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The present gravitational wave detection effort

dc.contributor.authorRiles, Keithen_US
dc.contributor.authorthe Ligo Scientific Collaborationen_US
dc.contributor.authorthe Virgo Scientific Collaborationen_US
dc.date.accessioned2011-08-10T13:53:40Z
dc.date.available2011-08-10T13:53:40Z
dc.date.issued2010-01en_US
dc.identifier.citationRiles, Keith; the Ligo Scientific Collaboration; the Virgo Scientific Collaboration (2010). "The present gravitational wave detection effort." Journal of Physics: Conference Series, 203(): 012002. <http://hdl.handle.net/2027.42/85430>en_US
dc.identifier.issn1742-6596en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/85430
dc.description.abstractGravitational radiation offers a new non-electromagnetic window through which to observe the universe. The LIGO and Virgo Collaborations have completed a first joint data run with unprecedented sensitivities to gravitational waves. Results from searches in the data for a variety of astrophysical sources are presented. A second joint data run with improved detector sensitivities is underway, and soon major upgrades will be carried out to build Advanced LIGO and Advanced Virgo with expected improvements in event rates of more than 1000. In parallel there is a vigorous effort in the radio pulsar community to detect nHz gravitational waves via the timing residuals in an array of pulsars at different locations in the sky.en_US
dc.titleThe present gravitational wave detection efforten_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/85430/1/jpconf10_203_012002.pdf
dc.identifier.doi10.1088/1742-6596/203/1/012002en_US
dc.identifier.sourceJournal of Physics: Conference Seriesen_US
dc.owningcollnamePhysics, Department of


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