Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Autoren

  • The LIGO Scientific Collaboration
  • Virgo Collaboration
  • Sukanta Bose
  • D. D. Brown
  • Y. B. Chen
  • Manuela Hanke
  • J. Hennig
  • Sanjeev Kumar
  • R. N. Lang
  • H. K. Lee
  • H. M. Lee
  • H. W. Lee
  • J. Lee
  • X. Li
  • J. R. Sanders
  • Patricia Schmidt
  • L. Sun
  • Y. F. Wang
  • D. S. Wu
  • L. Zhang
  • X. J. Zhu
  • Minchuan Zhou
  • Gerald Bergmann
  • Aparna Bisht
  • Nina Bode
  • P. Booker
  • Marc Brinkmann
  • M. Cabero
  • O. de Varona
  • S. Hochheim
  • T. Dent
  • S. Doravari
  • J. Junker
  • Stefan Kaufer
  • Kai S. Karvinen
  • S. Khan
  • R. Kirchhoff
  • Patrick Koch
  • N. Koper
  • S. M. Köhlenbeck
  • Volker Kringel
  • G. Kuehn
  • S. Leavey
  • J. Lehmann
  • James Lough
  • Moritz Mehmet
  • J. Mukherjee
  • Arunava Mukherjee
  • Nikhil Mukund
  • M. Nery
  • F. Ohme
  • P. Oppermann
  • A. Rüdiger
  • M. Phelps
  • O. Puncken
  • Emil Schreiber
  • B. W. Schulte
  • Y. Setyawati
  • M. Steinke
  • M. Standke
  • Fabian Thies
  • Michael Weinert
  • F. Wellmann
  • Peter Weßels
  • Maximilian H. Wimmer
  • W. Winkler
  • J. Woehler

Organisationseinheiten

Externe Organisationen

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Inter-University Centre for Astronomy and Astrophysics India
  • University of Adelaide
  • Tata Institute of Fundamental Research (TIFR HYD)
  • LIGO Laboratory
  • Inje University
  • California Institute of Technology (Caltech)
  • Radboud Universität Nijmegen (RU)
  • University of Melbourne
  • University of Texas Rio Grande Valley
  • Monash University
  • Northwestern University
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer122
Seitenumfang15
FachzeitschriftAstrophysical Journal
Jahrgang875
Ausgabenummer2
PublikationsstatusVeröffentlicht - 23 Apr. 2019

Abstract

We describe directed searches for continuous gravitational waves (GWs) from 16 well-localized candidate neutron stars, assuming none of the stars has a binary companion. The searches were directed toward 15 supernova remnants and Fomalhaut b, a directly imaged extrasolar planet candidate that has been suggested to be a nearby old neutron star. Each search covered a broad band of frequencies and first and second time derivatives. After coherently integrating spans of data from the first Advanced LIGO observing run of 3.5-53.7 days per search, applying data-based vetoes, and discounting known instrumental artifacts, we found no astrophysical signals. We set upper limits on intrinsic GW strain as strict as 1 ×10 -25, fiducial neutron star ellipticity as strict as 2 ×10 -9, and fiducial r-mode amplitude as strict as 3 ×10 -8.

ASJC Scopus Sachgebiete

Zitieren

Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO. / The LIGO Scientific Collaboration; Virgo Collaboration; Bose, Sukanta et al.
in: Astrophysical Journal, Jahrgang 875, Nr. 2, 122, 23.04.2019.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

