Erratum: Search for gravitational waves from binary black hole inspiral, merger, and ringdown [Phys. Rev. D83, 122005 (2011)]
J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
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J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
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J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
This paper was published online on 5 November 2010 with an omission in the Collaboration author list. S. Dwyer has been added as of 12 April 2012. The Collaboration author list is incorrect in the printed version of the journal
J. Abadie, B. P. Abbott, R. Abbott, R. X. Adhikari et autres
This paper was published online on 1 February 2011 with an omission in the Collaboration author list. S. Dwyer has been added as of 12 April 2012. The Collaboration author list is incorrect in the printed version of the journal.
J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
This paper was published online on 6 June 2011 with an omission in the Collaboration author list. S. Dwyer has been added as of 12 April 2012. The Collaboration author list is incorrect in the printed version of the journal.
J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. We perform two directional searches for persistent GWs using data from the LIGO S5 science run: one optimized for pointlike sources and one for arbitrary extended sources. Finding …
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B. P. Abbott, R. Abbott, M. R. Abernathy, T. Accadia et autres
The gravitational-wave (GW) sky may include nearby pointlike sources as well as astrophysical and cosmological stochastic backgrounds. Since the relative strength and angular distribution of the many possible sources of GWs are not well constrained, searches for GW signals must be performed …
J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio …
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J. Abadie, B. Abbott, R. Abbott, M. R. Abernathy et autres
We present the first modeled search for gravitational waves using the complete binary black-hole gravitational waveform from inspiral through the merger and ringdown for binaries with negligible component spin. We searched approximately 2 years of LIGO data, taken between November 2005 and …
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J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres
Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation …
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J. Abadie, B. P. Abbott, R. Abbott, R. X. Adhikari et autres
Not Available
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J. Abadie, B. P. Abbott, Robert Abbott, R. X. Adhikari et autres
J. Abadie, B. Abbott, R. Abbott, R. X. Adhikari et autres
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mode oscillations in their parent neutron star that couple to gravitational-wave emission. In August 2006, a timing glitch was observed in the radio emission of PSR B0833-45, the Vela …
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