activity
20162022
most citedAccretion disks and coronae in the X-ray flashlight

92 citations · 95 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.HE20223 cited

A giant glitch from the magnetar SGR J1935+2154 before FRB 200428

Mingyu Ge, Yuan-Pei Yang, Fangjun Lu +11

Fast radio bursts (FRBs) are short pulses observed in radio frequencies usually originating from cosmological distances. The discovery of FRB 200428 and its X-ray counterpart from…

astro-ph.HE2022

Radio pulsations from a neutron star within the gamma-ray binary LS I +61 303

Shan-Shan Weng, Lei Qian, Bo-Jun Wang +9

LS I +61 303 is one of the rare gamma-ray binaries, emitting most of their luminosity in photons with energies beyond 100 MeV. The 26.5 d orbital period is clearly…

cs.CV2019

PSDNet and DPDNet: Efficient channel expansion, Depthwise-Pointwise-Depthwise Inverted Bottleneck Block

Guoqing Li, Meng Zhang, Qianru Zhang +7

In many real-time applications, the deployment of deep neural networks is constrained by high computational cost and efficient lightweight neural networks are widely concerned. In…

astro-ph.HE2018

Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

The IceCube, Fermi-LAT, MAGIC +13

Individual astrophysical sources previously detected in neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neut…

astro-ph.HE201792 cited

Accretion disks and coronae in the X-ray flashlight

N. Degenaar, D. R. Ballantyne, T. Belloni +10

Plasma accreted onto the surface of a neutron star can ignite due to unstable thermonuclear burning and produce a bright flash of X-ray emission called a Type-I X-ray burst. Such e…

cs.CV2016

Visual Saliency Based on Scale-Space Analysis in the Frequency Domain

Jian Li, Martin Levine, Xiangjing An +2

We address the issue of visual saliency from three perspectives. First, we consider saliency detection as a frequency domain analysis problem. Second, we achieve this by employing…