Beating the spin-down limit on gravitational wave emission from the crab pulsar (vol 683, pg L45, 2008)
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ASTROPHYSICAL JOURNAL LETTERS（2009）
引用 12|浏览83
摘要
A processing error in the signal template used in this search led to upper limits about 30% lower than we now know is warranted by the early S5 data. We have re-analyzed that data and find new upper limits on the strain parameter h(0) of 4.9 x 10(-25)/3.9 x 10(-25) for uniform/restricted prior assumptions concerning the Crab inclination and polarization angles. These results have now been superseded by upper limits of 2.6 x 10(-25)/2.0 x 10(-25) based on the full S5 data and presented in Abbott et al. (2009). The multitemplate search was not affected by the error.
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physics,astronomy
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