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20232026
most citedContemporaneous X-ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A

11 citations · 42 across the 22 of their papers we have counts for

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astro-ph.GA2024

A novel approach to understanding the link between supermassive black holes and host galaxies

Gabriel Sasseville, Julie Hlavacek-Larrondo, Samantha C. Berek +5

The strongest and most universal scaling relation between a supermassive black hole and its host galaxy is known as the relation, where is the mass of the…

astro-ph.HE2024★ 2 cited

Morphology of 35 Repeating Fast Radio Burst Sources at Microsecond Time Scales with CHIME/FRB

Alice P. Curtin, Ketan R. Sand, Ziggy Pleunis +27

The Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) project has discovered the most repeating fast radio burst (FRB) sources of any telescope. However,…

astro-ph.HE2024

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

Antonio Herrera-Martin, Radu V. Craiu, Gwendolyn M. Eadie +8

An important task in the study of fast radio bursts (FRBs) remains the automatic classification of repeating and non-repeating sources based on their morphological properties. We p…

stat.AP2024

K-Contact Distance for Noisy Nonhomogeneous Spatial Point Data with application to Repeating Fast Radio Burst sources

A. M. Cook, Dayi Li, Gwendolyn M. Eadie +12

This paper introduces an approach to analyze nonhomogeneous Poisson processes (NHPP) observed with noise, focusing on previously unstudied second-order characteristics of the noisy…

astro-ph.GA2024★ 8 cited

Discovery of Two Ultra-Diffuse Galaxies with Unusually Bright Globular Cluster Luminosity Functions via a Mark-Dependently Thinned Point Process (MATHPOP)

Dayi Li, Gwendolyn Eadie, Patrick Brown +8

We present \textsc{Mathpop}, a novel method to infer the globular cluster (GC) counts in ultra-diffuse galaxies (UDGs) and low-surface brightness galaxies (LSBGs). Many known UDGs…

astro-ph.HE2024

Morphology of 137 Fast Radio Bursts down to Microseconds Timescales from The First CHIME/FRB Baseband Catalog

Ketan R. Sand, Alice P. Curtin, Daniele Michilli +21

We present a spectro-temporal analysis of 137 fast radio bursts (FRBs) from the first CHIME/FRB baseband catalog, including 125 one-off bursts and 12 repeat bursts, down to microse…

astro-ph.HE2024★ 11 cited

Contemporaneous X-ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A

Amanda M. Cook, Paul Scholz, Aaron B. Pearlman +22

We present an extensive contemporaneous X-ray and radio campaign performed on the repeating fast radio burst (FRB) source FRB 20220912A for eight weeks immediately following the so…

astro-ph.GA2024★ 2 cited

On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis

D. J. Whitworth, S. Srinivasan, R. E. Pudritz +19

The magnetic field strength to gas density relation in the interstellar medium is of fundamental importance. We present and compare Bayesian analyses of the B-n relation for two co…

astro-ph.HE2024

Constraining the selection corrected luminosity function and total pulse count for radio transients

Fengqiu Adam Dong, Antonio Herrera-Martin, Ingrid Stairs +9

Studying transient phenomena, such as individual pulses from pulsars, has garnered considerable attention in the era of astronomical big data. Of specific interest to this study ar…

astro-ph.SR2024★ 3 cited

Detecting stellar flares in photometric data using hidden Markov models

J. Arturo Esquivel, Yunyi Shen, Vianey Leos-Barajas +5

We present a hidden Markov model (HMM) for discovering stellar flares in light curve data of stars. HMMs provide a framework to model time series data that are not stationary; they…

astro-ph.HE2024★ 3 cited

A pulsar-like swing in the polarisation position angle of a nearby fast radio burst

Ryan Mckinven, Mohit Bhardwaj, Tarraneh Eftekhari +41

Fast radio bursts (FRBs) last for milliseconds and arrive at Earth from cosmological distances. While their origin(s) and emission mechanism(s) are presently unknown, their signals…