supported by the National Natural Science Foundation of China(Grant Nos.10821061 and10833003)
A digital pulsar backend based on a Field Programmable Gate Array (FPGA) is developed. It is designed for incoherent de-dispersion of pulsar observations and has a maximum bandwidth of 512MHz. The channel bandwidth ...
supported by China Ministry of Science and Technology(Grant No.2013CB837900);the National Natural Science Foundationof China(Grant Nos.10833003,11003023,11273029 and 11261140641)
Pulsar hulling is a phenomenon of sudden cessation of pulse emission for a number of periods. The nulling fraction was often used to characterize the phenomenon. We propose a new method to analyse pulsar hulling pheno...
supported by the National Natural Science Foundation of China (Grant Nos. Y011091001,11003023 and 10833003)
Repeated scatterings of unpolarized photons by non-relativistic electrons in a static and uniform magnetic field are investigated by using the Boltzmann equation with quantum mechanical correction factors for the stim...
Supported by the National Natural Science Foundation of China(Grant Nos. 10821061, 10833003 and 11103032);Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences and the National Key Basic Research Science Foundation of China (2007CB815403);Funding for SDSS-III has been provided by the Alfred P.Sloan Foundation,the Participating Institutions,the National Science Foundation and the U.S.Department of Energy
We identify new strong lensing clusters of galaxies from the Sloan Digital Sky Survey Ⅲ (SDSS DR8) by visually inspecting color images of a large sample of clusters of galaxies. We find 68 new clusters showing gian...
supported by the National Natural Science Foundation of China(Grant Nos.10803009,10833003 and 11073030)
Distance measurement of gamma-ray pulsars is a current challenge in pulsar studies.The Large Area Telescope(LAT) aboard the Fermi gamma-ray observatory discovered more than 70 gamma-ray pulsars including 24 new gamm...
supported by the National Natural Science Foundation of China (Grant Nos. 10773016, 10821001 and 10833003);the Initialization Fund for President Award Winner of Chinese Academy of Sciences
Radio detection of pulsars in the Galactic disk is strongly affected by the dispersion and scattering effect of the interstellar medium and the Galactic background radio emission. In order to know the best conditions ...