9 citations · 35 across the 7 of their papers we have counts for
7 papers
Einstein Probe discovery of the magnetar EP J223759.5+531421
N. Rea, F. Coti Zelati, A. Borghese +44
We report the discovery and early outburst evolution of the new Galactic magnetar EP J223759.5+531421, detected by the Einstein Probe Wide-field X-ray Telescope on 2026 June 28. Fo…
Evidence of the gamma-ray counterpart from nova FM Cir with Fermi-LAT
H. H. Wang, H. D. Yan, L. C. -C. Lin +2
We report the analysis results of X-ray and gamma-ray data of the nova FM Cir taken by Swift and Fermi-LAT. The gamma-ray emission from FM Cir can be identified with a significance…
Evidence of stellar oscillations in the post-common envelop binary candidate ASASSN-V J205543.90+240033.5
J. Takata, A. K. H. Kong, X. F. Wang +7
ASASSN-V J205543.90+240033.5 (ASJ2055) is a possible post-common envelope binary system. Its optical photometric data shows an orbital variation about ~days and a fast period…
An Investigation of the state changes of PSR J2021+4026 and the Vela pulsar
H. -H. Wang, J. Takata, L. C. -C. Lin +1
We investigate the high energy emission activities of two bright gamma-ray pulsars, PSR~J2021+4026 and Vela. For PSR~J2021+4026, the state changes in the gamma-ray flux and spin-do…
Searching for cataclysmic variable stars in unidentified X-ray sources
J. Takata, X. F. Wang, A. K. H. Kong +6
We carry out a photometric search for new cataclysmic variable stars (CVs), with the goal of identification for candidates of AR~Scorpii-type binary systems. We select GAIA sources…
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…
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…