The LIGO Scientific Collaboration, Virgo Collaboration, Bose, S, Brown, DD, Chen, YB, Hanke, M, Hennig, J, Kumar, S, Lang, RN, Lee, HK, Lee, HM, Lee, HW, Lee, J, Li, X, Sanders, JR, Schmidt, P, Sun, L, Wang, YF, Wu, DS, Zhang, L, Zhu, XJ, Zhou, M, Bergmann, G, Bisht, A, Bode, N, Booker, P, Brinkmann, M, Cabero, M, de Varona, O, Hochheim, S, Dent, T, Doravari, S, Junker, J, Kaufer, S, Karvinen, KS, Khan, S, Kirchhoff, R, Koch, P, Koper, N, Köhlenbeck, SM, Kringel, V, Kuehn, G, Leavey, S, Lehmann, J, Lough, J, Mehmet, M, Mukherjee, J, Mukherjee, A, Mukund, N, Nery, M, Ohme, F, Oppermann, P, Rüdiger, A, Phelps, M, Puncken, O, Schreiber, E, Schulte, BW, Setyawati, Y, Steinke, M, Standke, M, Thies, F, Weinert, M, Wellmann, F, Weßels, P, Wimmer, MH, Winkler, W & Woehler, J 2019, 'Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO', Astrophysical Journal, Jg. 875, Nr. 2, 122. https://doi.org/10.48550/arXiv.1812.11656, https://doi.org/10.3847/1538-4357/ab113b, https://doi.org/10.3847/1538-4357/ac1f2c
The LIGO Scientific Collaboration, Virgo Collaboration, Bose, S., Brown, D. D., Chen, Y. B., Hanke, M., Hennig, J., Kumar, S., Lang, R. N., Lee, H. K., Lee, H. M., Lee, H. W., Lee, J., Li, X., Sanders, J. R., Schmidt, P., Sun, L., Wang, Y. F., Wu, D. S., ... Woehler, J. (2019). Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO. Astrophysical Journal, 875(2), Artikel 122. https://doi.org/10.48550/arXiv.1812.11656, https://doi.org/10.3847/1538-4357/ab113b, https://doi.org/10.3847/1538-4357/ac1f2c
The LIGO Scientific Collaboration, Virgo Collaboration, Bose S, Brown DD, Chen YB, Hanke M et al. Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO. Astrophysical Journal. 2019 Apr 23;875(2):122. doi: 10.48550/arXiv.1812.11656, 10.3847/1538-4357/ab113b, 10.3847/1538-4357/ac1f2c
The LIGO Scientific Collaboration ; Virgo Collaboration ; Bose, Sukanta et al. / Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO. in: Astrophysical Journal. 2019 ; Jahrgang 875, Nr. 2.
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title = "Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO",
abstract = "We describe directed searches for continuous gravitational waves (GWs) from 16 well-localized candidate neutron stars, assuming none of the stars has a binary companion. The searches were directed toward 15 supernova remnants and Fomalhaut b, a directly imaged extrasolar planet candidate that has been suggested to be a nearby old neutron star. Each search covered a broad band of frequencies and first and second time derivatives. After coherently integrating spans of data from the first Advanced LIGO observing run of 3.5-53.7 days per search, applying data-based vetoes, and discounting known instrumental artifacts, we found no astrophysical signals. We set upper limits on intrinsic GW strain as strict as 1 ×10 -25, fiducial neutron star ellipticity as strict as 2 ×10 -9, and fiducial r-mode amplitude as strict as 3 ×10 -8. ",
keywords = "gravitational waves, ISM: supernova remnants, stars: neutron",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and Abbott, {B. P.} and R. Abbott and Abbott, {T. D.} and S. Abraham and F. Acernese and K. Ackley and C. Adams and Adhikari, {R. X.} and Adya, {V. B.} and C. Affeldt and M. Agathos and K. Agatsuma and N. Aggarwal and Aguiar, {O. D.} and L. Aiello and A. Ain and P. Ajith and G. Allen and A. Allocca and Aloy, {M. A.} and Altin, {P. A.} and A. Amato and A. Ananyeva and Anderson, {S. B.} and Anderson, {W. G.} and Angelova, {S. V.} and S. Antier and S. Appert and K. Arai and Araya, {M. C.} and Areeda, {J. S.} and M. Ar{\`e}ne and N. Arnaud and Arun, {K. G.} and S. Ascenzi and G. Ashton and Aston, {S. M.} and P. Astone and F. Aubin and Danilishin, {S. L.} and K. Danzmann and M. Heurs and A. Hreibi and H. L{\"u}ck and D. Steinmeyer and H. Vahlbruch and L.-w. Wei and Wilken, {D. M.} and B. Willke and H. Wittel and Sukanta Bose and Brown, {D. D.} and Chen, {Y. B.} and Manuela Hanke and J. Hennig and Sanjeev Kumar and Lang, {R. N.} and Lee, {H. K.} and Lee, {H. M.} and Lee, {H. W.} and J. Lee and X. Li and Sanders, {J. R.} and Patricia Schmidt and L. Sun and Wang, {Y. F.} and Wu, {D. S.} and L. Zhang and Zhu, {X. J.} and Minchuan Zhou and Gerald Bergmann and Aparna Bisht and Nina Bode and P. Booker and Marc Brinkmann and M. Cabero and {de Varona}, O. and S. Hochheim and T. Dent and S. Doravari and J. Junker and Stefan Kaufer and Karvinen, {Kai S.} and S. Khan and R. Kirchhoff and Patrick Koch and N. Koper and K{\"o}hlenbeck, {S. M.} and Volker Kringel and G. Kuehn and S. Leavey and J. Lehmann and James Lough and Moritz Mehmet and J. Mukherjee and Arunava Mukherjee and Nikhil Mukund and M. Nery and F. Ohme and P. Oppermann and A. R{\"u}diger and M. Phelps and O. Puncken and Emil Schreiber and Schulte, {B. W.} and Y. Setyawati and M. Steinke and M. Standke and Fabian Thies and Michael Weinert and F. Wellmann and Peter We{\ss}els and Wimmer, {Maximilian H.} and W. Winkler and J. Woehler",
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month = apr,
day = "23",
doi = "10.48550/arXiv.1812.11656",
language = "English",
volume = "875",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
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Download

TY - JOUR

T1 - Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

AU - Abbott, T. D.

