dc.identifier.uri |
http://dx.doi.org/10.15488/11117 |
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dc.identifier.uri |
https://www.repo.uni-hannover.de/handle/123456789/11200 |
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dc.contributor.author |
Adya, V.B.
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dc.contributor.author |
Affeldt, Christoph
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dc.contributor.author |
Allen, Bruce
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dc.contributor.author |
Ashton, G.
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dc.contributor.author |
Aulbert, C.
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dc.contributor.author |
Baune, C.
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dc.contributor.author |
Beer, C.
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dc.contributor.author |
Bergmann, G.
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dc.contributor.author |
Birnholtz, O.
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dc.contributor.author |
Bock, O.
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dc.contributor.author |
Bode, N.
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dc.contributor.author |
Brinkmann, M.
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dc.contributor.author |
Cabero, M.
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dc.contributor.author |
Capano, C.D.
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dc.contributor.author |
Danilishin, S.L.
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dc.contributor.author |
Danzmann, K.
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dc.contributor.author |
Denker, T.
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dc.contributor.author |
Dent, T.
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dc.contributor.author |
Doravari, S.
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dc.contributor.author |
Drago, M.
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dc.contributor.author |
Eggenstein, H.-B.
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dc.contributor.author |
Fehrmann, H.
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dc.contributor.author |
Gabbard, H.
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dc.contributor.author |
Goetz, E.
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dc.contributor.author |
Grote, H.
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dc.contributor.author |
Hanke, M.M.
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dc.contributor.author |
Heurs, M.
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dc.contributor.author |
Hu, Y.M.
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dc.contributor.author |
Indik, N.
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dc.contributor.author |
Junker, J.
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dc.contributor.author |
Karvinen, K.S.
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dc.contributor.author |
Khan, S.
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dc.contributor.author |
Kirchhoff, R.
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dc.contributor.author |
Koch, P.
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dc.contributor.author |
et al.
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dc.contributor.author |
LIGO Scientific Collaboration
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dc.contributor.author |
Virgo Collaboration
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dc.date.accessioned |
2021-07-07T06:57:34Z |
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dc.date.available |
2021-07-07T06:57:34Z |
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dc.date.issued |
2017 |
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dc.identifier.citation |
Adya, V.B.; Affeldt, C.; Allen, B.; Ashton, G.; Aulbert, C. et al.: Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-based Cross-correlation Search in Advanced LIGO Data. In: The astrophysical journal : an international review of spectroscopy and astronomical physics 847 (2017), Nr. 1, 47. DOI: https://doi.org/10.3847/1538-4357/aa86f0 |
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dc.description.abstract |
We present the results of a semicoherent search for continuous gravitational waves from the low-mass X-ray binary Scorpius X-1, using data from the first Advanced LIGO observing run. The search method uses details of the modeled, parametrized continuous signal to combine coherently data separated by less than a specified coherence time, which can be adjusted to trade off sensitivity against computational cost. A search was conducted over the frequency range 25–2000 Hz, spanning the current observationally constrained range of binary orbital parameters. No significant detection candidates were found, and frequency-dependent upper limits were set using a combination of sensitivity estimates and simulated signal injections. The most stringent upper limit was set at 125 Hz , with comparable limits set across the most sensitive frequency range from 100 to 200 Hz. At this frequency, the 95% upper limit on the signal amplitude h0 is2,3 x 10 {hoch} -25 marginalized over the unknown inclination angle of the neutron star's spin, and 8.0 x 10 {hoch} -26 assuming the best orientation (which results in circularly polarized gravitational waves). These limits are a factor of 3–4 stronger than those set by other analyses of the same data, and a factor of ~7 stronger than the best upper limits set using data from Initial LIGO science runs. In the vicinity of 100 Hz, the limits are a factor of between 1.2 and 3.5 above the predictions of the torque balance model, depending on the inclination angle; if the most likely inclination angle of 44° is assumed, they are within a factor of 1.7. |
eng |
dc.language.iso |
eng |
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dc.publisher |
London : Institute of Physics Publ. |
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dc.relation.ispartofseries |
The astrophysical journal : an international review of spectroscopy and astronomical physics 847 (2017), Nr. 1 |
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dc.rights |
CC BY 3.0 Unported |
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dc.rights.uri |
https://creativecommons.org/licenses/by/3.0/ |
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dc.subject |
gravitational waves |
eng |
dc.subject |
Advanced LIGO observing run |
eng |
dc.subject |
low-mass X-ray binary Scorpius X-1 |
eng |
dc.subject.ddc |
520 | Astronomie, Kartographie
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ger |
dc.title |
Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-based Cross-correlation Search in Advanced LIGO Data |
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dc.type |
Article |
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dc.type |
Text |
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dc.relation.essn |
1538-4357 |
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dc.relation.issn |
0004-637X |
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dc.relation.doi |
https://doi.org/10.3847/1538-4357/aa86f0 |
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dc.bibliographicCitation.issue |
1 |
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dc.bibliographicCitation.volume |
847 |
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dc.bibliographicCitation.firstPage |
47 |
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dc.description.version |
publishedVersion |
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tib.accessRights |
frei zug�nglich |
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