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Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs
R Abbott, H Abe, F Acernese, K Ackley, N Adhikari, RX Adhikari, VK Adkins, VB Adya, C Affeldt, D Agarwal, M Agathos, K Agatsuma, N Aggarwal, OD Aguiar, L Aiello, A Ain, P Ajith, T Akutsu, S Albanesi, RA Alfaidi, A Allocca, PA Altin, A Amato, C Anand, S Anand, A Ananyeva, SB Anderson, WG Anderson, M Ando, T Andrade, N Andres, M Andrés-Carcasona, T Andrić, SV Angelova, S Ansoldi, JM Antelis, S Antier, T Apostolatos, EZ Appavuravther, S Appert, SK Apple, K Arai, A Araya, MC Araya, JS Areeda, M Arène, N Aritomi, N Arnaud, M Arogeti, SM Aronson, KG Arun, H Asada, Y Asali, G Ashton, Y Aso, M Assiduo, SA de Souza Melo, SM Aston, P Astone, F Aubin, K AultONeal, C Austin, S Babak, F Badaracco, MKM Bader, C Badger, S Bae, Y Bae, AM Baer, S Bagnasco, Y Bai, M Bailes, J Baird, R Bajpai, T Baka, M Ball, G Ballardin, SW Ballmer, A Balsamo, G Baltus, S Banagiri, B Banerjee, D Bankar, JC Barayoga, C Barbieri, BC Barish, D Barker, P Barneo, F Barone, B Barr, L Barsotti, M Barsuglia, D Barta, J Bartlett, MA Barton, I Bartos, S Basak, R Bassiri, A Basti, M Bawaj
Aug 08, 2022
We present a targeted search for continuous gravitational waves (GWs) from
236 pulsars using data from the third observing run of LIGO and Virgo (O3)
combined with data from the second observing run (O2). Searches were...
Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run
R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, N Adhikari, RX Adhikari, VB Adya, C Affeldt, D Agarwal, M Agathos, K Agatsuma, N Aggarwal, OD Aguiar, L Aiello, A Ain, P Ajith, T Akutsu, S Albanesi, A Allocca, PA Altin, A Amato, C Anand, S Anand, A Ananyeva, SB Anderson, WG Anderson, M Ando, T Andrade, N Andres, T Andrić, SV Angelova, S Ansoldi, JM Antelis, S Antier, S Appert, K Arai, K Arai, Y Arai, S Araki, A Araya, MC Araya, JS Areeda, M Arène, N Aritomi, N Arnaud, SM Aronson, KG Arun, H Asada, Y Asali, G Ashton, Y Aso, M Assiduo, SM Aston, P Astone, F Aubin, C Austin, S Babak, F Badaracco, MKM Bader, C Badger, S Bae, Y Bae, AM Baer, S Bagnasco, Y Bai, M Bailes, L Baiotti, J Baird, R Bajpai, M Ball, G Ballardin, SW Ballmer, A Balsamo, G Baltus, S Banagiri, D Bankar, JC Barayoga, C Barbieri, BC Barish, D Barker, P Barneo, F Barone, B Barr, L Barsotti, M Barsuglia, D Barta, J Bartlett, MA Barton, I Bartos, R Bassiri, A Basti, M Bawaj, JC Bayley, AC Baylor, M Bazzan, B Bécsy, VM Bedakihale, M Bejger, I Belahcene
Jun 29, 2022
Isolated neutron stars that are asymmetric with respect to their spin axis
are possible sources of detectable continuous gravitational waves. This paper
presents a fully-coherent search for such signals from eighteen pulsars in...