papers

Publications (35)

astro-ph.SR2025

Enigmatic centi-SFU and mSFU nonthermal radio transients detected in the middle corona

Surajit Mondal, Bin Chen, Sijie Yu +43

Decades of solar coronal observations have provided substantial evidence for accelerated particles in the corona. In most cases, the location of particle acceleration can be roughl…

stat.ME2021

Auto-balanced common shock claim models

Greg Taylor, Phuong Anh Vu

The paper is concerned with common shock models of claim triangles. These are usually constructed as a linear combinations of shock components and idiosyncratic components. Previou…

astro-ph.HE2025

Searches for Prompt Low-Frequency Radio Counterparts to Gravitational Wave Event S250206dm with the OVRO-LWA Time Machine

Nikita Kosogorov, Gregg Hallinan, Casey Law +46

We report on a search for prompt, low-frequency radio emission from the gravitational-wave (GW) merger S250206dm using the Owens Valley Radio Observatory Long Wavelength Array (OVR…

astro-ph.IM2021

Bringing SOUL on sky

Enrico Pinna, Fabio Rossi, Alfio Puglisi +20

The SOUL project is upgrading the 4 SCAO systems of LBT, pushing the current guide star limits of about 2 magnitudes fainter thanks to Electron Multiplied CCD detector. This improv…

astro-ph.IM2026

All-Sky Ultra-Narrowband Spectral Imaging with the OVRO-LWA: Technosignature Constraints and Axion-Like Particle Prospects

Nikita Kosogorov, Gregg Hallinan, Greg Hellbourg +46

We present an imaging-domain search for technosignatures at decametric wavelengths with the OVRO-LWA, targeting ultra-narrowband continuous-wave signals between 50 and 86 MHz. We i…

astro-ph.IM2026

A Commensal Radio-Only Cosmic Ray Detector at the Owens Valley Radio Observatory Long Wavelength Array

Kathryn A. Plant, Andrew Romero-Wolf, Gregg Hallinan +46

The brief (10 nanoseconds) transient radio emission from cosmic ray air showers carries key information about the energy and mass composition of high energy cosmic rays, but anthro…

astro-ph.GA2018

The Next-Generation Very Large Array: Supermassive Black Hole Pairs and Binaries

Sarah Burke-Spolaor, Laura Blecha, Tamara Bogdanovic +7

The Next-Generation Very Large Array (ngVLA) has the potential to be a workhorse for the discovery and study of paired supermassive black holes either at large separations (dual) o…

stat.ML2023

Machine Learning with High-Cardinality Categorical Features in Actuarial Applications

Benjamin Avanzi, Greg Taylor, Melantha Wang +1

High-cardinality categorical features are pervasive in actuarial data (e.g. occupation in commercial property insurance). Standard categorical encoding methods like one-hot encodin…

astro-ph.CO2010

The radio properties of a complete, X-ray selected sample of nearby, massive elliptical galaxies

Robert Dunn, Steve Allen, Greg Taylor +4

We investigate the radio properties of a complete sample of nearby, massive, X-ray bright elliptical and S0 galaxies. Our sample contains 18 galaxies with ROSAT All-Sky Survey X-ra…

astro-ph.SR2025

Possible First Detection of Gyroresonance Emission from a Coronal Mass Ejection in the Middle Corona

Surajit Mondal, Bin Chen, Xingyao Chen +45

Routine measurements of the magnetic field of coronal mass ejections (CMEs) have been a key challenge in solar physics. Making such measurements is important both from a space weat…

stat.AP2022

Log normal claim models with common shocks

Greg Taylor

This paper is concerned with modelling multiple claim arrays that are subject to one or more common shocks. It uses a structure that involves very general forms both idiosyncratic…

q-fin.RM2020

Modelling and understanding count processes through a Markov-modulated non-homogeneous Poisson process framework

