activity
20042026
most citedPhysical processes shaping GRB X-ray afterglow lightcurves: theoretical implications from the Swift XRT observations

1.1k citations · 8.3k across the 171 of their papers we have counts for

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Showing 2016Show all

14 papers · 1 filter

astro-ph.HE2016★ 12 cited

Testing the dark matter subhalo hypothesis of the gamma-ray source 3FGL J2212.5+0703

Yuan-Peng Wang, Kai-Kai Duan, Peng-Xiong Ma +8

N-body simulations predict that galaxies at the Milky Way scale host a large number of dark matter (DM) subhalos. Some of these subhalos, if they are massive enough or close enough…

astro-ph.HE2016★ 15 cited

Neutron star-black hole coalescence rate inferred from macronova/kilonova observations

Xiang Li, Yi-Ming Hu, Zhi-Ping Jin +2

Neutron starblack hole (NSBH) coalescences are widely believed to be promising gravitational wave sources in the era of advanced detectors of LIGO/Virgo but such binaries hav…

astro-ph.HE2016★ 14 cited

3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?

Zi-Qing Xia, Kai-Kai Duan, Shang Li +8

Milky Way-like galaxies are predicted to host a very large number of dark matter subhalos. Some massive and nearby subhalos could generate detectable gamma-rays, appearing as unide…

astro-ph.HE2016★ 23 cited

Evaluating the bulk Lorentz factors of outflow material: lessons learned from the extremely-energetic outburst GRB 160625B

Yuan-Zhu Wang, Hao Wang, Shuai Zhang +6

GRB 160625B is an extremely-bright outburst with well-monitored afterglow emission. The geometry-corrected energy is high up to erg or even $\sim 8\times 10…

astro-ph.HE2016★ 220 cited

Possible dark matter annihilation signal in the AMS-02 antiproton data

Ming-Yang Cui, Qiang Yuan, Yue-Lin Sming Tsai +1

Using the latest AMS-02 cosmic ray antiproton flux data, we search for potential dark matter annihilation signal. The background parameters about the propagation, source injection,…

astro-ph.HE2016★ 11 cited

HESS J1427-608: an unusual hard unbroken ray spectrum in a very wide energy range

Xiao-Lei Guo, Yu-Liang Xin, Neng-Hui Liao +5

We report the detection of a GeV -ray source which is spatially overlapping and thus very likely associated with the unidentified very-high-energy (VHE) -ray source HESS J142…

astro-ph.HE2016★ 14 cited

Search for gamma-ray line features from Milky Way satellites with Fermi-LAT Pass 8 data

Yun-Feng Liang, Zi-Qing Xia, Zhao-Qiang Shen +7

With 91 months of the publicly available Fermi-LAT Pass 8 data, we analyze the gamma-ray emission from the Milky Way satellites to search for potential line signals due to the anni…

hep-ph2016★ 5 cited

Interpretations of the possible 42.7 GeV -ray line

Lei Feng, Yun-Feng Liang, Tie-Kuang Dong +1

Recently Liang et al. found a tentative line signal at about 43 GeV in the directions of sixteen nearby Galaxy Clusters. If arising from dark matter annihilation, the mass of the d…

hep-ph2016★ 2 cited

-ray emission signals in the massive graviton mediated dark matter model

Cun Zhang, Ming-Yang Cui, Lei Feng +2

Dark matter may interact with Standard Model (SM) particle through the exchange of a massive spin-2 graviton producing signals that can be detected. In this work we examine the …

astro-ph.HE2016★ 19 cited

Discovery of -ray emission from the radio-intermediate quasar III Zw 2: violent jet activity with intraday -ray variability

Neng-Hui Liao, Yu-Liang Xin, Xu-Liang Fan +4

III Zw 2 is the prototype of radio-intermediate quasars. Although there is the evidence of possessing strong jet, significant -ray emission has not been reported before. In this…

astro-ph.HE2016★ 215 cited

The Macronova in GRB 050709 and the GRB/macronova connection

Zhi-Ping Jin, Kenta Hotokezaka, Xiang Li +6

GRB 050709 was the first short Gamma-ray Burst (sGRB) with an identified optical afterglow. In this work we report a re-analysis of the publicly available data of this event and th…

astro-ph.HE2016★ 52 cited

Search for a gamma-ray line feature from a group of nearby Galaxy clusters with Fermi LAT Pass 8 data

Yun-Feng Liang, Zhao-Qiang Shen, Xiang Li +6

Galaxy clusters are the largest gravitationally bound objects in the universe and may be suitable targets for indirect dark matter searches. With 85 months of Fermi-LAT Pass 8 publ…

astro-ph.HE2016★ 49 cited

Implications of the Tentative Association between GW150914 and a {\it Fermi}-GBM Transient

Xiang Li, Fu-Wen Zhang, Qiang Yuan +4

The merger-driven Gamma-ray Bursts (GRBs) and their associated gravitational wave (GW) radiation, if both successfully detected, have some far-reaching implications, including for…

astro-ph.HE2016★ 38 cited

GRB/GW association: Long-short GRB candidates, time-lag, measuring gravitational wave velocity and testing Einstein's equivalence principle

Xiang Li, Yi-Ming Hu, Yi-Zhong Fan +1

Short-duration gamma-ray bursts (SGRBs) are widely believed to be powered by the mergers of compact binaries, such as binary neutron stars or possibly neutron star-black hole binar…