output
20042025
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations

Showing 2024Show all

13 papers · 1 filter

astro-ph.HE20241 cited

Tentative Blazar Candidate EP240709A Associated with 4FGL J0031.5-5648: NICER and Archival Multiwavelength Observations

Mason Ng, Jeremy Hare, Gaurava K. Jaisawal +3

We report on follow-up observations of the recently discovered transient by the Einstein Probe, EP240709A, with the Neutron star Interior Composition Explorer (NICER). We also inco…

astro-ph.HE20244 cited

Cocoon shock, X-ray cavities and extended Inverse Compton emission in Hercules A: clues from Chandra observations

F. Ubertosi, Y. Gong, P. Nulsen +7

We present a detailed analysis of jet activity in the radio galaxy 3C348 at the center of the galaxy cluster Hercules A. We use archival Chandra data to investigate the jet-driven…

astro-ph.HE20241 cited

Pulsed and Polarized X-ray Emission from Neutron Star Surfaces

Matthew G. Baring, Hoa Dinh Thi, George A. Younes +1

The intense magnetic fields of neutron stars naturally lead to strong anisotropy and polarization of radiation emanating from their surfaces, both being sensitive to the hot spot p…

astro-ph.HE2024

Multiwavelength study of 1eRASS J085039.9-421151 with eROSITA NuSTAR and X-shooter

Aafia Zainab, Artur Avakyan, Victor Doroshenko +23

The eROSITA instrument on board Spectrum-Roentgen-Gamma has completed four scans of the X-ray sky, leading to the detection of almost one million X-ray sources in eRASS1 only, incl…

astro-ph.HE202423 cited

Recurring tidal disruption events a decade apart in IRAS F01004-2237

Luming Sun, Ning Jiang, Liming Dou +16

We report the discovery of a second optical flare that occurred in September 2021 in IRAS F01004-2237, where the first flare occurred in 2010 has been reported, and present a detai…

astro-ph.HE20241 cited

Towards Modelling AR Sco: Generalised Particle Dynamics and Strong Radiation-Reaction Regimes

L. Du Plessis, C. Venter, A. K. Harding +3

Numerical simulations of relativistic plasmas have become more feasible, popular, and crucial for various astrophysical sources with the availability of computational resources. Th…