2020MNRAS.494.1994Z


Query : 2020MNRAS.494.1994Z

2020MNRAS.494.1994Z - Mon. Not. R. Astron. Soc., 494, 1994-2003 (2020/May-2)

A radio burst detection method based on the Hough transform.

ZUO S. and CHEN X.

Abstract (from CDS):

We present a simple and fast method for incoherent dedispersion and fast radio burst (FRB) detection based on the Hough transform, which is widely used for feature extraction in image analysis. The Hough transform maps a point in the time-frequency data to a straight line in the parameter space and points on the same dispersed f–2 curve to a bundle of lines all crossing at the same point, thus the curve is transformed to a single point in the parameter space, enabling an easier way for the detection of radio burst. By choosing an appropriate truncation threshold, in a reasonably radio quiet environment, i.e. with radio frequency interferences present but not dominant, the computing speed of the method is very fast. Using simulation data of different noise levels, we studied how the detected peak varies with different truncation thresholds. We also tested the method with some real pulsar and FRB data.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - radio continuum: transients

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 FRB 010724 rB 01 18 06.0 -72 12 19           ~ 94 1
2 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1
3 NAME FRB J1852-08 rB 18 52 05.0 -08 29 35           ~ 54 0
4 FRB 010125 rB 19 06 53.00 -40 37 14.4           ~ 46 1
5 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
6 FRB 110626 rB 21 03 43.0 -44 44 19           ~ 49 1
7 FRB 110523 rB 21 45 31.0 -00 15 23           ~ 91 0
8 FRB 140514 rB 22 34 06.20 -12 18 46.5           ~ 80 0
9 FRB 110220 rB 22 34 38.0 -12 33 44           ~ 82 0
10 FRB 120127 rB 23 15 06.0 -18 25 37           ~ 51 0
11 PSR B2319+60 Psr 23 21 55.213 +60 24 30.71     13.80     ~ 200 0
12 FRB 110703 rB 23 30 51.0 -02 52 24           ~ 54 0

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