activity
20102024
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 1.8k across the 38 of their papers we have counts for

collaborators

30 papers

astro-ph.HE20231 cited

Prospects for Time-Domain and Multi-Messenger Science with AXIS

The AXIS Time-Domain, Multi-Messenger Science Working Group, : +19

The Advanced X-ray Imaging Satellite (AXIS) promises revolutionary science in the X-ray and multi-messenger time domain. AXIS will leverage excellent spatial resolution (<1.5 arcse…

astro-ph.IM202377 cited

Overview of the Advanced X-ray Imaging Satellite (AXIS)

Christopher S. Reynolds, Erin A. Kara, Richard F. Mushotzky +40

The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra X-ray Observatory by providing low-background, arcsecond-resolutio…

astro-ph.HE2023

Variability as a predictor for the hard-to-soft state transition in GX 339-4

Matteo Lucchini, Marina Ten Have, Jingyi Wang +17

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by non…

astro-ph.HE2023

AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 817

Jack M. M. Neustadt, Christopher S. Kochanek, John Montano +49

We fit the UV/optical lightcurves of the Seyfert 1 galaxy Mrk 817 to produce maps of the accretion disk temperature fluctuations resolved in time and radius. The maps are…

astro-ph.HE2023

Accretion disk wind of Hercules X-1 during the Short High state

P. Kosec, E. Kara, A. C. Fabian +5

Hercules X-1 is a nearly edge-on X-ray binary with a warped, precessing accretion disk, which manifests through a 35-day cycle of alternating High and Low flux states. This disk pr…

astro-ph.HE2023

Discovery of a variable multi-phase outflow in the X-ray-emitting tidal disruption event ASASSN-20qc

P. Kosec, D. Pasham, E. Kara +1

Tidal disruption events (TDEs) are exotic transients that can lead to temporary super-Eddington accretion onto a supermassive black hole. Such accretion mode is naturally expected…