activity
20092022
most citedA Candidate Young Massive Planet in Orbit around the Classical T Tauri Star CI Tau

108 citations · 306 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2022

Flare Quasi-Periodic Pulsation Associated with Recurrent Jets

Dong Li, Fanpeng Shi, Haisheng Zhao +6

Quasi-periodic pulsations (QPPs), which carry time features and plasma characteristics of flare emissions, are frequently observed in light curves of solar/stellar flares. In this…

astro-ph.SR2022★ 21 cited

Quasi-periodic Accelerations of Energetic Particles during a Solar Flare

Dong Li, Wei Chen

We report the observation of non-stationary Quasi-Periodic Pulsations (QPPs) in high-energy particles during the impulsive phase of an X4.8 flare on 2002 July 23 (SOL2002-07-23T00:…

astro-ph.HE2021★ 12 cited

GECAM detection of a bright type-I X-ray burst from 4U 0614+09: confirmation its spin frequency at 413 Hz

Y. P. Chen, J. Li, S. L. Xiong +87

One month after launching Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM), a bright thermonuclear X-ray burst from 4U~0614+09, was observed on Ja…

astro-ph.IM2020★ 4 cited

The influence of the Insight-HXMT/LE time response on timing analysis

Deng-Ke Zhou, Shi-Jie Zheng, Li-Ming Song +28

LE is the low energy telescope of Insight-HXMT. It uses swept charge devices (SCDs) to detect soft X-ray photons. The time response of LE is caused by the structure of SCDs. With t…

astro-ph.HE2017★ 24 cited

Determine the Lorentz factor and the viewing angle of GRB 170817A

Yuan-Chuan Zou, Fei-Fei Wang, Reetanjali Moharana +5

GRB 170817A is a weak short gamma-ray burst (GRB) accompanied by the gravitational wave (GW) event GW170817. It is believed, that an off beaming relativistic jet, produces this wea…

astro-ph.HE2017★ 30 cited

Bright "Merger-nova" Emission Powered by Magnetic wind from a New-Born Black Hole

Shuai-Bing Ma, Wei-Hua Lei, He Gao +4

Mergers of neutron star-neutron star (NS-NS) or neutron star-black hole (NS-BH) binaries are candidate sources of gravitational waves (GWs). At least a fraction of the merger remna…

astro-ph.HE2017★ 49 cited

Signature of a New-Born Black Hole from the Collapse of a Supra-massive Millisecond Magnetar

Wei Chen, Wei Xie, Wei-Hua Lei +5

The X-ray plateau followed by a steep decay ("internal plateau") has been observed in both long and short gamma-ray burst (GRBs), implying a millisecond magnetar operating in some…

astro-ph.EP2016★ 14 cited

H-alpha Variability in PTFO8-8695 and the Possible Direct Detection of Emission from a 2 Million Year Old Evaporating Hot Jupiter

Christopher M. Johns-Krull, Lisa Prato, Jacob N. McLane +9

We use high time cadence, high spectral resolution optical observations to detect excess H-alpha emission from the 2 - 3 Myr old weak lined T Tauri star PTFO8-8695. This excess emi…

astro-ph.EP2016★ 108 cited

A Candidate Young Massive Planet in Orbit around the Classical T Tauri Star CI Tau

Christopher M. Johns-Krull, Jacob N. McLane, L. Prato +10

The ~2 Myr old classical T Tauri star CI Tau shows periodic variability in its radial velocity (RV) variations measured at infrared (IR) and optical wavelengths. We find that these…

astro-ph.HE2014★ 12 cited

GRB 131231A: Implications of the GeV emission

Bin Liu, Wei Chen, Yun-Feng Liang +7

GRB 131231A was detected by the Large Area Telescope onboard Fermi Space Gamma-ray Telescope. The high energy gamma-ray ( MeV) afterglow emission spectrum is $F_ν\propto ν^{…

astro-ph.SR2013★ 23 cited

Magnetically Controlled Accretion on the Classical T Tauri Stars GQ Lupi and TW Hydrae

C. M. Johns-Krull, W. Chen, J. A. Valenti +8

We present high spectral resolution () Stokes polarimetry of the Classical T Tauri stars (CTTSs) GQ Lup and TW Hya obtained with the polarimetric upgrade to th…

astro-ph.HE2009★ 9 cited

Phase-resolved spectral analysis of 4U 1901+03 during its outburst

Ya-Juan Lei, Wei Chen, Jin-Lu Qu +5

The high mass X-ray binary 4U 1901+03 was reported to have the pulse profile evolving with the X-ray luminosity and energy during its outburst in February-July 2003: the pulse peak…