Full band all-sky search for periodic gravitational waves in the O1 LIGO data

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Standard

Full band all-sky search for periodic gravitational waves in the O1 LIGO data. / LIGO Sci Collaboration; Virgo Collaboration.

In: Physical Review D, Vol. 97, No. 10, 102003, 11.05.2018.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

LIGO Sci Collaboration & Virgo Collaboration 2018, 'Full band all-sky search for periodic gravitational waves in the O1 LIGO data', Physical Review D, vol. 97, no. 10, 102003. https://doi.org/10.1103/PhysRevD.97.102003

APA

LIGO Sci Collaboration, & Virgo Collaboration (2018). Full band all-sky search for periodic gravitational waves in the O1 LIGO data. Physical Review D, 97(10), [102003]. https://doi.org/10.1103/PhysRevD.97.102003

Vancouver

LIGO Sci Collaboration, Virgo Collaboration. Full band all-sky search for periodic gravitational waves in the O1 LIGO data. Physical Review D. 2018 May 11;97(10). 102003. https://doi.org/10.1103/PhysRevD.97.102003

Author

LIGO Sci Collaboration ; Virgo Collaboration. / Full band all-sky search for periodic gravitational waves in the O1 LIGO data. In: Physical Review D. 2018 ; Vol. 97, No. 10.

Bibtex

@article{f89c01bed5f743d6a2f42160e4e6a254,
title = "Full band all-sky search for periodic gravitational waves in the O1 LIGO data",
abstract = "We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run 01. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is similar to 4 x 10(-25) near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 x 10(-24) . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is similar to 1.5 x 10(-25)",
author = "Anderson, {S. B.} and S. Ascenzi and B. Barr and Bell, {A. S.} and J. Birch and Brown, {D. A.} and Brown, {D. A.} and H. Cao and J. Cao and M. Chan and Chen, {H. Y.} and Diaz, {M. C.} and B. Farr and Farr, {W. M.} and Holz, {D. E.} and Wang, {W. H.} and Wang, {Y. F.} and Wei, {L. -W.} and Williams, {R. D.} and L. Yang and L. Zhang and Zhang, {Y. -H.} and C. Zhao and Zhu, {S. J.} and Zhu, {X. J.} and {LIGO Sci Collaboration} and {Virgo Collaboration}",
year = "2018",
month = may,
day = "11",
doi = "10.1103/PhysRevD.97.102003",
language = "English",
volume = "97",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "10",

}

RIS

TY - JOUR

T1 - Full band all-sky search for periodic gravitational waves in the O1 LIGO data

AU - Anderson, S. B.

AU - Ascenzi, S.

AU - Barr, B.

AU - Bell, A. S.

AU - Birch, J.

AU - Brown, D. A.

AU - Brown, D. A.

AU - Cao, H.

AU - Cao, J.

AU - Chan, M.

AU - Chen, H. Y.

AU - Diaz, M. C.

AU - Farr, B.

AU - Farr, W. M.

AU - Holz, D. E.

AU - Wang, W. H.

AU - Wang, Y. F.

AU - Wei, L. -W.

AU - Williams, R. D.

AU - Yang, L.

AU - Zhang, L.

AU - Zhang, Y. -H.

AU - Zhao, C.

AU - Zhu, S. J.

AU - Zhu, X. J.

AU - LIGO Sci Collaboration

AU - Virgo Collaboration

PY - 2018/5/11

Y1 - 2018/5/11

N2 - We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run 01. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is similar to 4 x 10(-25) near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 x 10(-24) . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is similar to 1.5 x 10(-25)

AB - We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0, +0.1] x 10(-8) Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run 01. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is similar to 4 x 10(-25) near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 x 10(-24) . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is similar to 1.5 x 10(-25)

U2 - 10.1103/PhysRevD.97.102003

DO - 10.1103/PhysRevD.97.102003

M3 - Journal article

VL - 97

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 10

M1 - 102003

ER -

ID: 258842332