activity
20092021
most citedEvidence for CP violation in time-integrated D0 -> h-h+ decay rates

224 citations · 2.8k across the 41 of their papers we have counts for

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Showing astro-ph.IMShow all

7 papers · 1 filter

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…

astro-ph.IM2018★ 20 cited

In-Orbit Instrument Performance Study and Calibration for POLAR Polarization Measurements

Zhengheng Li, Merlin Kole, Jianchao Sun +30

POLAR is a compact space-borne detector designed to perform reliable measurements of the polarization for transient sources like Gamma-Ray Bursts in the energy range 50-500keV. The…

astro-ph.IM2017★ 58 cited

Design and construction of the POLAR detector

N. Produit, T. W. Bao, T. Batsch +35

The POLAR detector is a space based Gamma Ray Burst (GRB) polarimeter with a wide field of view, which covers almost half the sky. The instrument uses Compton scattering of gamma r…

astro-ph.IM2017★ 24 cited

Instrument Performance and Simulation Verification of the POLAR Detector

M. Kole, Z. H. Li, N. Produit +32

POLAR is a new satellite-born detector aiming to measure the polarization of an unprecedented number of Gamma-Ray Bursts in the 50-500 keV energy range. The instrument, launched on…

astro-ph.IM2017

Gain factor and parameter settings optimization of the new gamma-ray burst polarimeter POLAR

X. F. Zhang, W. Hajdas, H. L. Xiao +38

As a space-borne detector POLAR is designed to conduct hard X-ray polarization measurements of gamma-ray bursts on the statistically significant sample of events and with an unprec…

astro-ph.IM2016

POLAR: Final Calibration and In-Flight Performance of a Dedicated GRB Polarimeter

M. Kole, T. W. Bao, T. Batsch +41

Gamma-ray polarimetry is a new powerful tool to study the processes responsible for the emission from astrophysical sources and the environments in which this emission takes place.…