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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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Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. / ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration.

In: The Astrophysical Journal, Vol. 870, 134, 16.01.2019.

Research output: Contribution to journalJournal article

Harvard

ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration 2019, 'Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube', The Astrophysical Journal, vol. 870, 134. https://doi.org/10.3847/1538-4357/aaf21d

APA

ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration (2019). Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. The Astrophysical Journal, 870, [134]. https://doi.org/10.3847/1538-4357/aaf21d

Vancouver

ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration. Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. The Astrophysical Journal. 2019 Jan 16;870. 134. https://doi.org/10.3847/1538-4357/aaf21d

Author

ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration. / Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube. In: The Astrophysical Journal. 2019 ; Vol. 870.

Bibtex

@article{d4dd5a9d0f434e1ea4181e517473d81e,
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.",
keywords = "gravitational waves, neutrinos",
author = "{ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration} and M. Pitkin",
year = "2019",
month = jan,
day = "16",
doi = "10.3847/1538-4357/aaf21d",
language = "English",
volume = "870",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",

}

RIS

TY - JOUR

T1 - Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

AU - ANTARES Collaboration, IceCube Collaboration, The LIGO Scientific Collaboration and the Virgo Collaboration

AU - Pitkin, M.

PY - 2019/1/16

Y1 - 2019/1/16

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.

KW - gravitational waves

KW - neutrinos

U2 - 10.3847/1538-4357/aaf21d

DO - 10.3847/1538-4357/aaf21d

M3 - Journal article

VL - 870

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

M1 - 134

ER -