activity
20242026
collaborators

6 papers

astro-ph.HE2026

Exploring LSST's capabilities for early detection of outbursts in low-mass X-ray binaries

Susmita Sett, Arash Bahramian, Kristen Dage +2

Following long periods of quiescence, low-mass X-ray binaries can exhibit intense X-ray outbursts triggered by instabilities within the accretion disk. These outbursts can sometime…

astro-ph.HE2025

No evidence for accretion around the intermediate-mass black hole in Omega Centauri

Angiraben D. Mahida, Arash Bahramian, James C. A. Miller Jones +5

For over a decade, both theoretical predictions and observational studies have suggested that Centauri ( Cen), the most massive Milky Way globular cluster, might harbor an…

astro-ph.HE2025

Investigating four new candidate redback pulsars discovered in the image plane

Flora Petrou, Natasha Hurley-Walker, Sam McSweeney +12

This paper reports the discovery and follow-up of four candidate redback spider pulsars: GPM J1723-33, GPM J1734-28, GPM J1752-30 and GPM J1815-14, discovered with the Murchison Wi…

astro-ph.GA2025

Classifying Compact Radio Emission in Nearby Galaxies: a 10GHz Study of Active Galactic Nuclei, Supernovae, Anomalous Microwave Emission and Star Forming Regions

Kristen C. Dage, Eric W. Koch, Evangelia Tremou +19

We present 115 compact radio point sources in three galaxies, NGC 5474, NGC 4631 and M51, taken in the most extended (A-)configuration of the Karl G. Jansky Very Large Array at 10G…

astro-ph.HE2025

Radio Continuum Studies of Ultra-Compact and Short Orbital Period X-Ray Binaries

Kristen C. Dage, Teresa Panurach, Kwangmin Oh +14

We present the radio continuum counterparts to the enigmatic ultra-compact X-ray binaries (UCXBs); a black hole or neutron star accreting from a hydrogen-deficient white dwarf dono…

astro-ph.HE2024

Detecting the Black Hole Candidate Population in M51's Young Massive Star Clusters: Constraints on Accreting Intermediate Mass Black Holes

Kristen C. Dage, Evangelia Tremou, Bolivia Cuevas Otahola +24

Intermediate mass black holes (10^2 < M_BH< 10^5 Msun) are an open question in our understanding of black hole evolution and growth. They have long been linked to dense star cluste…