Benjamin Avanzi, Greg Taylor, Bernard Wong +1

The Markov-modulated Poisson process is utilised for count modelling in a variety of areas such as queueing, reliability, network and insurance claims analysis. In this paper, we e…

astro-ph.SR2025

Probing the Turbulent Corona and Heliosphere Using Radio Spectral Imaging Observation during the Solar Conjunction of Crab Nebula

Peijin Zhang, Surajit Mondal, Bin Chen +41

Measuring plasma parameters in the upper solar corona and inner heliosphere is challenging because of the region's weakly emissive nature and inaccessibility for most in situ obser…

stat.AP2026

Dynamic Financial Analysis (DFA) of General Insurers under Climate Change

Benjamin Avanzi, Yanfeng Li, Greg Taylor +1

Climate change is expected to significantly affect the physical, financial, and economic environments over the long term, posing risks to the financial health of general insurers.…

astro-ph.IM2019

Self-triggered radio detection and identification of cosmic air showers with the OVRO-LWA

Ryan Monroe, Andres Romero Wolf, Gregg Hallinan +12

A successful ground array Radio Frequency (RF)-only self-trigger on 10 high-energy cosmic ray events is demonstrated with 256 dual-polarization antennas of the Owens Valley Radio O…

astro-ph.SR2026

Estimating Electron Densities in the Middle Solar Corona using White-light and Radio Observations

Surajit Mondal, Shaheda Begum Shaik, Russell A. Howard +45

The electron density of the solar corona is a fundamental parameter in many areas of solar physics. Traditionally, routine estimates of coronal density have relied exclusively on w…

q-fin.RM2024

On the evolution of data breach reporting patterns and frequency in the United States: a cross-state analysis

Benjamin Avanzi, Xingyun Tan, Greg Taylor +1

Understanding the emergence of data breaches is crucial for cyber insurance. However, analyses of data breach frequency trends in the current literature lead to contradictory concl…

astro-ph.HE2016

Polarization Signatures of Kink Instabilities in the Blazar Emission Region from Relativistic Magnetohydrodynamic Simulations

Haocheng Zhang, Hui Li, Fan Guo +1

Kink instabilities are likely to occur in the current-carrying magnetized plasma jets. Recent observations of the blazar radiation and polarization signatures suggest that the blaz…

astro-ph2004

A2255: the First Detection of Filamentary Polarized Emission in a Radio Halo

Federica Govoni, Matteo Murgia, Luigina Feretti +3

A deep radio observation of the A2255 cluster of galaxies has been carried out at 1.4 GHz with the Very Large Array synthesis telescope. Thanks to the excellent (u,v) coverage and…

astro-ph.IM2019

A Real-Time, All-Sky, High Time Resolution, Direct Imager for the Long Wavelength Array

James Kent, Jayce Dowell, Adam Beardsley +3

The future of radio astronomy will require instruments with large collecting areas for higher sensitivity, wide fields of view for faster survey speeds, and efficient computing and…

stat.ME2021

Stochastic loss reserving with mixture density neural networks

Muhammed Taher Al-Mudafer, Benjamin Avanzi, Greg Taylor +1

Neural networks offer a versatile, flexible and accurate approach to loss reserving. However, such applications have focused primarily on the (important) problem of fitting accurat…

stat.ME2023

On the impact of outliers in loss reserving

Benjamin Avanzi, Mark Lavender, Greg Taylor +1

The sensitivity of loss reserving techniques to outliers in the data or deviations from model assumptions is a well known challenge. It has been shown that the popular chain-ladder…

astro-ph.SR2026

Summary of the First Year of the Space Weather Around Young Suns Program: 900 Hours of Low-frequency Radio and Optical Data Dedicated to Young, Solar-type Stars

Ivey Davis, Gregg Hallinan, Nikita Kosogorov +51

The Space Weather Around Young Suns (SWAYS) program was introduced in \citet{Davis2025} as a multi-wavelength monitoring program for studying the activity and particle environments…

astro-ph.IM2017

A Next Generation Low Band Observatory: A Community Study Exploring Low Frequency Options for ngVLA

