activity
20042025
most citedAn Overabundance of Transient X-ray Binaries within 1 pc of the Galactic Center

178 citations · 538 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2025

The BAGLE Python Package for Bayesian Analysis of Gravitational Lensing Events

J. R. Lu, M. Medford, C. Y. Lam +8

We present the open-source Python package, BAGLE (Bayesian Analysis of Gravitational Lensing Events), which enables modeling and joint fitting of photometric and astrometric data s…

astro-ph.SR2023

A hidden population of massive white dwarfs: two spotted K+WD binaries

D. M. Rowan, T. Jayasinghe, M. A. Tucker +10

The identification and characterization of massive () white dwarfs is challenging in part due to their low luminosity. Here we present two candidate single-lin…

astro-ph.GA2023★ 19 cited

The formation history of our Galaxy's nuclear stellar disc constrained from HST observations of the Quintuplet field

R. Schoedel, F. Nogueras-Lara, M. Hosek +9

Until recently it was thought that the nuclear stellar disc at the centre of our Galaxy was formed via quasi-continuous star formation over billions of years. However, an analysis…

astro-ph.HE2023★ 29 cited

JWST Low-Resolution MIRI Spectral Observations of SN~2021aefx: High-density Burning in a Type Ia Supernova

J. M. DerKacy, C. Ashall, P. Hoeflich +38

We present a JWST/MIRI low-resolution mid-infrared (MIR) spectroscopic observation of the normal Type Ia supernova (SN Ia) SN 2021aefx at +323 days past rest-frame B-band maximum l…

astro-ph.HE2022★ 11 cited

SN 2021fxy: Mid-Ultraviolet Flux Suppression is a Common Feature of Type Ia Supernovae

J. M. DerKacy, S. Paugh, E. Baron +26

We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT, UV…

astro-ph.HE2022★ 23 cited

The Absolute Magnitudes of 1991T-like Supernovae

M. M. Phillips, C. Ashall, Christopher R. Burns +20

1991T-like supernovae are the luminous, slow-declining extreme of the Branch shallow-silicon (SS) subclass of Type Ia supernovae. They are distinguished by extremely weak Ca II H &…