supported by the National Key R&D Program of China(2017YFA0402600);State Key DevelopmentProgram for Basic Research(2015CB857100);National Basic Research Program of China(973 program,No.2015CB857101);National Natural Science Foundation of China(Grant Nos.11703047,11773041,U1631132and U1831131);supported by the CAS“Light of West China”Program;by the CAS Key Laboratory of FAST,National Astronomical Observatories,Chinese Academy of Sciences;supported in part by the Youth Innovation Promotion Association of CAS(id.2018075)。
We developed a pulsar search pipeline based on PulsaR Exploration and Search TOolkit(PRESTO).This pipeline simply runs dedispersion,Fast Fourier Transform(FFT)and acceleration search in process-level parallel to short...
supported by the National Basic Research Program of China (973 program, Grant No. 2012CB821800);the National Natural Science Foundation of China (Grant Nos. 11573008, 11178001, 11225314, 11303069 and 11373011)
The Five-hundred-meter Aperture Spherical radio Telescope(FAST) has the potential to discover many new pulsars and new phenomena. In this paper we mainly concentrate on how FAST can impact study of the pulsar emission...
the support from the professorship award under the Chinese Academy of Sciences(CAS) President's International Fellowship Initiative(PIFI) in 2015;the support from the Guizhou Scientific Collaboration Program (No.20130421);the support from the National Natural Science Foundation of China(NSFC, Nos.11305133 and 11273020);the support from NSFC(No.Y411101N01)the support from NSFC(No.11103045);grants from NSFC (No.11373038);the support by National Basic Research Program of China(973 program) Nos.2012CB821800 and 2015CB57100
The Five-hundred-meter Aperture Spherical Telescope (FAST) will begin its early-science oper- ations during 2016. Drift-scan pulsar surveys will be carried out during this period using an ultra-wide-band receiver sy...
supported by the National Natural Science Foundation of China (Grant Nos. 10935001 and 10973002);the National Basic Research Program of China (973 program, Grant No. 2009CB824800);the China Postdoctoral Science Foundation and the John Templeton Foundation
It is conventionally thought that the state equation of dense matter softens and thus cannot result in high maximum mass if pulsars are quark stars and that a recently discovered 2M⊙ pulsar (PSR J1614–2230) may ma...