Authors
Benjamin P Abbott, R Abbott, TD Abbott, S Abraham, Fausto Acernese, K Ackley, C Adams, Rana X Adhikari, VB Adya, C Affeldt, M Agathos, Kazuhiro Agatsuma, N Aggarwal, OD Aguiar, L Aiello, A Ain, P Ajith, G Allen, A Allocca, MA Aloy, PA Altin, A Amato, A Ananyeva, SB Anderson, WG Anderson, SV Angelova, S Antier, S Appert, K Arai, MC Araya, JS Areeda, M Arène, N Arnaud, STEFANO Ascenzi, G Ashton, SM Aston, P Astone, Francois Aubin, P Aufmuth, K Aultoneal, C Austin, V Avendano, A Avila-Alvarez, Stanislav Babak, P Bacon, F Badaracco, MKM Bader, S Bae, M Bailes, PT Baker, F Baldaccini, G Ballardin, SW Ballmer, S Banagiri, JC Barayoga, SE Barclay, BC Barish, D Barker, K Barkett, S Barnum, F Barone, Bryan Barr, L Barsotti, Matteo Barsuglia, D Barta, J Bartlett, Imre Bartos, R Bassiri, A Basti, M Bawaj, Joseph C Bayley, M Bazzan, B Bécsy, Michal Bejger, I Belahcene, AS Bell, D Beniwal, BK Berger, G Bergmann, S Bernuzzi, JJ Bero, Christopher PL Berry, D Bersanetti, A Bertolini, J Betzwieser, R Bhandare, J Bidler, IA Bilenko, SA Bilgili, G Billingsley, J Birch, R Birney, O Birnholtz, S Biscans, S Biscoveanu, A Bisht, M Bitossi, MA Bizouard, JK Blackburn, CD Blair, DG Blair, RM Blair, Steven Bloemen, N Bode, M Boer, Y Boetzel, G Bogaert, François Bondu, E Bonilla, R Bonnand, P Booker, BA Boom, CD Booth, R Bork, V Boschi, S Bose, K Bossie, V Bossilkov, J Bosveld, Y Bouffanais, A Bozzi, C Bradaschia, PR Brady, A Bramley, M Branchesi, JE Brau, T Briant, JH Briggs, F Brighenti, A Brillet, M Brinkmann, V Brisson, P Brockill, AF Brooks, DD Brown, S Brunett, A Buikema, Tomasz Bulik, HJ Bulten, A Buonanno, D Buskulic, Christelle Buy, RL Byer, M Cabero, Laura Cadonati, G Cagnoli, C Cahillane, J Calderón Bustillo, TA Callister, E Calloni
Publication date
2019/6/26
Journal
The Astrophysical Journal
Volume
879
Issue
1
Pages
10
Publisher
IOP Publishing
Description
There have been several previous searches for persistent (or continuous) quasi-monochromatic gravitational waves emitted by a selection of known pulsars using data from the LIGO, Virgo, and GEO600 gravitational-wave detectors (Abbott et al. 2004, 2005, 2017a, 2007, 2008, 2010; Abadie et al. 2011; Aasi et al. 2014). In the majority of these, the signals that have been searched for are those that would be expected from stars with a nonzero l= m= 2 mass quadrupole moment Q22 and with polarization content consistent with the expectations of general relativity (see, eg, Zimmermann & Szedenits 1979; Bonazzola & Gourgoulhon 1996; Jaranowski et al. 1998). Such signals would be produced at twice the stellar rotation frequencies, and searches have generally assumed that the rotation frequency derived from electromagnetic observations of the pulsars is phase locked to the star, s rotation and thus the …
Total citations
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