funded by the National Natural Science Foundation of China (Grant Nos.11373028,U1531112,91736207,11873050, 11873049 and U1831130);the A Project of the Young Scholar of the “West Light” of the Chinese Academy of Sciences (XAB2015A06);the Cultivation Fund of Xi’an University of Science and Technology (No. 201707)
Employing multiple pulsars and using an appropriate algorithm to establish ensemble pulsar timescale can reduce the influences of various noises on the long-term stability of pulsar timescale,compared to a single puls...
supported by the National Natural Science Foundation of China(Grant Nos.11103024,11373028 and 11403030);the Science and Technology Research Development Program of Shaanxi Province;the CAS“Light of West China”Program;the Open Project of Key Laboratory for Research in Galaxies and Cosmology,Chinese Academy of Sciences(Grant No.14010205)
Relic gravitational waves (RGWs), a background originating during inflation, would leave imprints on pulsar timing residuals. This makes RGWs an important source for detection of RGWs using the method of pulsar timi...