activity
20062023
most citedThe unprecedented optical outburst of the quasar 3C 454.3. The WEBT campaign of 2004-2005

186 citations · 269 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Magnetars and Other Isolated Neutron Stars

J. A. J. Alford, G. A. Younes, Z. Wadiasingh +23

The hard X-ray emission from magnetars and other isolated neutron stars remains under-explored. An instrument with higher sensitivity to hard X-rays is critical to understanding th…

astro-ph.HE2022★ 1 cited

Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode

G. Younes, M. G. Baring, A. K. Harding +16

Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic fields. Many attributes of m…

astro-ph.HE2020★ 7 cited

An X-ray study for white dwarf binary AR Scorpii

J. Takata, X. F. Wang, H. H. Wang +4

We report a study of the X-ray emission from the white dwarf/M-type star binary system AR Scorpii using archival data taken in 2016-2020. It has been known that the X-ray emission…

astro-ph.HE2020★ 9 cited

A multi-wavelength study of PSR J11196127 after 2016 outburst

H. -H. Wang, L. C. -C. Lin, S. Dai +4

PSR~J11196127, a high-magnetic field pulsar detected from radio to high-energy wavelengths, underwent a magnetar-like outburst beginning on July 27, 2016. In this paper, we stud…

astro-ph.HE2020★ 22 cited

Repeated state change of variable gamma-ray pulsar, PSR J2021+4026

J. Takata, H. H. Wang, L. C. C. Lin +6

PSR J2021+4026 is a radio-quiet gamma-ray pulsar and the first pulsar that shows state change of the gamma-ray emission and spin-down rate. The state change of PSR J2021+4026 was f…

astro-ph.HE2018★ 9 cited

X-ray study of Variable Gamma-ray Pulsar PSR J2021+4026

H. H. Wang, J. Takata., C. -P. Hu +2

PSR~J2021+4026 showed a sudden decrease in the gamma-ray emission at the glitch that occurred around 2011, October 16, and a relaxation of the flux to the pre-glitch state at aroun…