Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run

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
  • R. 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
  • R. Kirchhoff
  • Patrick Koch
  • N. Koper
  • S. M. Köhlenbeck
  • Volker Kringel
  • Kai S. Karvinen
  • S. Khan
  • S. Leavey
  • J. Lehmann
  • James Lough
  • Moritz Mehmet
  • Arunava Mukherjee
  • Nikhil Mukund
  • M. Nery
  • F. Ohme
  • P. Oppermann
  • A. Rüdiger
  • M. Phelps
  • O. Puncken
  • Emil Schreiber
  • B. W. Schulte
  • Y. Setyawati
  • M. Standke
  • Fabian Thies
  • M. Steinke
  • Michael Weinert
  • F. Wellmann
  • Peter Weßels
  • Maximilian H. Wimmer
  • W. Winkler
  • J. Woehler

Organisationseinheiten

Externe Organisationen

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Washington State University Pullman
  • 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
  • Fudan University
  • Monash University
  • Northwestern University
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer163
Seitenumfang14
FachzeitschriftAstrophysical Journal
Jahrgang874
Ausgabenummer2
PublikationsstatusVeröffentlicht - 4 Apr. 2019

Abstract

We present the results of a search for short- and intermediate-duration gravitational-wave signals from four magnetar bursts in Advanced LIGO's second observing run. We find no evidence of a signal and set upper bounds on the root sum squared of the total dimensionless strain (h rss ) from incoming intermediate-duration gravitational waves ranging from 1.1 ×10 -22 at 150 Hz to 4.4 ×10 -22 at 1550 Hz at 50% detection efficiency. From the known distance to the magnetar SGR 1806-20 (8.7 kpc), we can place upper bounds on the isotropic gravitational-wave energy of 3.4 ×10 44 erg at 150 Hz assuming optimal orientation. This represents an improvement of about a factor of 10 in strain sensitivity from the previous search for such signals, conducted during initial LIGO's sixth science run. The short-duration search yielded upper limits of 2.1 ×10 44 erg for short white noise bursts, and 2.3 ×10 47 erg for 100 ms long ringdowns at 1500 Hz, both at 50% detection efficiency.

ASJC Scopus Sachgebiete

Zitieren

Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run. / The LIGO Scientific Collaboration; Virgo Collaboration; Bose, Sukanta et al.
in: Astrophysical Journal, Jahrgang 874, Nr. 2, 163, 04.04.2019.

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, R, 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, Kirchhoff, R, Koch, P, Koper, N, Köhlenbeck, SM, Kringel, V, Karvinen, KS, Khan, S, Leavey, S, Lehmann, J, Lough, J, Mehmet, M, Mukherjee, A, Mukund, N, Nery, M, Ohme, F, Oppermann, P, Rüdiger, A, Phelps, M, Puncken, O, Schreiber, E, Schulte, BW, Setyawati, Y, Standke, M, Thies, F, Steinke, M, Weinert, M, Wellmann, F, Weßels, P, Wimmer, MH, Winkler, W & Woehler, J 2019, 'Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run', Astrophysical Journal, Jg. 874, Nr. 2, 163. https://doi.org/10.3847/1538-4357/ab0e15
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). Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run. Astrophysical Journal, 874(2), Artikel 163. https://doi.org/10.3847/1538-4357/ab0e15
The LIGO Scientific Collaboration, Virgo Collaboration, Bose S, Brown DD, Chen YB, Hanke M et al. Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run. Astrophysical Journal. 2019 Apr 4;874(2):163. doi: 10.3847/1538-4357/ab0e15
The LIGO Scientific Collaboration ; Virgo Collaboration ; Bose, Sukanta et al. / Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run. in: Astrophysical Journal. 2019 ; Jahrgang 874, Nr. 2.
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title = "Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO{\textquoteright}s Second Observing Run",
abstract = "We present the results of a search for short- and intermediate-duration gravitational-wave signals from four magnetar bursts in Advanced LIGO's second observing run. We find no evidence of a signal and set upper bounds on the root sum squared of the total dimensionless strain (h rss ) from incoming intermediate-duration gravitational waves ranging from 1.1 ×10 -22 at 150 Hz to 4.4 ×10 -22 at 1550 Hz at 50% detection efficiency. From the known distance to the magnetar SGR 1806-20 (8.7 kpc), we can place upper bounds on the isotropic gravitational-wave energy of 3.4 ×10 44 erg at 150 Hz assuming optimal orientation. This represents an improvement of about a factor of 10 in strain sensitivity from the previous search for such signals, conducted during initial LIGO's sixth science run. The short-duration search yielded upper limits of 2.1 ×10 44 erg for short white noise bursts, and 2.3 ×10 47 erg for 100 ms long ringdowns at 1500 Hz, both at 50% detection efficiency. ",
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language = "English",
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Download

