activity
20192025
most citedRadio Galaxy Zoo: Unsupervised Clustering of Convolutionally Auto-encoded Radio-astronomical Images

50 citations · 147 across the 13 of their papers we have counts for

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5 papers · 1 filter

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 i…

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

Do Neutron Star Ultra-Luminous X-Ray Sources Masquerade as Intermediate Mass Black Holes in Radio and X-Ray?

Teresa Panurach, Kristen C. Dage, Ryan Urquhart +8

Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve…

astro-ph.HE2023★ 1 cited

Long-period radio pulsars: population study in the neutron star and white dwarf rotating dipole scenarios

Nanda Rea, Natasha Hurley-Walker, Celsa Pardo-Araujo +9

The nature of two recently discovered radio emitters with unusually long periods of 18min (GLEAM-X J1627-52) and 21min (GPM J1839-10) is highly debated. Their bright radio emission…

astro-ph.HE2019★ 20 cited

Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5

Rami Z. E. Alsaberi, C. Maitra, M. D. Filipovi'c +32

We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphol…