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Ruiz Morales, Maria EsterAuthor

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May 15, 2025
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Search for Continuous Gravitational Waves from Known Pulsars in the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Publicated to:Astrophysical Journal. 983 (2): - 2025-04-20 983(2), DOI: 10.3847/1538-4357/adb3a0

Authors: Abac AG; Abbott R; Abouelfettouh I; Acernese F; Ackley K; Adhicary S; Adhikari N; Adhikari RX; Adkins VK; Agarwal D; Agathos M; Aghaei Abchouyeh M; Aguiar OD; Aguilar I; Aiello L; Ain A; Ajith P; Akutsu T; Albanesi S; Alfaidi RA; Al-Jodah A; Alléné C; Allocca A; Al-Shammari S; Altin PA; Alvarez-Lopez S; Amato A; Amez-Droz L; Amorosi A; Amra C; Ananyeva A; Anderson SB; Anderson WG; Andia M; Ando M; Andrade T; Andres N; Andrés-Carcasona M; Andrić T; Anglin J; Ansoldi S; Antelis JM; Antier S; Aoumi M; Appavuravther EZ; Appert S; Apple SK; Arai K; Araya A; Araya MC; Areeda JS; Argianas L; Aritomi N; Armato F; Arnaud N; Arogeti M; Aronson SM; Ashton G; Aso Y; Assiduo M; Assis de Souza Melo S; Aston SM; Astone P; Attadio F; Aubin F; AultONeal K; Avallone G; Babak S; Badaracco F; Badger C; Bae S; Bagnasco S; Bagui E; Baier JG; Baiotti L; Bajpai R; Baka T; Ball M; Ballardin G; Ballmer SW; Banagiri S; Banerjee B; Bankar D; Baral P; Barayoga JC; Barish BC; Barker D; Barneo P; Barone F; Barr B; Barsotti L; Barsuglia M; Barta D; Bartoletti AM; Barton MA; Bartos I; Basak S; Basalaev A; Bassiri R; Basti A

Affiliations

APC - AstroParticule et Cosmologie - Author
California Institute of Technology - Author
California State University, Fullerton - Author
Cardiff University - Author
Concordia University Wisconsin - Author
Embry-Riddle Aeronautical University, Prescott - Author
European Gravitational Observatory (EGO) - Author
Georgia Institute of Technology - Author
Gran Sasso Science Institute - Author
Institut de Física d'Altes Energies, Bellaterra - Author
Institut Fresnel - Author
Institut Pluridisciplinaire Hubert Curien - Author
Instituto Nacional de Pesquisas Espaciais - Author
Inter-University Centre for Astronomy and Astrophysics India - Author
Istituto Nazionale di Fisica Nucleare - INFN - Author
Istituto Nazionale di Fisica Nucleare - INFN; Sapienza Università di Roma - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Genova - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Genova; Università degli Studi di Genova - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli; Dipartimento di Medicina, Chirurgia e Odontoiatria “Scuola Medica Salernitana" - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli; Università degli Studi di Napoli Federico II - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Perugia; Università degli Studi di Camerino - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Torino - Author
Istituto Nazionale di Fisica Nucleare, Sezione di Torino; Friedrich-Schiller-Universität Jena; Università degli Studi di Torino - Author
Kenyon College - Author
King's College London - Author
Korea Institute of Science and Technology Information - Author
LIGO Hanford - Author
LIGO Livingston - Author
Louisiana State University - Author
Massachusetts Institute of Technology - Author
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) - Author
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut); Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut); Gottfried Wilhelm Leibniz Universität Hannover; Gran Sasso Science Institute - Author
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Author
National Institutes of Natural Sciences - National Astronomical Observatory of Japan; National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Author
National Institutes of Natural Sciences - National Astronomical Observatory of Japan; The Graduate University for Advanced Studies - Author
Northwestern University - Author
Observatoire de la Cote d'Azur - Author
Pennsylvania State University - Author
Queen Mary University of London - Author
Royal Holloway, University of London - Author
Sejong University - Author
Stanford University - Author
Syracuse University - Author
Tata Institute of Fundamental Research, Mumbai - Author
Tecnologico de Monterrey - Author
The Australian National University - Author
The University of Osaka - Author
The University of Tokyo - Author
The University of Western Australia - Author
Università degli Studi di Roma "Tor Vergata"; Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata; Cardiff University - Author
Università degli Studi di Salerno - Author
Università degli Studi di Salerno; Istituto Nazionale di Fisica Nucleare, Sezione di Napoli - Author
Università degli Studi di Udine; Istituto Nazionale di Fisica Nucleare, Sezione di Trieste - Author
Università degli Studi di Urbino Carlo Bo; Istituto Nazionale di Fisica Nucleare, Sezione di Firenze - Author
Università di Pisa; Istituto Nazionale di Fisica Nucleare, Sezione di Pisa - Author
Universitat de Barcelona - Author
Universitat de Barcelona; Universitat de Barcelona - Author
Universitat Hamburg - Author
Université Catholique de Louvain; Inter-University Centre for Astronomy and Astrophysics India - Author
Université Libre de Bruxelles - Author
Université Paris-Saclay - Author
Université Paris-Saclay; European Gravitational Observatory (EGO) - Author
Universite Savoie Mont Blanc - Author
Universiteit Antwerpen - Author
Universiteit Maastricht; FOM-Institute of Subatomic Physics - NIKHEF - Author
Universiteit Utrecht - Author
University of Florida - Author
University of Glasgow - Author
University of Oregon - Author
University of Warwick - Author
University of Washington - Author
University of Wisconsin-Milwaukee - Author
Villanova University - Author
Wigner Research Centre for Physics - Author
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Abstract

Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of general relativity. We present a search for CWs from a set of 45 known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run, known as O4a. We conducted a targeted search for each pulsar using three independent analysis methods considering single-harmonic and dual-harmonic emission models. We find no evidence of a CW signal in O4a data for both models and set upper limits on the signal amplitude and on the ellipticity, which quantifies the asymmetry in the neutron star mass distribution. For the single-harmonic emission model, 29 targets have the upper limit on the amplitude below the theoretical spin-down limit. The lowest upper limit on the amplitude is 6.4 × 10-27 for the young energetic pulsar J0537-6910, while the lowest constraint on the ellipticity is 8.8 × 10-9 for the bright nearby millisecond pulsar J0437-4715. Additionally, for a subset of 16 targets, we performed a narrowband search that is more robust regarding the emission model, with no evidence of a signal. We also found no evidence of nonstandard polarizations as predicted by the Brans-Dicke theory.

Keywords

Astronomia / físicaAstronomy & astrophysicsAstronomy and astrophysicsEngenharias iiiEngenharias ivEnsinoGeociênciasInterdisciplinarMateriaisQuímicaSpace and planetary science

Quality index

Bibliometric impact. Analysis of the contribution and dissemination channel

The work has been published in the journal Astrophysical Journal due to its progression and the good impact it has achieved in recent years, according to the agency WoS (JCR), it has become a reference in its field. In the year of publication of the work, 2025, it was in position 17/84, thus managing to position itself as a Q1 (Primer Cuartil), in the category Astronomy & Astrophysics.

Impact and social visibility

From the perspective of influence or social adoption, and based on metrics associated with mentions and interactions provided by agencies specializing in calculating the so-called "Alternative or Social Metrics," we can highlight as of 2025-07-23:

  • The use, from an academic perspective evidenced by the Altmetric agency indicator referring to aggregations made by the personal bibliographic manager Mendeley, gives us a total of: 8.

With a more dissemination-oriented intent and targeting more general audiences, we can observe other more global scores such as:

  • The Total Score from Altmetric: 202.5.
  • The number of mentions on the social network X (formerly Twitter): 1 (Altmetric).
  • The number of mentions in news outlets: 26 (Altmetric).

Leadership analysis of institutional authors

This work has been carried out with international collaboration, specifically with researchers from: Australia; Belgium; Brazil; France; Georgia; Germany; Gran Bretanya; Hungary; India; Italy; Japan; Mexico; Netherlands; Republic of Korea; United Kingdom; United States of America.