Greg Taylor, Jayce Dowell, Joe Malins +9

We present a community study exploring the low frequency (5 - 800 MHz) options and opportunities for the ngVLA project and its infrastructure. We describe a Next Generation LOw Ban…

stat.ME2023

Detection and treatment of outliers for multivariate robust loss reserving

Benjamin Avanzi, Mark Lavender, Greg Taylor +1

Traditional techniques for calculating outstanding claim liabilities such as the chain ladder are notoriously at risk of being distorted by outliers in past claims data. Unfortunat…

astro-ph.HE2012

VLBI and Archival VLA and WSRT Observations of the GRB 030329 Radio Afterglow

Robert Mesler, Ylva Pihlström, Greg Taylor +1

We present VLBI and archival Karl G. Jansky Very Large Array (VLA) and Westerbork Synthesis Radio Telescope (WSRT) observations of the radio afterglow from the gamma-ray burst (GRB…

astro-ph.SR2026

Implementation of a Near-Realtime Recording and Reporting System of Solar Radio Bursts

Peijin Zhang, Anastasia Kuske, Bin Chen +48

Strong solar activity is often accompanied by a variety of radio bursts. These bursts are valuable diagnostics of coronal and heliospheric processes and also have potential applica…

astro-ph.CO2010

Extreme AGN Feedback and Cool Core Destruction in the X-ray Luminous Galaxy Cluster MACS J1931.8-2634

Steven Ehlert, Steve Allen, Anja von der Linden +14

We report on a deep, multiwavelength study of the galaxy cluster MACS J1931.8-2634 using Chandra X-ray, Subaru optical, and VLA 1.4 GHz radio data. This cluster (z=0.352) harbors o…

astro-ph.SR2020

Detection of Echoes in PSR B1508+55 at frequencies below 100 MHz using the LWA1

Karishma Bansal, Greg Taylor, Kevin Stovall +1

PSR B1508+55 is known to have a single component profile above 300 MHz. However, when we study it at frequencies below 100 MHz using the first station of the Long Wavelength Array,…

astro-ph.IM2014

Very Long Baseline Interferometry with the SKA

Zsolt Paragi, Leith Godfrey, Cormac Reynolds +79

Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by pr…

astro-ph.SR2020

Observing Flare Stars Below 100 MHz with the LWA

Ivey Davis, Greg Taylor, Jayce Dowell

We observed the flare stars AD Leonis, Wolf 424, EQ Pegasi, EV Lacertae, and UV Ceti for nearly 135 hours. These stars were observed between 63 and 83 MHz using the interferometry…

q-fin.ST2025

On the use of case estimate and transactional payment data in neural networks for individual loss reserving

Benjamin Avanzi, Matthew Lambrianidis, Greg Taylor +1

The use of neural networks trained on individual claims data has become increasingly popular in the actuarial reserving literature. We consider how to best input historical payment…

astro-ph.IM2023

Optimization and Commissioning of the EPIC Commensal Radio Transient Imager for the Long Wavelength Array

Hariharan Krishnan, Adam P. Beardsley, Judd D. Bowman +4

Next generation aperture arrays are expected to consist of hundreds to thousands of antenna elements with substantial digital signal processing to handle large operating bandwidths…

astro-ph.SR2025

Measuring the Magnetic Field of a Coronal Mass Ejection from Low to Middle Corona

Xingyao Chen, Bin Chen, Sijie Yu +44

A major challenge in understanding the initiation and evolution of coronal mass ejections (CMEs) is measuring the magnetic field of the magnetic flux ropes (MFRs) that drive CMEs.…

astro-ph.GA2019

Studying the magnetized ISM with all-sky polarimetric radio maps

Colin Lonsdale, Elena Orlando, Gregg Hallinan +2

Synchrotron radiation from the interstellar medium (ISM) of our galaxy dominates the sky brightness at low radio frequencies, and carries information about relativistic and thermal…