Published November 20, 2022 | Version v1

Magnetic field reversal in the turbulent environment around a repeating fast radio burst

  • 1. West Virginia University, Department of Physics and Astronomy, P. O. Box 6315, Morgantown, WV, USA, Center for Gravitational Waves and Cosmology, West Virginia University, Chestnut Ridge Research Building, Morgantown, WV, USA
  • 2. Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA

Description

All the bursts of FRB 20190520B detected from the Green Bank Telescope (GBT) that was used in the Anna-Thomas et al (2022) paper. This dataset contains both L-Band (1.4 GHz) and C-Band (6 GHz) bursts. The data is in pulse archive format, which can be read using the software suite PSRCHIVE or the package PyPulse. The L-band bursts are not calibrated. The C-Band bursts which has an extension .calib is calibrated for both flux and polarization and those which has an extension .calibP is only calibrated for polarization. 

Files

Files (3.2 GB)

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Additional details

Related works

Is described by
Preprint: arXiv:2202.11112 (arXiv)

References

  • Anna-Thomas et al (2022); A Highly Variable Magnetized Environment in a Fast Radio Burst Source; arxiv:2202.11112