Detection of Repeating FRB 180916.J0158+65 Down to Frequencies of 300 MHz

@article{Chawla2020DetectionOR,
  title={Detection of Repeating FRB 180916.J0158+65 Down to Frequencies of 300 MHz},
  author={Pragya Chawla and Bridget C. Andersen and Mohit Bhardwaj and Emmanuel Fonseca and Alexander Josephy and Victoria M. Kaspi and Daniele Michilli and Ziggy Pleunis and Kevin Bandura and C. G. Bassa and P. J. Boyle and Charanjot Brar and Tomas Cassanelli and D. Cubranic and M. A. Dobbs and F. Q. Dong and Bryan M. Gaensler and Deborah C. Good and Jason W. T. Hessels and Tom L. Landecker and Calvin Leung and D. Z. Li and H. H. Lin and Kiyoshi W. Masui and Ryan Mckinven and Juan Mena-Parra and M. Merryfield and Bradley W. Meyers and Arun Kumar Naidu and Cherry Ng and Chitrang Patel and Masoud Rafiei-Ravandi and M. Rahman and P. Sanghavi and Paul Scholz and Kaitlyn Shin and K. M. Smith and Ingrid H. Stairs and Shriharsh P. Tendulkar and Keith Vanderlinde},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2020}
}
We report on the detection of seven bursts from the periodically active, repeating fast radio burst (FRB) source FRB 180916.J0158+65 in the 300-400-MHz frequency range with the Green Bank Telescope (GBT). Emission in multiple bursts is visible down to the bottom of the GBT band, suggesting that the cutoff frequency (if it exists) for FRB emission is lower than 300 MHz. Observations were conducted during predicted periods of activity of the source, and had simultaneous coverage with the Low… 

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