GLORIA — GEOMAR Library Ocean Research Information Access

1

Online Resource

Multi-messenger Observations of a Binary Neutron Star Merger

Abbott, B. P. ; Abbott, R. ; Abbott, T. D. ; [et al.]

American Astronomical Society ; 2017

In: The Astrophysical Journal Vol. 848, No. 2 ( 2017-10-16), p. L12-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 848, No. 2 ( 2017-10-16), p. L12-

Type of Medium: Online Resource

ISSN: 2041-8213

URL: Article

DOI: 10.3847/2041-8213/aa91c9

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2017

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 2006858-X

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2

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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Albert, A. ; André, M. ; Anghinolfi, M. ; [et al.]

American Astronomical Society ; 2017

In: The Astrophysical Journal Vol. 850, No. 2 ( 2017-11-30), p. L35-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 850, No. 2 ( 2017-11-30), p. L35-

Type of Medium: Online Resource

ISSN: 2041-8213

URL: Article

DOI: 10.3847/2041-8213/aa9aed

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2017

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 2006858-X

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3

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Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

Abbott, R. ; Abe, H. ; Acernese, F. ; [et al.]

American Astronomical Society ; 2023

In: The Astrophysical Journal Supplement Series Vol. 267, No. 2 ( 2023-08-01), p. 29-

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In: The Astrophysical Journal Supplement Series, American Astronomical Society, Vol. 267, No. 2 ( 2023-08-01), p. 29-

Abstract: The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org . The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.

Type of Medium: Online Resource

ISSN: 0067-0049 , 1538-4365

URL: Article

DOI: 10.3847/1538-4365/acdc9f

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2023

detail.hit.zdb_id: 2006860-8

detail.hit.zdb_id: 2207650-5

SSG: 16,12

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4

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Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

Albert, A. ; André, M. ; Anghinolfi, M. ; [et al.]

American Physical Society (APS) ; 2017

In: Physical Review D Vol. 96, No. 2 ( 2017-7-12)

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In: Physical Review D, American Physical Society (APS), Vol. 96, No. 2 ( 2017-7-12)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.96.022005

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2017

detail.hit.zdb_id: 2844732-3

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5

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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

Albert, A. ; André, M. ; Anghinolfi, M. ; [et al.]

American Astronomical Society ; 2019

In: The Astrophysical Journal Vol. 870, No. 2 ( 2019-01-16), p. 134-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 870, No. 2 ( 2019-01-16), p. 134-

Type of Medium: Online Resource

ISSN: 1538-4357

URL: Article

DOI: 10.3847/1538-4357/aaf21d

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2019

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 1473835-1

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6

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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Abbott, R. ; Abbott, T. D. ; Abraham, S. ; [et al.]

American Astronomical Society ; 2021

In: The Astrophysical Journal Letters Vol. 915, No. 1 ( 2021-07-01), p. L5-

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In: The Astrophysical Journal Letters, American Astronomical Society, Vol. 915, No. 1 ( 2021-07-01), p. L5-

Abstract: We report the observation of gravitational waves from two compact binary coalescences in LIGO’s and Virgo’s third observing run with properties consistent with neutron star–black hole (NSBH) binaries. The two events are named GW200105_162426 and GW200115_042309, abbreviated as GW200105 and GW200115; the first was observed by LIGO Livingston and Virgo and the second by all three LIGO–Virgo detectors. The source of GW200105 has component masses 8 . 9 − 1 . 5 + 1. 2 and 1. 9 − 0. 2 + 0. 3 M ⊙ , whereas the source of GW200115 has component masses 5. 7 − 2 . 1 + 1. 8 and 1. 5 − 0. 3 + 0. 7 M ⊙ (all measurements quoted at the 90% credible level). The probability that the secondary’s mass is below the maximal mass of a neutron star is 89%–96% and 87%–98%, respectively, for GW200105 and GW200115, with the ranges arising from different astrophysical assumptions. The source luminosity distances are 280 − 110 + 110 and 300 − 100 + 150 Mpc , respectively. The magnitude of the primary spin of GW200105 is less than 0.23 at the 90% credible level, and its orientation is unconstrained. For GW200115, the primary spin has a negative spin projection onto the orbital angular momentum at 88% probability. We are unable to constrain the spin or tidal deformation of the secondary component for either event. We infer an NSBH merger rate density of 45 − 33 + 75 Gpc − 3 yr − 1 when assuming that GW200105 and GW200115 are representative of the NSBH population or 130 − 69 + 112 Gpc − 3 yr − 1 under the assumption of a broader distribution of component masses.

