activity
20122025
most citedA non-thermal pulsed X-ray emission of AR~Scorpii

34 citations · 226 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2025

Effectiveness of Stacks in the Stacked Hilbert-Huang Transform

Lupin Chun-Che Lin, Chin-Ping Hu, Chien-Chang Yen +6

The Hilbert-Huang transform (HHT) consists of empirical mode decomposition (EMD), which is a template-free method that represents the combination of different intrinsic modes on a…

astro-ph.HE2021★ 11 cited

Investigation of gamma-ray variability and glitches of PSR J1420-6048

Lupin C. -C. Lin, H. H. Wang, C. Y. Hui +4

PSR J1420-6048 is a young gamma-ray pulsar with recurrent glitches. Utilizing long-term monitoring data obtained from the Fermi Gamma-ray Space Telescope, we found that PSR J1420-6…

astro-ph.HE2017★ 34 cited

A non-thermal pulsed X-ray emission of AR~Scorpii

J. Takata, C. -P. Hu, L. C. C. Lin +5

We report the analysis result of UV/X-ray emission from AR~Scorpii, which is an intermediate polar (IP) composed of a magnetic white dwarf and a M-type star, with the XMM-Newton da…

astro-ph.HE2017★ 28 cited

Mode change of a gamma-ray pulsar, PSR J2021+4026

J. Zhao, C. W. Ng, L. C. C. Lin +8

A glitch of a pulsar is known as a sudden increase in the spin frequency and spin-down rate (frequency time derivative), and it can be caused by a sudden rel\ ease of the stress bu…

astro-ph.HE2016★ 9 cited

Chandra and Swift X-ray Observations of the X-ray Pulsar SMC X-2 During the Outburst of 2015

K. L. Li, C. -P Hu, L. C. C. Lin +1

We report the Chandra/HRC-S and Swift/XRT observations for the 2015 outburst of the high-mass X-ray binary (HMXB) pulsar in the Small Magellanic Cloud, SMC X-2. While previous stud…

astro-ph.HE2016★ 19 cited

A Possible 55-day X-ray Period of the Ultraluminous Accreting Pulsar M82 X-2

A. K. H. Kong, C. -P. Hu, L. C. -C. Lin +4

We report a possible detection of a 55-day X-ray modulation for the ultraluminous accreting pulsar M82 X-2 from archival Chandra observations. Because M82 X-2 is known to have a 2.…

astro-ph.HE2015★ 17 cited

Long-term X-ray Variability of Ultraluminous X-ray Sources

L. C. -C. Lin, C. -P. Hu, A. K. H. Kong +3

Long-term X-ray modulations on timescales from tens to hundreds of days have been widely studied for X-ray binaries located in the Milky Way and the Magellanic Clouds. For other ne…

astro-ph.HE2015★ 18 cited

Searches for millisecond pulsar candidates among the unidentified Fermi objects

C. Y. Hui, S. M. Park, C. P. Hu +9

Here we report the results of searching millisecond pulsar (MSP) candidates from the Fermi LAT second source catalog (2FGL). Seven unassociated ray sources in this catalog are…

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★ 26 cited

Discovery of an ultracompact gamma-ray millisecond pulsar binary candidate

A. K. H. Kong, R. Jin, T. -C. Yen +8

We report multi-wavelength observations of the unidentified Fermi object 2FGL J1653.6-0159. With the help of high-resolution X-ray observation, we have identified an X-ray and opti…

astro-ph.HE2014★ 11 cited

Discovery of X-ray pulsations from "next Geminga" - PSR J1836+5925

L. C. C. Lin, C. Y. Hui, K. T. Li +5

We report the X-ray pulsation of ~173.3 ms for the "next Geminga", PSR J1836+5925, with recent XMM-Newton investigations. The X-ray periodicity is consistent wtih the gamma-ray eph…

astro-ph.HE2013★ 28 cited

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.HE2012★ 6 cited

Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106

C. Y. Hui, K. A. Seo, C. P. Hu +2

We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cat…