On the Problems of Detecting Fast Radio Bursts with the LPA LPI

E. A. Brylyakova; Брылякова Е. А.; S. A. Tyul’bashev; Тюльбашев С. А.

doi:10.31857/S0004629923020044

On the Problems of Detecting Fast Radio Bursts with the LPA LPI

Authors: Brylyakova E.A.¹, Tyul’bashev S.A.¹
Affiliations:
1. Lebedev Physical Institute, Astro Space Center, Pushchino Radio Astronomy Observatory
Issue: Vol 100, No 2 (2023)
Pages: 186-195
Section: Articles
URL: https://journals.rcsi.science/0004-6299/article/view/139065
DOI: https://doi.org/10.31857/S0004629923020044
EDN: https://elibrary.ru/CJOIYX
ID: 139065

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Abstract
About the authors
References
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Abstract

We present a verification of fast radio bursts (FRBs) previously published by V.A. Fedorova and A.E. Rodin. These FRBs were found in the monitoring data with the Large Phased Array (LPA) radio telescope using a search algorithm based on data convolution with a scattered pulse pattern. The same 6-channel data (channel width 415 kHz) were used for verification, in which FRBs were found with dispersion measures of 247, 570, and 1767 pc/cm3. An additional verification of the published FRBs was also carried out in 32‑channel data (channel width 78 kHz). We can not confirm any of the published FRBs on the signal-to-noise ratios claimed in the original paper. The main errors are caused by incorrect determination of the baseline and incorrect estimation of noise standard deviations.

Keywords

fast radio bursts, nature of radio bursts

About the authors

E. A. Brylyakova

Lebedev Physical Institute, Astro Space Center, Pushchino Radio Astronomy Observatory

Email: elinxt@bk.ru
142290, Pushchino, Russia

S. A. Tyul’bashev

Lebedev Physical Institute, Astro Space Center, Pushchino Radio Astronomy Observatory

Author for correspondence.
Email: serg@prao.ru
142290, Pushchino, Russia

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