scholarly journals PRACTICAL METHODS FOR CONTINUOUS GRAVITATIONAL WAVE DETECTION USING PULSAR TIMING DATA

2012 ◽  
Vol 753 (2) ◽  
pp. 96 ◽  
Author(s):  
J. A. Ellis ◽  
F. A. Jenet ◽  
M. A. McLaughlin
2021 ◽  
Vol 911 (2) ◽  
pp. L34
Author(s):  
Nihan S. Pol ◽  
Stephen R. Taylor ◽  
Luke Zoltan Kelley ◽  
Sarah J. Vigeland ◽  
Joseph Simon ◽  
...  

Physics Today ◽  
2010 ◽  
Vol 63 (1) ◽  
pp. 62-63
Author(s):  
Paul Demorest ◽  
Joseph Lazio ◽  
Andrea Lommen

2005 ◽  
Vol 22 (3) ◽  
pp. 179-183 ◽  
Author(s):  
George Hobbs

AbstractThe number of known millisecond pulsars has dramatically increased in the last few years. Regular observations of these pulsars may allow gravitational waves with frequencies ∼10−9 Hz to be detected. A ‘pulsar timing array’ is therefore complimentary to other searches for gravitational waves using ground-based or space-based interferometers that are sensitive to much higher frequencies. In this review we describe (1) the basic methods for using an array of pulsars as a gravitational wave detector, (2) the sources of the potentially detectable waves, (3) current limits on individual sources and a stochastic background, and (4) the new project recently started using the Parkes radio telescope.


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