Type of Medium: Online Resource

ISSN: 2041-8205 , 2041-8213

URL: Article

DOI: 10.3847/2041-8213/ac082e

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2021

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 2006858-X

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7

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All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data

Abbott, R. ; Abbott, T. D. ; Abraham, S. ; [et al.]

American Physical Society (APS) ; 2021

In: Physical Review D Vol. 104, No. 8 ( 2021-10-8)

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In: Physical Review D, American Physical Society (APS), Vol. 104, No. 8 ( 2021-10-8)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.104.082004

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2021

detail.hit.zdb_id: 2844732-3

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8

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Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3

Abbott, R. ; Abbott, T. D. ; Acernese, F. ; [et al.]

American Physical Society (APS) ; 2023

In: Physical Review X Vol. 13, No. 1 ( 2023-3-29)

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In: Physical Review X, American Physical Society (APS), Vol. 13, No. 1 ( 2023-3-29)

Type of Medium: Online Resource

ISSN: 2160-3308

URL: Article

DOI: 10.1103/PhysRevX.13.011048

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2023

detail.hit.zdb_id: 2622565-7

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9

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Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO–Virgo Observing Run O3a

Abbott, R. ; Abbott, T. D. ; Acernese, F. ; [et al.]

American Astronomical Society ; 2023

In: The Astrophysical Journal Vol. 955, No. 2 ( 2023-10-01), p. 155-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 955, No. 2 ( 2023-10-01), p. 155-

Abstract: We search for gravitational-wave (GW) transients associated with fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst Project, during the first part of the third observing run of Advanced LIGO and Advanced Virgo (2019 April 1 15:00 UTC–2019 October 1 15:00 UTC). Triggers from 22 FRBs were analyzed with a search that targets both binary neutron star (BNS) and neutron star–black hole (NSBH) mergers. A targeted search for generic GW transients was conducted on 40 FRBs. We find no significant evidence for a GW association in either search. Given the large uncertainties in the distances of our FRB sample, we are unable to exclude the possibility of a GW association. Assessing the volumetric event rates of both FRB and binary mergers, an association is limited to 15% of the FRB population for BNS mergers or 1% for NSBH mergers. We report 90% confidence lower bounds on the distance to each FRB for a range of GW progenitor models and set upper limits on the energy emitted through GWs for a range of emission scenarios. We find values of order 10 51 –10 57 erg for models with central GW frequencies in the range 70–3560 Hz. At the sensitivity of this search, we find these limits to be above the predicted GW emissions for the models considered. We also find no significant coincident detection of GWs with the repeater, FRB 20200120E, which is the closest known extragalactic FRB.

Type of Medium: Online Resource

ISSN: 0004-637X , 1538-4357

URL: Article

DOI: 10.3847/1538-4357/acd770

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2023

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 1473835-1

SSG: 16,12

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10

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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

Abbott, R. ; Abe, H. ; Acernese, F. ; [et al.]

American Physical Society (APS) ; 2022

In: Physical Review D Vol. 106, No. 10 ( 2022-11-28)

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In: Physical Review D, American Physical Society (APS), Vol. 106, No. 10 ( 2022-11-28)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.106.102008

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2022

detail.hit.zdb_id: 2844732-3

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