期刊
CLASSICAL AND QUANTUM GRAVITY
卷 27, 期 8, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/27/8/084013
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- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1009580, 0748580] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [0969857] Funding Source: National Science Foundation
- Office Of The Director
- Office Of Internatl Science &Engineering [0968296] Funding Source: National Science Foundation
- Science and Technology Facilities Council [ST/G002487/1, ST/F002874/1] Funding Source: researchfish
- STFC [ST/G002487/1, ST/F002874/1] Funding Source: UKRI
The International Pulsar Timing Array project combines observations of pulsars from both northern and southern hemisphere observatories with the main aim of detecting ultra-low frequency (similar to 10(-9)-10(-8) Hz) gravitational waves. Here we introduce the project, review the methods used to search for gravitational waves emitted from coalescing supermassive binary black-hole systems in the centres of merging galaxies and discuss the status of the project.
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