@Article{AasiAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBB:2021:SeCoGr,
               author = "Aasi, J. and Abbott, R. and Abbott, T. D. and Abraham, S. and 
                         Acernese, F. and Ackley, K. and Adams, A. and Adams, C. and 
                         Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. 
                         and Agatsuma, K. and Aggarwal, N. and Aguiar, Odylio Denys de and 
                         Aiello, L. and Ain, A. and Ajith, P. and Akcay, S. and Allen, G. 
                         and Allocca, A. and Altin, P. A. and Amato, A. and Anand, S. and 
                         Ananyeva, A. and Anderson, S. B. and Anderson, W. G. and Angelova, 
                         S. V. and Ansoldi, S. and Antelis, J. M. and Antier, S. and 
                         Appert, S. and Arai, K. and Araya, M. C. and Areeda, J. S. and 
                         Ar{\`e}ne, M. and Arnaud, N. and Aronson, S. M. and Arun, K. G. 
                         and Asali, Y. and Ascenzi, S. and Ashton, G. and Aston, S. M. and 
                         Astone, P. and Aubin, F. and Aufmuth, P. and Aultoneal, K. and 
                         Austin, C. and Avendano, V. and Babak, S. and Badaracco, F. and 
                         Bader, M. K. M. and Bae, S. and Baer, A. M. and Bagnasco, S. and 
                         Baird, J. and Ball, M. and Ballardin, G. and Ballmer, S. W. and 
                         Bals, A. and Balsamo, A. and Baltus, G. and Banagiri, S. and 
                         Bankar, D. and Bankar, R. S. and Barayoga, J. C. and Barbieri, C. 
                         and Barish, B. C. and Barker, D. and Barneo, P. and Barnum, S. and 
                         Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and 
                         Barta, D. and Bartlett, J. and Bartos, I. and Bassiri, R. and 
                         Basti, A. and Bawaj, M. and Bayley, J. C. and Bazzan, M. and 
                         Becher, B. R. and B{\'e}csy, B. and Bedakihale, V. M. and Bejger, 
                         M. and Belahcene, I. and Beniwal, D. and Benjamin, M. G. and 
                         Benkel, R. and Bennett, T. F. and Bentley, J. D. and Bergamin, F. 
                         and Berger, B. K. and Bergmann, G. and Bernuzzi, S. and Berry, C. 
                         P. L. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and 
                         Bhandare, R. and Bhandari, A. V. and Bhattacharjee, D. and Bidler, 
                         J. and Bilenko, I. A. and Billingsley, G. and Birney, R. and 
                         Birnholtz and {O. .}",
          affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
                         and {} and {} and {} and {} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)}",
                title = "Searches for Continuous Gravitational Waves from Young Supernova 
                         Remnants in the Early Third Observing Run of Advanced LIGO and 
                         Virgo",
              journal = "Astrophysical Journal",
                 year = "2021",
               volume = "921",
               number = "1",
                pages = "e80",
                month = "Nov.",
             abstract = "We present results of three wide-band directed searches for 
                         continuous gravitational waves from 15 young supernova remnants in 
                         the first half of the third Advanced LIGO and Virgo observing run. 
                         We use three search pipelines with distinct signal models and 
                         methods of identifying noise artifacts. Without ephemerides of 
                         these sources, the searches are conducted over a fRequency band 
                         spanning from 10 to 2 kHz. We find no evidence of continuous 
                         gravitational radiation from these sources. We set upper limits on 
                         the intrinsic signal strain at 95% confidence level in sample 
                         subbands, estimate the sensitivity in the full band, and derive 
                         the corresponding constraints on the fiducial neutron star 
                         ellipticity and r-mode amplitude. The best 95% confidence 
                         constraints placed on the signal strain are 7.7 x 10(-26) and 7.8 
                         x 10(-26) near 200 Hz for the supernova remnants G39.2-0.3 and 
                         G65.7+1.2, respectively. The most stringent constraints on the 
                         ellipticity and r-mode amplitude reach less than or similar to 
                         10(-7) and less than or similar to 10(-5), respectively, at 
                         frequencies above similar to 400 Hz for the closest supernova 
                         remnant G266.2-1.2/Vela Jr.",
                  doi = "10.3847/1538-4357/ac17ea",
                  url = "http://dx.doi.org/10.3847/1538-4357/ac17ea",
                 issn = "0004-637X and 1538-4357",
                label = "20210628",
             language = "en",
           targetfile = "Abbott_2021_ApJ_921_80.pdf",
                  url = "https://www.scopus.com/inward/record.uri?eid=2-s2.0-85108209768\&doi=10.1103%2fPhysRevD.103.122002\&partnerID=40\&md5=2afc88279299b10b56e641010b5e8e79",
        urlaccessdate = "02 maio 2024"
}