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20212026
most citedThe nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies

84 citations · 248 across the 20 of their papers we have counts for

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6 papers · 1 filter

astro-ph.HE2025★ 1 cited

Possible evidence for extended X-ray emission surrounding PSR B0656+14 with eROSITA

Shu Niu, Qiang Yuan, Shui-Nai Zhang +3

Extended very-high-energy -ray emission from middle-aged pulsars as revealed recently by several groundbased -ray experiments has strong implication on the transport of high-…

astro-ph.HE2024★ 1 cited

Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri

Yu-Xuan Chen, Lei Lei, Zi-Qing Xia +3

We investigate the production of axion-like particles (ALPs) in stellar cores, where they interact with electromagnetic fields and electrons, with typical masses between $\mathcal…

astro-ph.HE2023

Constraints Based on Non-detection of Kilonova Optical Searching

Runduo Liang, Zhengyan Liu, Lei Lei +1

Mergers of binary neutron stars are multimessenger sources of gravitational waves that have an optical luminous counterpart, commonly referred to as 'kilonova'. Inspired by the det…

astro-ph.HE2023★ 84 cited

The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies

Ziwei Wang, Lei Lei, Hao Jiao +2

Recently, pulsar timing array (PTA) experiments have provided compelling evidence for the existence of the nanohertz stochastic gravitational wave background (SGWB). In this work,…

astro-ph.HE2022★ 10 cited

GRB 080503: A very early blue kilonova and an adjacent non-thermal radiation component

Hao Zhou, Zhi-Ping Jin, Stefano Covino +5

The temporal behavior of the very dim optical afterglow of GRB 080503 is at odds with the regular forward shock afterglow model and a sole kilonova component responsible for optica…

astro-ph.HE2021★ 3 cited

A kilonova from an ultra-quick merger of a neutron star binary

Zhi-Ping Jin, Hao Zhou, Stefano Covino +6

GRB 060505 was the first well-known nearby (at redshift 0.089) "hybrid" gamma-ray burst that has a duration longer than 2 seconds but without the association of a supernova down to…