2025ApJ...982...46H


Query : 2025ApJ...982...46H

2025ApJ...982...46H - Astrophys. J., 982, 46 (2025/March-3)

Rare Event Classification with Weighted Logistic Regression for Identifying Repeating Fast Radio Bursts.

HERRERA-MARTIN A., CRAIU R.V., EADIE G.M., STENNING D.C., BINGHAM D., GAENSLER B.M., PLEUNIS Z., SCHOLZ P., MCKINVEN R., KHAREL B. and MASUI K.W.

Abstract (from CDS):

An important task in the study of fast radio bursts (FRBs) remains the automatic classification of repeating and nonrepeating sources based on their morphological properties. We propose a statistical model that considers a modified logistic regression to classify FRB sources. The classical logistic regression model is modified to accommodate the small proportion of repeaters in the data, a feature that is likely due to the sampling procedure and duration and is not a characteristic of the population of FRB sources. The weighted logistic regression hinges on the choice of a tuning parameter that represents the true proportion τ of repeating FRB sources in the entire population. The proposed method has a sound statistical foundation, direct interpretability, and operates with only five parameters, enabling quicker retraining with added data. Using the CHIME/FRB Collaboration sample of repeating and nonrepeating FRBs and numerical experiments, we achieve a classification accuracy for repeaters of nearly 75% or higher when τ is set in the range of 50%-60%. This implies a tentative high proportion of repeaters, which is surprising, but is also in agreement with recent estimates of τ that are obtained using other methods.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Radio transient sources - Classification - Astrostatistics techniques - Sampling distribution - Astrostatistics distributions - Regression - Nonlinear regression - Linear regression

Simbad objects: 15

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Number of rows : 15
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 20190107B rB 02 13 48.0000 +83 24 00.000           ~ 8 0
2 FRB 20190308B rB 02 34 21.6000 +83 37 12.000           ~ 10 0
3 FRB 20190201A rB 04 16 07.2000 +84 50 24.000           ~ 6 0
4 FRB 20190609C rB 04 52 40.8000 +24 03 36.000           ~ 16 0
5 FRB 20190328C rB 04 55 19.2000 +81 57 36.000           ~ 9 0
6 FRB 20190113A rB 07 12 33.6000 -02 59 24.000           ~ 10 0
7 FRB 20180909A rB 08 14 31.2000 +56 45 36.000           ~ 8 0
8 FRB 20200120E rB 09 57 56.7 +68 49 32           ~ 219 0
9 FRB 20190127B rB 10 03 40.8000 +83 33 36.000           ~ 8 0
10 FRB 20190303D rB 11 58 16.8000 +70 50 24.000           ~ 8 0
11 FRB 20190110C rB 16 27 55.2000 +41 25 12.000           ~ 36 0
12 FRB 20190226B rB 18 14 16.8000 +61 48 36.000           ~ 9 0
13 FRB 20190430C rB 18 28 52.8000 +24 55 12.000           ~ 17 0
14 FRB 20190210C rB 19 43 00.0000 +89 06 00.000           ~ 9 0
15 FRB 20180910A rB 23 31 04.8000 +88 12 36.000           ~ 14 0

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