
Indexed in
License and use
Citations
Analysis of institutional authors
Ruiz Morales, Maria EsterAuthorSearch 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
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
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
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.