activity
20152025
most citedSearching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

76 citations · 428 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2025★ 16 cited

A pulsar-helium star compact binary system formed by common envelope evolution

Z. L. Yang, J. L. Han, D. J. Zhou +33

A stellar common envelope occurs in a binary system when the atmosphere of an evolving star expands to encompass an orbiting companion object. Such systems are predicted to evolve…

astro-ph.HE2024★ 6 cited

Massive stars exploding in a He-rich circumstellar medium X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt

Z. -Y. Wang, A. Pastorello, K. Maeda +48

We present optical and near-infrared observations of two Type Ibn supernovae (SNe), SN 2018jmt and SN 2019cj. Their light curves have rise times of about 10 days, reaching an absol…

astro-ph.HE2024

Investigation of profile shifting and subpulse movement in PSR J0344-0901 with FAST

H. M. Tedila, R. Yuen, N. Wang +13

We report two phenomena detected in PSR J03440901 from two observations conducted at frequency centered at 1.25 GHz using the Five-hundred-meter Aperture Spherical radio Telesco…

astro-ph.HE2024

Pulse Jitter and Single-pulse Variability in Millisecond Pulsars

S. Q. Wang, N. Wang, J. B. Wang +8

Understanding the jitter noise resulting from single-pulse phase and shape variations is important for the detection of gravitational waves using pulsar timing array. We presented…

astro-ph.HE2023

Discovery of four pulsars in a pilot survey at intermediate Galactic latitudes with FAST

Q. J. Zhi, J. T. Bai, S. Dai +21

We present the discovery and timing results of four pulsars discovered in a pilot survey at intermediate Galactic latitudes with the Five-hundred Aperture Spherical Telescope (FAST…

astro-ph.HE2023

Wide Bandwidth Observations of PSR J094139 and PSR J11075907

S. N. Sun, N. Wang, W. M. Yan +2

We present a polarization analysis of PSR J094139 and PSR J11075907, which exhibit transitions between being pulsars and rotating radio transients (RRATs), using the ultra-wi…

gr-qc2023★ 76 cited

Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

M. Falxa, S. Babak, P. T. Baker +123

The International Pulsar Timing Array 2nd data release is the combination of datasets from worldwide collaborations. In this study, we search for continuous waves: gravitational wa…

astro-ph.HE2022★ 25 cited

Arecibo and FAST Timing Follow-up of twelve Millisecond Pulsars Discovered in Commensal Radio Astronomy FAST Survey

C. C. Miao, W. W. Zhu, D. Li +46

We report the phase-connected timing ephemeris, polarization pulse profiles, Faraday rotation measurements, and Rotating-Vector-Model (RVM) fitting results of twelve millisecond pu…

hep-th2022★ 16 cited

Emission Variation of a Long-period Pulsar Discovered by the Five-hundred-meter Aperture Spherical Radio Telescope (FAST)

H. M. Tedila, R. Yuen, N. Wang +16

We report on the variation in the single-pulse emission from PSR J1900+4221 (CRAFTS 19C10) observed at frequency centered at 1.25 GHz using the Five-hundred-meter Aperture Spherica…

astro-ph.HE2021★ 22 cited

Unusual Emission Variations Near the Eclipse of A Black Widow PSR J17200533

S. Q. Wang, J. B. Wang, N. Wang +15

We report on an {unusually} bright observation of PSR J17200533 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar is in a black widow system tha…

astro-ph.HE2021★ 14 cited

A single pulse study of a millisecond pulsar PSR J0621+1002

S. Q. Wang, J. B. Wang, N. Wang +8

We present radio observation of a millisecond pulsar PSR J0621+1002 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar shows periodic pulse intensit…

astro-ph.HE2020★ 12 cited

The two emission states of PSR B1534+12

S. Q. Wang, G. Hobbs, J. B. Wang +10

We have observed PSR~B1534+12 (J1537+1155), a pulsar with a neutron star companion, using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). We found that this pulsa…

astro-ph.HE2020★ 16 cited

Radio observations of two intermittent pulsars: PSRs J1832+0029 and J1841-0500

S. Q. Wang, J. B. Wang, G. Hobbs +8

We present long-term observations of two intermittent pulsars, PSRs~J1832+0029 and J18410500 using the Parkes 64\,m radio telescope. The radio emission for these pulsars switche…

astro-ph.HE2020★ 14 cited

Parkes transient events: I. Database of single pulses, initial results and missing FRBs

S. -B. Zhang, G. Hobbs, C. J. Russell +16

A large number of observations from the Parkes 64\,m-diameter radio telescope, recorded with high time resolution, are publicly available. We have re-processed all of the observati…

astro-ph.HE2017★ 27 cited

Broad-lined type Ic supernova iPTF16asu: A challenge to all popular models

L. J. Wang, X. F. Wang, Z. Cano +9

It is well-known that ordinary supernovae (SNe) are powered by 56Ni cascade decay. Broad-lined type Ic SNe (SNe Ic-BL) are a subclass of SNe that are not all exclusively powered by…

astro-ph.HE2017★ 12 cited

A Monte Carlo approach to magnetar-powered transients: II. Broad-lined type Ic supernovae not associated with GRBs

Ling-Jun Wang, Zach Cano, Shan-Qin Wang +11

Broad-lined type Ic supernovae (SNe Ic-BL) are a subclass of rare core collapse SNe whose energy source is debated in the literature. Recently a series of investigations on SNe Ic-…

astro-ph.HE2016★ 30 cited

Evidence for magnetar formation in broad-lined type Ic supernovae 1998bw and 2002ap

L. J. Wang, H. Yu, L. D. Liu +6

Broad-lined type Ic supernovae (SNe Ic-BL) are peculiar stellar explosions that distinguish themselves from ordinary SNe. Some SNe Ic-BL are associated with long-duration (\gtrsim…

astro-ph.HE2016★ 29 cited

Optical Transients Powered by Magnetars: Dynamics, Light Curves, and Transition to the Nebular Phase

L. J. Wang, S. Q. Wang, Z. G. Dai +4

Millisecond magnetars can be formed via several channels: core-collapse of massive stars, accretion-induced collapse of white dwarfs (WDs), double WD mergers, double neutron star (…

astro-ph.HE2015★ 45 cited

A Triple-Energy-Source Model for Superluminous Supernova iPTF13ehe

S. Q. Wang, L. D. Liu, Z. G. Dai +2

Almost all superluminous supernovae (SLSNe) whose peak magnitudes are mag can be explained by the Ni-powered model, magnetar-powered (highly magnetized pulsar…

astro-ph.HE2015★ 68 cited

The Most Luminous Supernova ASASSN-15lh: Signature of a Newborn Rapidly-Rotating Strange Quark Star

Z. G. Dai, S. Q. Wang, J. S. Wang +2

In this paper we show that the most luminous supernova discovered very recently, ASASSN-15lh, could have been powered by a newborn ultra-strongly-magnetized pulsar, which initially…