL - 986
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 182
ER -