activity
20162023
most citedDiscovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT

129 citations · 282 across the 10 of their papers we have counts for

collaborators

14 papers

astro-ph.CO2023★ 9 cited

Forecasts of CMB lensing reconstruction of AliCPT-1 from the foreground cleaned polarization data

Jiakang Han, Bin Hu, Shamik Ghosh +14

Cosmic microwave background radiation (CMB) observations are unavoidably contaminated by emission from various extra-galactic foregrounds, which must be removed to obtain reliable…

astro-ph.HE2022★ 11 cited

Gamma-Ray Polarimetry of the Crab Pulsar Observed by POLAR

Han-Cheng Li, Nicolas Produit, Shuang-Nan Zhang +15

The X/ ray polarimetry of the Crab pulsar/nebula is believed to hold crucial information on their emission models. In the past, several missions have shown evidence of polarized…

astro-ph.HE2021

Polarization measurements of the Crab Pulsar with POLAR

Hancheng Li, POLAR Collaboration

POLAR is a dedicated Gamma-Ray Burst polarimeter making use of Compton-scattering which took data from the second Chinese spacelab, the Tiangong-2 from September 2016 to April 2017…

astro-ph.HE2020★ 129 cited

Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT

Xiang Ma, Lian Tao, Shuang-Nan Zhang +119

Low-frequency quasi-periodic oscillations (LFQPOs) are commonly found in black hole X-ray binaries, and their origin is still under debate. The properties of LFQPOs at high energie…

astro-ph.HE2020★ 79 cited

The POLAR Gamma-Ray Burst Polarization Catalog

Merlin Kole, Nicolas De Angelis, Francesco Berlato +18

Despite over 50 years of research, many open questions remain about the origin and nature of GRBs. Polarization measurements of the prompt emission of these extreme phenomena have…

astro-ph.IM2019★ 4 cited

Phase-resolved gamma-ray spectroscopy of the Crab pulsar observed by POLAR

Han-Cheng Li, Neal Gauvin, Ming-Yu Ge +15

The POLAR detector is a space based Gamma-Ray Burst (GRB) polarimeter sensitive in the 15-500 keV energy range. Apart from its main scientific goal as a Gamma-Ray Burst polarimeter…