TY - JOUR

T1 - Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run

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 - Ascenzi, S.

AU - Ashton, G.

AU - Aston, S. M.

AU - Astone, P.

AU - Aubin, F.

AU - Aufmuth, P.

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, R.

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 - Kirchhoff, R.

AU - Koch, Patrick

AU - Koper, N.

AU - Köhlenbeck, S. M.

AU - Kringel, Volker

AU - Karvinen, Kai S.

AU - Khan, S.

AU - Leavey, S.

AU - Lehmann, J.

AU - Lough, James

AU - Mehmet, Moritz

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 - Standke, M.

AU - Thies, Fabian

AU - Steinke, M.

AU - Weinert, Michael

AU - Wellmann, F.

AU - Weßels, Peter

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

PY - 2019/4/4

Y1 - 2019/4/4

N2 - We present the results of a search for short- and intermediate-duration gravitational-wave signals from four magnetar bursts in Advanced LIGO's second observing run. We find no evidence of a signal and set upper bounds on the root sum squared of the total dimensionless strain (h rss ) from incoming intermediate-duration gravitational waves ranging from 1.1 ×10 -22 at 150 Hz to 4.4 ×10 -22 at 1550 Hz at 50% detection efficiency. From the known distance to the magnetar SGR 1806-20 (8.7 kpc), we can place upper bounds on the isotropic gravitational-wave energy of 3.4 ×10 44 erg at 150 Hz assuming optimal orientation. This represents an improvement of about a factor of 10 in strain sensitivity from the previous search for such signals, conducted during initial LIGO's sixth science run. The short-duration search yielded upper limits of 2.1 ×10 44 erg for short white noise bursts, and 2.3 ×10 47 erg for 100 ms long ringdowns at 1500 Hz, both at 50% detection efficiency.

AB - We present the results of a search for short- and intermediate-duration gravitational-wave signals from four magnetar bursts in Advanced LIGO's second observing run. We find no evidence of a signal and set upper bounds on the root sum squared of the total dimensionless strain (h rss ) from incoming intermediate-duration gravitational waves ranging from 1.1 ×10 -22 at 150 Hz to 4.4 ×10 -22 at 1550 Hz at 50% detection efficiency. From the known distance to the magnetar SGR 1806-20 (8.7 kpc), we can place upper bounds on the isotropic gravitational-wave energy of 3.4 ×10 44 erg at 150 Hz assuming optimal orientation. This represents an improvement of about a factor of 10 in strain sensitivity from the previous search for such signals, conducted during initial LIGO's sixth science run. The short-duration search yielded upper limits of 2.1 ×10 44 erg for short white noise bursts, and 2.3 ×10 47 erg for 100 ms long ringdowns at 1500 Hz, both at 50% detection efficiency.

KW - gravitational waves

KW - stars: magnetars

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U2 - 10.3847/1538-4357/ab0e15

DO - 10.3847/1538-4357/ab0e15

M3 - Article

VL - 874

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 163

ER -

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