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  New searches for continuous gravitational waves from seven fast pulsars

Ashok, A., Beheshtipour, B., Papa, M. A., Freire, P. C. C., Steltner, B., Machenschalk, B., et al. (2021). New searches for continuous gravitational waves from seven fast pulsars. The Astrophysical Journal, 923(1): 85. doi:10.3847/1538-4357/ac2582.

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 Creators:
Ashok, Anjana1, Author           
Beheshtipour, Banafsheh1, Author           
Papa, Maria Alessandra1, Author           
Freire , Paulo C. C., Author
Steltner, Benjamin1, Author           
Machenschalk, Bernd1, Author           
Behnke, Oliver2, Author           
Allen, Bruce2, Author           
Prix, Reinhard1, Author           
Affiliations:
1Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_2630691              
2Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,General Relativity and Quantum Cosmology, gr-qc
 Abstract: We conduct searches for continuous gravitational waves from seven pulsars,
that have not been targeted in continuous wave searches of Advanced LIGO data
before. We target emission at exactly twice the rotation frequency of the
pulsars and in a small band around such frequency. The former search assumes
that the gravitational wave quadrupole is changing phase-locked with the
rotation of the pulsar. The search over a range of frequencies allows for
differential rotation between the component emitting the radio signal and the
component emitting the gravitational waves, for example the crust or
magnetosphere versus the core. Timing solutions derived from the Arecibo
327-MHz Drift-Scan Pulsar Survey (AO327) observations are used. No evidence of
a signal is found and upper limits are set on the gravitational wave amplitude.
For one of the pulsars we probe gravitational wave intrinsic amplitudes just a
factor of 3.8 higher than the spin-down limit, assuming a canonical moment of
inertia of $10^{38}$ kg m$^2$. Our tightest ellipticity is $1.7 \times
10^{-8}$, which is a value well within the range of what a neutron star crust
could support.

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 Dates: 2021-07-202021-07-282021
 Publication Status: Issued
 Pages: Submitted to The Astrophysical Journal
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 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 2107.09727
DOI: 10.3847/1538-4357/ac2582
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Title: The Astrophysical Journal
Source Genre: Journal
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Pages: - Volume / Issue: 923 (1) Sequence Number: 85 Start / End Page: - Identifier: -