Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Antares, and Icecube; Markus Tobias Ahlers; Etienne Bourbeau; D. Jason Koskinen; Michael James Larson; Morten Ankersen Medici; Subir Sarkar; Thomas Simon Stuttard; M Rameez

doi:10.3847/1538-4357/aaf21d

Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

Antares, and Icecube, Markus Tobias Ahlers, Etienne Bourbeau, D. Jason Koskinen, Michael James Larson, Morten Ankersen Medici, Subir Sarkar, Thomas Simon Stuttard, M Rameez

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Abstract

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

Original language	English
Article number	134
Journal	Astrophysical Journal
Volume	870
Issue number	2
Number of pages	16
ISSN	0004-637X
DOIs	https://doi.org/10.3847/1538-4357/aaf21d
Publication status	Published - 10 Jan 2019

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Antares, and Icecube, Ahlers, M. T., Bourbeau, E., Koskinen, D. J., Larson, M. J., Medici, M. A., Sarkar, S., Stuttard, T. S., & Rameez, M. (2019). Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. Astrophysical Journal, 870(2), Article 134. https://doi.org/10.3847/1538-4357/aaf21d

Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. / Antares, and Icecube ; Ahlers, Markus Tobias; Bourbeau, Etienne et al.
In: Astrophysical Journal, Vol. 870, No. 2, 134, 10.01.2019.

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

Antares, and Icecube, Ahlers, MT, Bourbeau, E, Koskinen, DJ, Larson, MJ, Medici, MA, Sarkar, S, Stuttard, TS & Rameez, M 2019, 'Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube', Astrophysical Journal, vol. 870, no. 2, 134. https://doi.org/10.3847/1538-4357/aaf21d

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title = "Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube",

abstract = "Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.",

author = "Andreas Albert and M. Andr{\'e} and M. Ardid and J.J. Aubert and J. Aublin and T. Avgitas and B. Baret and J. Barrios-Marti and S. Basa and B. Belhorma and V. Bertin and S. Biagi and R. Bormuth and J. Boumaaza and S. Bourret and Marna Bouwhuis and H. Br{\^a}nza{\c s} and R. Bruijn and Jurgen Brunner and Busto, {Jes{\'u}s H.} and A. Capone and L. Caramete and J. Carr and S. Celli and M. Chabab and {Cherkaoui El Moursli}, R. and T. Chiarusi and {Antares, and Icecube} and Ahlers, {Markus Tobias} and Etienne Bourbeau and Koskinen, {D. Jason} and Larson, {Michael James} and Medici, {Morten Ankersen} and Subir Sarkar and Stuttard, {Thomas Simon} and M Rameez",

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AU - Aubert, J.J.

AU - Aublin, J.

AU - Avgitas, T.

AU - Baret, B.

AU - Barrios-Marti, J.

AU - Basa, S.

AU - Belhorma, B.

AU - Bertin, V.

AU - Biagi, S.

AU - Bormuth, R.

AU - Boumaaza, J.

AU - Bourret, S.

AU - Bouwhuis, Marna

AU - Brânzaş, H.

AU - Bruijn, R.

AU - Brunner, Jurgen

AU - Busto, Jesús H.

AU - Capone, A.

AU - Caramete, L.

AU - Carr, J.

AU - Celli, S.

AU - Chabab, M.

AU - Cherkaoui El Moursli, R.

AU - Chiarusi, T.

AU - Antares, and Icecube

AU - Ahlers, Markus Tobias

AU - Bourbeau, Etienne

AU - Koskinen, D. Jason

AU - Larson, Michael James

AU - Medici, Morten Ankersen

AU - Sarkar, Subir

AU - Stuttard, Thomas Simon

AU - Rameez, M

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N2 - Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

AB - Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

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DO - 10.3847/1538-4357/aaf21d

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VL - 870

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JF - Astrophysical Journal

IS - 2

M1 - 134

ER -

Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

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