English

An analysis pipeline for CHIME/FRB full-array baseband data

High Energy Astrophysical Phenomena 2021-04-14 v2 Instrumentation and Methods for Astrophysics

Abstract

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) has become a leading facility for detecting fast radio bursts (FRBs) through the CHIME/FRB backend. CHIME/FRB searches for fast transients in polarization-summed intensity data streams that have 24-kHz spectral and 1-ms temporal resolution. The intensity beams are pointed to pre-determined locations in the sky. A triggered baseband system records the coherent electric field measured by each antenna in the CHIME array at the time of FRB detections. Here we describe the analysis techniques and automated pipeline developed to process these full-array baseband data recordings. Whereas the real-time FRB detection pipeline has a localization limit of several arcminutes, offline analysis of baseband data yields source localizations with sub-arcminute precision, as characterized by using a sample of pulsars and one repeating FRB with known positions. The baseband pipeline also enables resolving temporal substructure on a micro-second scale and the study of polarization including detections of Faraday rotation.

Keywords

Cite

@article{arxiv.2010.06748,
  title  = {An analysis pipeline for CHIME/FRB full-array baseband data},
  author = {D. Michilli and K. W. Masui and R. Mckinven and D. Cubranic and M. Bruneault and C. Brar and C. Patel and P. J. Boyle and I. H. Stairs and A. Renard and K. Bandura and S. Berger and D. Breitman and T. Cassanelli and M. Dobbs and V. M. Kaspi and C. Leung and J. Mena-Parra and Z. Pleunis and L. Russell and P. Scholz and S. R. Siegel and S. P. Tendulkar and K. Vanderlinde},
  journal= {arXiv preprint arXiv:2010.06748},
  year   = {2021}
}
R2 v1 2026-06-23T19:19:39.612Z