The single pulse observation of PSR J1752+2359 at 1250 MHz made using the Five-hundred-meter Aperture Spherical radio Te......

Discovery of pulsars is one of the main goals for large radio telescopes.The Five-hundred-meter Aperture Spherical radio......

Pulsar timing is a classic technology of detecting irregularities in pulsar rotation.We carried out this method for 18 y......

Pulsars are very stable spinning stars,which have the potential to application in the work of time-keeping and autonomou......

PSR J0742-2822 is known for its quasi-periodic changes in the observed pulse profile and spin-down rate.In this paper,we......

It is conjectured that coherent re-emission of cyclotron resonance absorption could result in pulsar giant pulses.This c......

Discovery of pulsars is one of the main goals for large radio telescopes.The Five-hundredmeter Aperture Spherical radio ......

We investigated the pulsar radio luminosity(L),emission efficiency(ratio of radio luminosity to its spin-down power E),a......

Radio frequency interference(RFI)is an important challenge in radio astronomy.RFI comes from various sources and increas......

The form of timing residuals due to errors in pulsar spin period P and its derivative P, in positions, as well as in pro......

Pulsars are very stable spinning stars, which have the potential to application in the work of time-keeping and autonomo......

脉冲星数据比对分析和可视化系统(PSRDB,URL:http://www.psrdb.net/),由FAST(Five-hundred-meter Aperture Spherical Radio Teles......

One large glitch was detected in PSR B1737-30 using data spanning from MJD 57999 to 58406 obtained with the newly built ......

As the performance of dedicated facilities has continually improved, large numbers of pulsar candidates are being receiv......

The Five-hundred-meter Aperture Spherical radio Telescope(FAST) has the potential to discover many new pulsars and new p......

We perform a search for gravitational waves(GWs) from several supermassive binary black hole(SMBBH) candidates(NGC 5548,......