Abstract
This is an Erratum for the article 2008 ApJ 683 L45
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 These results have now been superseded by upper limits of 2.6 x 10(-25)/2.0 x 10(-25) based on the full S5 data and presented in Abbott et al.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.
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 These results have now been superseded by upper limits of 2.6 x 10(-25)/2.0 x 10(-25) based on the full S5 data and presented in Abbott et al.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.
Original language | English |
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Pages (from-to) | L203-L204 |
Number of pages | 2 |
Journal | Astrophysical Journal |
Volume | 706 |
Issue number | 1 |
DOIs | |
Publication status | Published - 20 Nov 2009 |
Keywords
- astroparticles
- cosmology
- gravitation
- astrophysics
- Crab pulsar