> Details
Abbott, Benjamin P.
[Author];
Abbott, Rich
[Author];
Abbott, Thomas D.
[Author];
Acernese, Fausto
[Author];
Ackley, Kendall
[Author];
Adams, Carl
[Author];
Adams, Thomas
[Author];
Addesso, Paolo
[Author];
Adhikari, Rana X.
[Author];
Adya, Vaishali B.
[Author];
Affeldt, Christoph
[Author];
Afrough, Mohammad
[Author];
Agarwal, Bhanu
[Author];
Agathos, Michalis
[Author];
Agatsuma, Kazuhiro
[Author];
Aggarwal, Nancy
[Author];
Aguiar, Odylio D.
[Author];
Aiello, Lorenzo
[Author];
Ain, Anirban
[Author];
Allen, Bruce
[Author];
Allen, Gabrielle
[Author];
Allocca, Annalisa
[Author];
Altin, Paul A.
[Author];
Amato, Alex
[Author];
[...]
Full band all-sky search for periodic gravitational waves in the O1 LIGO data
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- Media type: E-Article; Text
- Title: Full band all-sky search for periodic gravitational waves in the O1 LIGO data
- Contributor: Abbott, Benjamin P. [Author]; Abbott, Rich [Author]; Abbott, Thomas D. [Author]; Acernese, Fausto [Author]; Ackley, Kendall [Author]; Adams, Carl [Author]; Adams, Thomas [Author]; Addesso, Paolo [Author]; Adhikari, Rana X. [Author]; Adya, Vaishali B. [Author]; Affeldt, Christoph [Author]; Afrough, Mohammad [Author]; Agarwal, Bhanu [Author]; Agathos, Michalis [Author]; Agatsuma, Kazuhiro [Author]; Aggarwal, Nancy [Author]; Aguiar, Odylio D. [Author]; Aiello, Lorenzo [Author]; Ain, Anirban [Author]; Allen, Bruce [Author]; Allen, Gabrielle [Author]; Allocca, Annalisa [Author]; Altin, Paul A. [Author]; Amato, Alex [Author]; [...]
- imprint: College Park, MD : American Physical Society, 2018
- Published in: Physical Review D 97 (2018), Nr. 10 ; Physical Review D
- Issue: published Version
- Language: English
- DOI: https://doi.org/10.15488/12001; https://doi.org/10.1103/PhysRevD.97.102003
- ISSN: 2470-0010
- Keywords: gravitational radiation detector ; gravitational radiation ; frequency: time dependence ; frequency: low ; LIGO ; gravitational radiation: emission ; neutron star ; galaxy
- Origination:
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Footnote:
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- Description: We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of [-1.0,+0.1]×10-8 Hz/s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run O1. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h0 is ∼4×10-25 near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3×10-24. For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is ∼1.5×10-25. © 2018 American Physical Society.
- Access State: Open Access