dc.identifier.uri |
http://dx.doi.org/10.15488/1734 |
|
dc.identifier.uri |
http://www.repo.uni-hannover.de/handle/123456789/1759 |
|
dc.contributor.author |
Abbott, B.P.
|
|
dc.contributor.author |
Allen, Bruce
|
|
dc.contributor.author |
Aufmuth, Peter
|
|
dc.contributor.author |
Danzmann, Karsten
|
|
dc.contributor.author |
Vahlbruch, H.
|
|
dc.contributor.author |
et al.
|
|
dc.contributor.author |
IPN Collaboration
|
|
dc.date.accessioned |
2017-07-17T11:09:07Z |
|
dc.date.available |
2017-07-17T11:09:07Z |
|
dc.date.issued |
2017 |
|
dc.identifier.citation |
Abbott, B.P.; Allen, B.; Aufmuth, P.; Danzmann, K.; Vahlbruch, H.; et al. (The IPN Collaboration): Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B. In: Astrophysical Journal 841 (2017), Nr. 2, 89. DOI: https://doi.org/10.3847/1538-4357/aa6c47 |
|
dc.description.abstract |
We present the results of the search for gravitational waves (GWs) associated with γ-ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). We find no evidence of a GW signal for any of the 41 γ-ray bursts for which LIGO data are available with sufficient duration. For all γ-ray bursts, we place lower bounds on the distance to the source using the optimistic assumption that GWs with an energy of were emitted within the – Hz band, and we find a median 90% confidence limit of 71 Mpc at 150 Hz. For the subset of 19 short/hard γ-ray bursts, we place lower bounds on distance with a median 90% confidence limit of 90 Mpc for binary neutron star (BNS) coalescences, and 150 and 139 Mpc for neutron star–black hole coalescences with spins aligned to the orbital angular momentum and in a generic configuration, respectively. These are the highest distance limits ever achieved by GW searches. We also discuss in detail the results of the search for GWs associated with GRB 150906B, an event that was localized by the InterPlanetary Network near the local galaxy NGC 3313, which is at a luminosity distance of Mpc (z = 0.0124). Assuming the γ-ray emission is beamed with a jet half-opening angle , we exclude a BNS and a neutron star–black hole in NGC 3313 as the progenitor of this event with confidence >99%. Further, we exclude such progenitors up to a distance of 102 Mpc and 170 Mpc, respectively. |
eng |
dc.description.sponsorship |
United States National Science Foundation (NSF) |
|
dc.description.sponsorship |
Science and Technology Facilities Council (STFC) of the United Kingdom |
|
dc.description.sponsorship |
Max-Planck-Society (MPS) |
|
dc.description.sponsorship |
State of Niedersachsen |
|
dc.description.sponsorship |
Australian Research Council |
|
dc.description.sponsorship |
Italian Istituto Nazionale di Fisica Nucleare (INFN) |
|
dc.description.sponsorship |
French Centre National de la Recherche Scientifique (CNRS) |
|
dc.description.sponsorship |
Netherlands Organisation for Scientific Research |
|
dc.description.sponsorship |
Council of Scientific and Industrial Research of India |
|
dc.description.sponsorship |
Science & Engineering Research Board (SERB), India |
|
dc.description.sponsorship |
Ministry of Human Resource Development, India |
|
dc.description.sponsorship |
Spanish Ministerio de Economía y Competitividad |
|
dc.description.sponsorship |
Conselleria d’Economia i Competitivitat |
|
dc.description.sponsorship |
Conselleria d’Educació Cultura i Universitats of the Govern de les Illes Balears |
|
dc.description.sponsorship |
National Science Centre of Poland |
|
dc.description.sponsorship |
European Commission |
|
dc.description.sponsorship |
Royal Society |
|
dc.description.sponsorship |
Scottish Funding Council |
|
dc.description.sponsorship |
Scottish Universities Physics Alliance |
|
dc.description.sponsorship |
Hungarian Scientific Research Fund (OTKA) |
|
dc.description.sponsorship |
Lyon Institute of Origins (LIO) |
|
dc.description.sponsorship |
National Research Foundation of Korea |
|
dc.description.sponsorship |
Industry Canada |
|
dc.description.sponsorship |
Province of Ontario |
|
dc.description.sponsorship |
Brazilian Ministry of Science |
|
dc.description.sponsorship |
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) |
|
dc.description.sponsorship |
Russian Foundation for Basic Research |
|
dc.description.sponsorship |
Leverhulme Trust |
|
dc.description.sponsorship |
Ministry of Science and Technology (MOST) |
|
dc.description.sponsorship |
Kavli Foundation |
|
dc.description.sponsorship |
NASA/NNX15AU74G |
|
dc.description.sponsorship |
RFBR/15-02-00532-i |
|
dc.description.sponsorship |
RFBR/16-29-13009-ofi-m |
|
dc.language.iso |
eng |
|
dc.publisher |
Bristol : IOP Publishing Ltd. |
|
dc.relation.ispartofseries |
Astrophysical Journal 841 (2017), Nr. 2 |
|
dc.rights |
CC BY 3.0 Unported |
|
dc.rights.uri |
https://creativecommons.org/licenses/by/3.0/ |
|
dc.subject |
binaries: close |
eng |
dc.subject |
gamma-ray burst: general |
eng |
dc.subject |
gravitational waves |
eng |
dc.subject |
Gravitationswelle |
ger |
dc.subject.ddc |
520 | Astronomie, Kartographie
|
ger |
dc.title |
Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B |
eng |
dc.type |
Article |
|
dc.type |
Text |
|
dc.relation.essn |
1538-4357 |
|
dc.relation.doi |
https://doi.org/10.3847/1538-4357/aa6c47 |
|
dc.bibliographicCitation.issue |
2 |
|
dc.bibliographicCitation.volume |
841 |
|
dc.bibliographicCitation.firstPage |
89 |
|
dc.description.version |
publishedVersion |
|
tib.accessRights |
frei zug�nglich |
|