Multiwavelength Polarization Observations of Mrk 501

Xin Ke Hu, Yu Wei Yu, Jin Zhang, Xiang Gao Wang, Kishore C. Patra, Thomas G. Brink, Wei Kang Zheng, Qi Wang, De Feng Kong, Liang Jun Chen, Ji Wang Zhou, Jia Xin Cao, Ming Xuan Lu, Zi Min Zhou, Yi Ning Wei, Xin Bo Huang, Xing Lin Li, Hao Lou, Ji Rong Mao, En Wei LiangAlexei V. Filippenko

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3 Citations (Scopus)

Abstract

Mrk 501 is a prototypical high-synchrotron-peaked blazar and serves as one of the primary targets for the Imaging X-ray Polarimetry Explorer (IXPE). In this study, we report X-ray polarization measurements of Mrk 501 based on six IXPE observations. The detection of X-ray polarization at a confidence level exceeding 99% is achieved in four out of the six observations conducted across the entire energy range (2-8 keV) of IXPE. The maximum polarization degree (ΠX) is measured to be 15.8% ± 2.8%, accompanied by a polarization angle (ψ X) of 98.°0 ± 5.°1 at a confidence level of 5.6σ. During the remaining two observations, only an upper limit of ΠX < 12% could be derived at the 99% confidence level. No temporal variability in polarization is observed throughout all six IXPE observations for Mrk 501. A discernible trend of energy-dependent variation in the polarization degree is detected in optical spectropolarimetry; however, no analogous indication is observed in ΠX. The chromatic behavior of Π and the consistent values of ψ across different frequencies from X-ray to radio bands, along with the agreement between ψ and jet position angle, strongly support the interpretation of the energy-stratified model with shock-accelerated particles in the jet of Mrk 501. Additionally, the possibility of the presence of a global helical magnetic field in the jet of Mrk 501 is discussed.

Original languageEnglish
Article numberL22
JournalAstrophysical Journal Letters
Volume970
Issue number1
DOIs
Publication statusPublished - 1 Jul 2024

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