Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
arXiv:1901.08066 · doi:10.1093/mnras/stz377
Abstract
We investigate the previously proposed possibility that multi-epoch broadband polarimetry could act as a complement or limited proxy for VLBI observations of blazars, in that the number of polarised emission components in the jet, and some of their properties and those of the foreground environment, might be inferred from the object's time-varying 1D Faraday depth spectrum (FDS) alone. We report on a pilot-scale experiment designed to establish the basic plausibility and utility of this idea. We analyse temporal changes in the complex polarisation spectra of nine spatially unresolved (at arcsecond scales) blazars in two epochs separated by 5 years, using data taken with the Australia Telescope Compact Array. The data allow for precise modelling, and we demonstrate that all objects in our sample show changes in their polarisation spectrum that cannot be accounted for by uncertainties in calibration or observational effects. By associating polarised emission components across epochs, we infer changes in their number, intrinsic fractional polarisation, intrinsic polarisation angle, rotation measure, and depolarisation characteristics. We attribute these changes to evolution in the structure of the blazar jets, most likely located at distances of up to tens of parsecs from the central active galactic nuclei. Our results suggest that continued work in this area is warranted; in particular, it will be important to determine the frequency ranges and temporal cadence most useful for scientifically exploiting the effects.
12 pages of text, 13 figures, 4 tables (29 pages total). Accepted for publication in MNRAS (Jan 2019)
References in corpus (26)
- CRATES: An All-Sky Survey of Flat-Spectrum Radio Sources
- MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
- Post-correlation radio frequency interference classification methods
- Science With The Australian Square Kilometre Array Pathfinder
- MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VIII. Faraday rotation in parsec-scale AGN jets
- Blazar flares powered by plasmoids in relativistic reconnection
- Calibrating High-Precision Faraday Rotation Measurements for LOFAR and the Next Generation of Low-Frequency Radio Telescopes
- The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey II: The First Four Epochs
- The WISE Blazar-Like Radio-Loud Sources: An All-Sky Catalog Of Candidate Gamma-Ray Blazars
- MOJAVE XII: Acceleration and Collimation of Blazar Jets on Parsec Scales
- Faraday rotation and polarization gradients in the jet of 3C~120: Interaction with the external medium and a helical magnetic field?
- The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array
- A Multi-epoch VLBI Survey of the Kinematics of Caltech-Jodrell Bank Flat-Spectrum Sources, Part II: Analysis of the Kinematics
- POLAMI: Polarimetric Monitoring of Active Galactic Nuclei at Millimetre Wavelengths. I. The program, calibration, and calibrators data products
- Comparison of algorithms for determination of rotation measure and Faraday structure I. 1100 - 1400 MHz
- The challenges of low-frequency radio polarimetry: lessons from the Murchison Widefield Array
- The VSOP 5 GHz Active Galactic Nucleus Survey: V. Imaging Results for the Remaining 140 sources
- The IDV source J1128+5925, a new candidate for annual modulation?
- Multi-frequency monitoring of gamma-ray loud blazars: I. Light curves and spectral energy distributions
- Single-dish and VLBI observations of Cygnus X-3 during the 2016 giant flare episode
- The F-GAMMA program: Multi-frequency study of Active Galactic Nuclei in the Fermi era. Program description and the first 2.5 years of monitoring
- The intra-hour variable quasar J18193845: 13-year evolution, jet polarization structure and interstellar scattering screen properties
- Polarization signatures of unresolved radio sources
- The MASIV Survey IV: relationship between intra-day scintillation and intrinsic variability of radio AGNs
- The University of Michigan Centimeter-Band All Stokes Blazar Monitoring Program: Single-Dish Polarimetry as a Probe of Parsec-Scale Magnetic Fields
- 18-22 cm VLBA Faraday rotation studies of six AGN jets
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- The Faraday Rotation Measure Grid of the LOFAR Two-metre Sky Survey: Data Release 2
- Discovery of ASKAP J173608.2-321635 as a Highly-Polarized Transient Point Source with the Australian SKA Pathfinder
- The Complex Large-scale Magnetic Fields in the First Galactic Quadrant as Revealed by the Faraday Depth Profile Disparity
- A Broadband Spectro-polarimetric View of the NVSS Rotation Measure Catalogue II: Effects of Off-axis Instrumental Polarisation
- LOFAR Deep Fields: Probing a broader population of polarized radio galaxies in ELAIS-N1
- Deterministic Aspect of the -ray Variability in Blazars
- The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II
- Message in a Bottle: Unveiling the Magneto-Ionic Complexity of AGNs through the Stokes QU-Fitting Technique
- Properties of Compact Faint Radio Sources as a Function of Angular Size from Stacking
- Broad-band Radio Polarimetry of disk galaxies and AGN with KAT 7