AU - Abraham, S.

AU - Acernese, F.

AU - Ackley, K.

AU - Adams, C.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Agathos, M.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Allen, G.

AU - Allocca, A.

AU - Aloy, M. A.

AU - Altin, P. A.

AU - Amato, A.

AU - Ananyeva, A.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Angelova, S. V.

AU - Antier, S.

AU - Appert, S.

AU - Arai, K.

AU - Araya, M. C.

AU - Areeda, J. S.

AU - Arène, M.

AU - Arnaud, N.

AU - Arun, K. G.

AU - Ascenzi, S.

AU - Ashton, G.

AU - Aston, S. M.

AU - Astone, P.

AU - Aubin, F.

AU - Danilishin, S. L.

AU - Danzmann, K.

AU - Heurs, M.

AU - Hreibi, A.

AU - Lück, H.

AU - Steinmeyer, D.

AU - Vahlbruch, H.

AU - Wei, L.-w.

AU - Wilken, D. M.

AU - Willke, B.

AU - Wittel, H.

AU - Bose, Sukanta

AU - Brown, D. D.

AU - Chen, Y. B.

AU - Hanke, Manuela

AU - Hennig, J.

AU - Kumar, Sanjeev

AU - Lang, R. N.

AU - Lee, H. K.

AU - Lee, H. M.

AU - Lee, H. W.

AU - Lee, J.

AU - Li, X.

AU - Sanders, J. R.

AU - Schmidt, Patricia

AU - Sun, L.

AU - Wang, Y. F.

AU - Wu, D. S.

AU - Zhang, L.

AU - Zhu, X. J.

AU - Zhou, Minchuan

AU - Bergmann, Gerald

AU - Bisht, Aparna

AU - Bode, Nina

AU - Booker, P.

AU - Brinkmann, Marc

AU - Cabero, M.

AU - de Varona, O.

AU - Hochheim, S.

AU - Dent, T.

AU - Doravari, S.

AU - Junker, J.

AU - Kaufer, Stefan

AU - Karvinen, Kai S.

AU - Khan, S.

AU - Kirchhoff, R.

AU - Koch, Patrick

AU - Koper, N.

AU - Köhlenbeck, S. M.

AU - Kringel, Volker

AU - Kuehn, G.

AU - Leavey, S.

AU - Lehmann, J.

AU - Lough, James

AU - Mehmet, Moritz

AU - Mukherjee, J.

AU - Mukherjee, Arunava

AU - Mukund, Nikhil

AU - Nery, M.

AU - Ohme, F.

AU - Oppermann, P.

AU - Rüdiger, A.

AU - Phelps, M.

AU - Puncken, O.

AU - Schreiber, Emil

AU - Schulte, B. W.

AU - Setyawati, Y.

AU - Steinke, M.

AU - Standke, M.

AU - Thies, Fabian

AU - Weinert, Michael

AU - Wellmann, F.

AU - Weßels, Peter

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

PY - 2019/4/23

Y1 - 2019/4/23

N2 - We describe directed searches for continuous gravitational waves (GWs) from 16 well-localized candidate neutron stars, assuming none of the stars has a binary companion. The searches were directed toward 15 supernova remnants and Fomalhaut b, a directly imaged extrasolar planet candidate that has been suggested to be a nearby old neutron star. Each search covered a broad band of frequencies and first and second time derivatives. After coherently integrating spans of data from the first Advanced LIGO observing run of 3.5-53.7 days per search, applying data-based vetoes, and discounting known instrumental artifacts, we found no astrophysical signals. We set upper limits on intrinsic GW strain as strict as 1 ×10 -25, fiducial neutron star ellipticity as strict as 2 ×10 -9, and fiducial r-mode amplitude as strict as 3 ×10 -8.

AB - We describe directed searches for continuous gravitational waves (GWs) from 16 well-localized candidate neutron stars, assuming none of the stars has a binary companion. The searches were directed toward 15 supernova remnants and Fomalhaut b, a directly imaged extrasolar planet candidate that has been suggested to be a nearby old neutron star. Each search covered a broad band of frequencies and first and second time derivatives. After coherently integrating spans of data from the first Advanced LIGO observing run of 3.5-53.7 days per search, applying data-based vetoes, and discounting known instrumental artifacts, we found no astrophysical signals. We set upper limits on intrinsic GW strain as strict as 1 ×10 -25, fiducial neutron star ellipticity as strict as 2 ×10 -9, and fiducial r-mode amplitude as strict as 3 ×10 -8.

KW - gravitational waves

KW - ISM: supernova remnants

KW - stars: neutron

UR - http://www.scopus.com/inward/record.url?scp=85067178226&partnerID=8YFLogxK

U2 - 10.48550/arXiv.1812.11656

DO - 10.48550/arXiv.1812.11656

M3 - Article

VL - 875

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 122

ER -

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