Prospects for Detecting X-ray Polarization in Blazar Jets
arXiv:1906.01647 · doi:10.3847/1538-4357/ab2719
Abstract
X-ray polarization should provide new probes of magnetic field geometry and acceleration physics near the base of blazar jets, but near-future missions will have limited sensitivity. We thus use existing lower energy data and X-ray variability measurements in the context of a basic synchro-Compton model to predict the X-ray polarization level and the probability of detection success for individual sources, listing the most attractive candidates for an IXPE campaign. We find that, as expected, several high-peak blazars such as Mrk 421 can be easily measured in 100 ksec exposures. Most low peak sources should only be accessible to triggered campaigns during bright flares. Surprisingly, a few intermediate peak sources can have anomalously high X-ray polarization and thus are attractive targets.
9 pages, 4 figures, published in APJ
References in corpus (12)
- The 5th edition of the Roma-BZCAT. A short presentation
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
- Constraining the limiting brightness temperature and Doppler factors for the largest sample of radio bright blazars
- RoboPol: The optical polarization of gamma-ray--loud and gamma-ray--quiet blazars
- RoboPol: Connection between optical polarization plane rotations and gamma-ray flares in blazars
- Log-normal flux distribution of bright Fermi blazars
- The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration
- Optical EVPA rotations in blazars: testing a stochastic variability model with RoboPol data
- Bimodal radio variability in OVRO-40m-monitored blazars
- The Polarization Behavior of Relativistic Synchrotron Jets
- Flux Distribution of Gamma-Ray Emission in Blazars: The Example of Mrk 501
- The PoGO+ Balloon-Borne Hard X-ray Polarimetry Mission
Cited by in corpus (21)
- Polarized Blazar X-rays imply particle acceleration in shocks
- The X-ray Polarization View of Mrk~421 in an Average Flux State as Observed by the Imaging X-ray Polarimetry Explorer
- Mapping the magnetic field in the solar corona through magnetoseismology
- X-ray Polarization Observations of BL Lacertae
- Magnetic Field Properties inside the Jet of Mrk 421: Multiwavelength Polarimetry Including the Imaging X-ray Polarimetry Explorer
- The Polarization Behavior of Relativistic Synchrotron Self-Compton Jets
- Detection of X-ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-ray Polarimetry Explorer
- Probing shock acceleration in BL Lac jets through X-ray polarimetry: the time-dependent view
- Testing particle acceleration models for BL LAC jets with the Imaging X-ray Polarimetry Explorer
- Hadronic X-ray Flares from Blazars
- High optical to X-ray polarization ratio reveals Compton scattering in BL Lacertae's jet
- IXPE Observation of the Low-Synchrotron Peaked Blazar S4 0954+65 During An Optical-X-ray Flare
- Determining the origin of the X-ray emission in blazars through multiwavelength polarization
- Monte-Carlo Applications for Partially Polarised Inverse External-Compton Scattering (MAPPIES) -- I. Description of the code and First Results
- Quantitative comparisons of VHE gamma-ray blazar flares with relativistic reconnection models
- Testing particle acceleration in blazar jets with continuous high-cadence optical polarization observations
- Spectral Energy Distribution Modeling of BL Lacertae During a Large Submillimeter Outburst and Low X-Ray Polarization State
- X-ray Spectroscopy of Interstellar Carbon: Evidence for Scattering by Carbon-Bearing Material in the Spectrum of 1ES 1553+113
- Testing High-Energy Emission Models for Blazars with X-ray Polarimetry
- Constraints on magnetic field and particle content in blazar jets through optical circular polarization
- Probing Magnetic Fields and Acceleration Mechanisms in Blazar Jets with X-ray Polarimetry