activity
20092014
most citedA detailed X-ray investigation of PSR J2021+4026 and -Cygni supernova remnant

19 citations · 29 across the 2 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2014★ 19 cited

A detailed X-ray investigation of PSR J2021+4026 and -Cygni supernova remnant

C. Y. Hui, K. A. Seo, L. C. C. Lin +9

We have investigated the field around the radio-quiet -ray pulsar, PSR J2021+4026, with a ~140 ks XMM-Newton observation and a ~56 ks archival Chandra data. Through analyzing th…

astro-ph.HE2014★ 10 cited

Identification campaign of supernova remnant candidates in the Milky Way. II. X-ray studies of G38.7-1.4

R. H. H. Huang, J. H. K. Wu, C. Y. Hui +3

We report on XMM-Newton and Chandra observations of the Galactic supernova remnant candidate G38.7-1.4, together with complementary radio, infrared, and gamma-ray data. An approxim…

astro-ph.HE2013

Discovery of X-ray Pulsation from the Geminga-like Pulsar PSR J2021+4026

L. C. C. Lin, C. Y. Hui, C. P. Hu +8

We report the discovery of X-ray periodicity of ~265.3 ms from a deep XMM-Newton observation of the radio-quiet gamma-ray pulsar, PSR J2021+4026, located at the edge of the superno…

astro-ph.HE2013

Search for pulsed gamma-ray emission from globular cluster M28

J. H. K. Wu, C. Y. Hui, E. M. H. Wu +5

Using the data from the Large Area Telescope on board the Fermi Gamma-ray Space Telescope, we have searched for the gamma-ray pulsations from the direction of globular cluster M28…

astro-ph.HE2012

Orbital Phase Dependent Gamma-ray emissions from the Black Widow Pulsar

E. M. H. Wu, J. Takata, K. S. Cheng +5

We report on evidence for orbital phase-dependence of the gamma-ray emission from PSR B1957+20 black widow system by using the data of the Fermi Large Area Telescope. We divide an…

astro-ph.HE2012

Pulsed γ-ray emission from magnetar 1E 2259+586

J. H. K. Wu, C. Y. Hui, R. H. H. Huang +6

Anomalous x-ray pulsars (AXPs) are thought to be magnetars which are young isolated neutron stars with extremely strong magnetic fields of > 10^14Gauss. Their tremendous magnetic f…