Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)]

Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s... week ending PHYSICAL REVIEW LETTERS 14 JULY 2017 PRL 119, 029901 (2017) Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)] B. P. Abbott et al. and et al. (Received 5 June 2017; published 11 July 2017) DOI: 10.1103/PhysRevLett.119.029901 In Fig. 1 of the Letter, we have plotted an estimator for Ω h , rather than Ω , where h ¼ 0.68 is the Hubble constant 0 0 0 divided by 100 km=s=Mpc. This is inconsistent with the legend of Fig. 1, which states that an estimator for Ω is plotted, as well as with the conventions used throughout the rest of the Letter. A new figure showing the estimator for Ω with h ¼ 0.68 is shown below. This does not affect any other result in the Letter. −5 x 10 ± 2 σ Ω 0 −2 −4 −6 20 30 40 50 60 70 80 Frequency (Hz) FIG. 1. We show the estimator for Ω in each frequency bin, along with 2σ error bars, in the frequency band that contains 99% of the sensitivity for α ¼ 0. The loss of sensitivity at around 65 Hz http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Physical Review Letters American Physical Society (APS)

Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)]

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Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)]

Abstract

week ending PHYSICAL REVIEW LETTERS 14 JULY 2017 PRL 119, 029901 (2017) Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)] B. P. Abbott et al. and et al. (Received 5 June 2017; published 11 July 2017) DOI: 10.1103/PhysRevLett.119.029901 In Fig. 1 of the Letter, we have plotted an estimator for Ω h , rather than Ω , where h ¼ 0.68 is the Hubble constant 0 0 0 divided by 100 km=s=Mpc. This is inconsistent with the legend of Fig. 1, which states that an estimator for Ω is plotted, as well as with the conventions used throughout the rest of the Letter. A new figure showing the estimator for Ω with h ¼ 0.68 is shown below. This does not affect any other result in the Letter. −5 x 10 ± 2 σ Ω 0 −2 −4 −6 20 30 40 50 60 70 80 Frequency (Hz) FIG. 1. We show the estimator for Ω in each frequency bin, along with 2σ error bars, in the frequency band that contains 99% of the sensitivity for α ¼ 0. The loss of sensitivity at around 65 Hz
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Publisher
The American Physical Society
Copyright
Copyright © © 2017 American Physical Society
ISSN
0031-9007
eISSN
1079-7114
D.O.I.
10.1103/PhysRevLett.119.029901
Publisher site
See Article on Publisher Site

Abstract

week ending PHYSICAL REVIEW LETTERS 14 JULY 2017 PRL 119, 029901 (2017) Erratum: Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run [Phys. Rev. Lett. 118, 121101 (2017)] B. P. Abbott et al. and et al. (Received 5 June 2017; published 11 July 2017) DOI: 10.1103/PhysRevLett.119.029901 In Fig. 1 of the Letter, we have plotted an estimator for Ω h , rather than Ω , where h ¼ 0.68 is the Hubble constant 0 0 0 divided by 100 km=s=Mpc. This is inconsistent with the legend of Fig. 1, which states that an estimator for Ω is plotted, as well as with the conventions used throughout the rest of the Letter. A new figure showing the estimator for Ω with h ¼ 0.68 is shown below. This does not affect any other result in the Letter. −5 x 10 ± 2 σ Ω 0 −2 −4 −6 20 30 40 50 60 70 80 Frequency (Hz) FIG. 1. We show the estimator for Ω in each frequency bin, along with 2σ error bars, in the frequency band that contains 99% of the sensitivity for α ¼ 0. The loss of sensitivity at around 65 Hz

Journal

Physical Review LettersAmerican Physical Society (APS)

Published: Jul 14, 2017

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