Erratum: "Beating The Spin-Down Limit On Gravitational Wave Emission From The Crab Pulsar"

LIGO Scientific Collaboration; S. Hild

doi:10.1088/0004-637X/706/1/L203

Erratum: "Beating The Spin-Down Limit On Gravitational Wave Emission From The Crab Pulsar"

LIGO Scientific Collaboration
, S. Hild

Research output: Contribution to journal › Erratum / corrigendum › Academic

Abstract

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 These results have now been superseded by upper limits of 2.6 x 10(-25)/2.0 x 10(-25) based on the full S5 data and presented in Abbott et al.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
Pages (from-to)	L203-L204
Number of pages	2
Journal	Astrophysical Journal Letters
Volume	706
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/706/1/L203
Publication status	Published - 20 Nov 2009
Externally published	Yes

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10.1088/0004-637X/706/1/L203

Beating the spin-down limit on gravitational wave emission from the Crab pulsar
LIGO Scientific Collaboration & Hild, S., 2008, In: Astrophysical Journal. 683, 1 PART 2, p. L45-L49
Research output: Contribution to journal › Article › Academic › peer-review

Cite this

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title = "Erratum: {"}Beating The Spin-Down Limit On Gravitational Wave Emission From The Crab Pulsar{"}",

abstract = "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 These results have now been superseded by upper limits of 2.6 x 10(-25)/2.0 x 10(-25) based on the full S5 data and presented in Abbott et al.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.",

author = "B. Abbott and R. Abbott and R. Adhikari and P. Ajith and B. Allen and G. Allen and R. Amin and S.B. Anderson and W.G. Anderson and M.A. Arain and M. Araya and H. Armandula and P. Armor and Y. Aso and S. Aston and P. Aufmuth and C. Aulbert and S. Babak and S. Ballmer and H. Bantilan and B.C. Barish and C. Barker and D. Barker and B. Barr and P. Barriga and M.A. Barton and M. Bastarrika and K. Bayer and J. Betzwieser and P.T. Beyersdorf and I.A. Bilenko and G. Billingsley and R. Biswas and E. Black and K. Blackburn and L. Blackburn and D. Blair and B. Bland and T.P. Bodiya and L. Bogue and R. Bork and V. Boschi and S. Bose and P.R. Brady and V.B. Braginsky and J.E. Brau and M. Brinkmann and A. Brooks and D.A. Brown and \{LIGO Scientific Collaboration\} and S. Hild",

year = "2009",

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doi = "10.1088/0004-637X/706/1/L203",

language = "English",

volume = "706",

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TY - JOUR

T1 - Erratum: "Beating The Spin-Down Limit On Gravitational Wave Emission From The Crab Pulsar"

AU - Abbott, B.

AU - Abbott, R.

AU - Adhikari, R.

AU - Ajith, P.

AU - Allen, B.

AU - Allen, G.

AU - Amin, R.

AU - Anderson, S.B.

AU - Anderson, W.G.

AU - Arain, M.A.

AU - Araya, M.

AU - Armandula, H.

AU - Armor, P.

AU - Aso, Y.

AU - Aston, S.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - Babak, S.

AU - Ballmer, S.

AU - Bantilan, H.

AU - Barish, B.C.

AU - Barker, C.

AU - Barker, D.

AU - Barr, B.

AU - Barriga, P.

AU - Barton, M.A.

AU - Bastarrika, M.

AU - Bayer, K.

AU - Betzwieser, J.

AU - Beyersdorf, P.T.

AU - Bilenko, I.A.

AU - Billingsley, G.

AU - Biswas, R.

AU - Black, E.

AU - Blackburn, K.

AU - Blackburn, L.

AU - Blair, D.

AU - Bland, B.

AU - Bodiya, T.P.

AU - Bogue, L.

AU - Bork, R.

AU - Boschi, V.

AU - Bose, S.

AU - Brady, P.R.

AU - Braginsky, V.B.

AU - Brau, J.E.

AU - Brinkmann, M.

AU - Brooks, A.

AU - Brown, D.A.

AU - LIGO Scientific Collaboration

AU - Hild, S.

PY - 2009/11/20

Y1 - 2009/11/20

N2 - 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.

AB - 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.

U2 - 10.1088/0004-637X/706/1/L203

DO - 10.1088/0004-637X/706/1/L203

M3 - Erratum / corrigendum

SN - 2041-8205

VL - 706

SP - L203-L204

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 1

ER -

Erratum: "Beating The Spin-Down Limit On Gravitational Wave Emission From The Crab Pulsar"

Abstract

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Research output

Beating the spin-down limit on gravitational wave emission from the Crab pulsar

Cite this