Multiwavelength Polarization Observations of Mrk 501
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.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 2024
- DOI:
- 10.3847/2041-8213/ad5e68
- arXiv:
- arXiv:2402.11949
- Bibcode:
- 2024ApJ...970L..22H
- Keywords:
-
- Relativistic jets;
- X-ray active galactic nuclei;
- Active galactic nuclei;
- Blazars;
- Spectropolarimetry;
- 1390;
- 2035;
- 16;
- 164;
- 1973;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 20 pages, 8 figures, 4 tables, accepted for publication in ApJL