Directed search for gravitational waves from Scorpius X-1 with initial LIGO data

We present results of a search for continuously emitted gravitational radiation, directed at the brightest low-mass x-ray binary, Scorpius X-1. Our semicoherent analysis covers 10 days of LIGO S5 data ranging from 50–550 Hz, and performs an incoherent sum of coherent F -statistic power distributed a...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Aasi, J., Abbott, B. P., Abbott, R., Abbott, T., Abernathy, M. R., Acernese, F., Domínguez, Alfredo Eduardo, Maglione, César Germán, Ortega Larcher, Walter Emanuel, Quiroga, Gonzalo Damián, Reula, Oscar Alejandro
Formato: article
Lenguaje:Inglés
Publicado: 2022
Materias:
Acceso en línea:http://hdl.handle.net/11086/29514
https://doi.org/10.1103/PhysRevD.91.062008
Aporte de:
id I10-R141-11086-29514
record_format dspace
institution Universidad Nacional de Córdoba
institution_str I-10
repository_str R-141
collection Repositorio Digital Universitario (UNC)
language Inglés
topic Gravitational waves
Neutron stars
X-ray binaries
General Relativity and Quantum Cosmology
Astrophysics
High Energy Astrophysical Phenomena
spellingShingle Gravitational waves
Neutron stars
X-ray binaries
General Relativity and Quantum Cosmology
Astrophysics
High Energy Astrophysical Phenomena
Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Acernese, F.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
topic_facet Gravitational waves
Neutron stars
X-ray binaries
General Relativity and Quantum Cosmology
Astrophysics
High Energy Astrophysical Phenomena
description We present results of a search for continuously emitted gravitational radiation, directed at the brightest low-mass x-ray binary, Scorpius X-1. Our semicoherent analysis covers 10 days of LIGO S5 data ranging from 50–550 Hz, and performs an incoherent sum of coherent F -statistic power distributed amongst frequency-modulated orbital sidebands. All candidates not removed at the veto stage were found to be consistent with noise at a 1% false alarm rate. We present Bayesian 95% confidence upper limits on gravitational-wave strain amplitude using two different prior distributions: a standard one, with no a priori assumptions about the orientation of Scorpius X-1; and an angle-restricted one, using a prior derived from electromagnetic observations. Median strain upper limits of 1.3 × 10−24 and 8 × 10−25 are reported at 150 Hz for the standard and angle-restricted searches respectively. This proof-of-principle analysis was limited to a short observation time by unknown effects of accretion on the intrinsic spin frequency of the neutron star, but improves upon previous upper limits by factors of ∼1.4 for the standard, and 2.3 for the angle-restricted search at the sensitive region of the detector.
format article
author Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Acernese, F.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
author_facet Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Acernese, F.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
author_sort Aasi, J.
title Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
title_short Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
title_full Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
title_fullStr Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
title_full_unstemmed Directed search for gravitational waves from Scorpius X-1 with initial LIGO data
title_sort directed search for gravitational waves from scorpius x-1 with initial ligo data
publishDate 2022
url http://hdl.handle.net/11086/29514
https://doi.org/10.1103/PhysRevD.91.062008
work_keys_str_mv AT aasij directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT abbottbp directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT abbottr directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT abbottt directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT abernathymr directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT acernesef directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT dominguezalfredoeduardo directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT maglionecesargerman directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT ortegalarcherwalteremanuel directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT quirogagonzalodamian directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
AT reulaoscaralejandro directedsearchforgravitationalwavesfromscorpiusx1withinitialligodata
bdutipo_str Repositorios
_version_ 1764820392260665346