activity
19972023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 4k across the 112 of their papers we have counts for

collaborators

113 papers

astro-ph.HE2023

Swift Deep Galactic Plane Survey Classification of Swift J170800402551.8 as a Candidate Intermediate Polar Cataclysmic Variable

B. O'Connor, E. Gogus, J. Hare +24

Here, we present the results of our multi-wavelength campaign aimed at classifying \textit{Swift} J170800402551.8 as part of the \textit{Swift} Deep Galactic Plane Survey (DGPS)…

astro-ph.HE2023★ 8 cited

Classifying IGR J15038-6021 as a magnetic CV with a massive white dwarf

John A. Tomsick, Snehaa Ganesh Kumar, Benjamin M. Coughenour +8

Cataclysmic variables (CVs) are binary systems consisting of a white dwarf (WD) accreting matter from a companion star. Observations of CVs provide an opportunity to learn about ac…

astro-ph.HE2023

The Swift Deep Galactic Plane Survey (DGPS) Phase-I Catalog

B. O'Connor, C. Kouveliotou, P. A. Evans +30

The \textit{Swift} Deep Galactic Plane Survey is a \textit{Swift} Key Project consisting of 380 tiled pointings covering 40 deg of the Galactic Plane between longitude \,…

astro-ph.HE2023★ 20 cited

The Orbital Period vs. Absolute Magnitude Relationship of Intermediate Polars: Implications for Low States and Outbursts

Koji Mukai, Magaretha L. Pretorius

Recent advances in time-domain astronomy have led to fresh observational insights into intermediate polars, a subtype of magnetic cataclysmic variables generally accreting via a pa…

astro-ph.HE2023★ 2 cited

Gravitational Redshift Detection from the Magnetic White Dwarf Harbored in RX J1712.6-2414

Takayuki Hayashi, Hideyuki Mori, Koji Mukai +2

Gravitational redshift is a fundamental parameter that allows us to determine the mass-to-radius ratio of compact stellar objects, such as black holes, neutron stars, and white dwa…

astro-ph.HE2023★ 9 cited

Catching a nova X-ray/UV flash in the visible? Early spectroscopy of the extremely slow Nova Velorum 2022 (Gaia22alz)

E. Aydi, L. Chomiuk, J. Mikołajewska +22

We present early spectral observations of the very slow Galactic nova Gaia22alz, over its gradual rise to peak brightness that lasted 180 days. During the first 50 days, when the n…