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Massive black holes are key ingredients of the assembly and evolution of cosmic structures. Pulsar Timing Arrays (PTAs) currently provide the only means to observe gravitational radiation from massive...
The optical counterpart of sax j1808.4{3658 in quiescence:evidence of an active radio pulsar?
Preliminary results on intermittent behaviour of Millisecond pulsar sax j1808.4-3658。
The Pulsar Luminosity Function     Pulsar  Luminosity Function       font style='font-size:12px;'> 2009/6/16
The Pulsar Luminosity Function。
This paper describes the design, tests and preliminary results of a real-time parallel signal processor built to aid a wide variety of pulsar observations. The signal processor reduces the distortions...
Superorbital Period Variations in the X-ray Pulsar LMC X-4     accretion disks  neutron—X-rays:binaries       font style='font-size:12px;'> 2009/5/19
We report the discovery of a decay in the superorbital period of the binary X-ray pulsar LMC X-4. Combining archival data and published long term X-ray light curves, we have found a decay in the thi...
We present spectral variations of the binary X-ray pulsar LMC X-4 observed with the RXTE/PCA during different phases of its 30.5 day long third period. Only out-of-eclipse data were used for this st...

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