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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45QF2N2
Repositorysid.inpe.br/mtc-m21d/2021/11.16.13.57
Last Update2021:11.16.13.57.19 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2021/11.16.13.57.19
Metadata Last Update2022:04.03.19.24.06 (UTC) administrator
DOI10.3847/1538-4357/ac17ea
ISSN0004-637X
1538-4357
Label20210628
Citation KeyAasiAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBB:2021:SeCoGr
TitleSearches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo
Year2021
MonthNov.
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size8754 KiB
2. Context
Author  1 Aasi, J.
  2 Abbott, R.
  3 Abbott, T. D.
  4 Abraham, S.
  5 Acernese, F.
  6 Ackley, K.
  7 Adams, A.
  8 Adams, C.
  9 Adhikari, R. X.
 10 Adya, V. B.
 11 Affeldt, C.
 12 Agathos, M.
 13 Agatsuma, K.
 14 Aggarwal, N.
 15 Aguiar, Odylio Denys de
 16 Aiello, L.
 17 Ain, A.
 18 Ajith, P.
 19 Akcay, S.
 20 Allen, G.
 21 Allocca, A.
 22 Altin, P. A.
 23 Amato, A.
 24 Anand, S.
 25 Ananyeva, A.
 26 Anderson, S. B.
 27 Anderson, W. G.
 28 Angelova, S. V.
 29 Ansoldi, S.
 30 Antelis, J. M.
 31 Antier, S.
 32 Appert, S.
 33 Arai, K.
 34 Araya, M. C.
 35 Areeda, J. S.
 36 Arène, M.
 37 Arnaud, N.
 38 Aronson, S. M.
 39 Arun, K. G.
 40 Asali, Y.
 41 Ascenzi, S.
 42 Ashton, G.
 43 Aston, S. M.
 44 Astone, P.
 45 Aubin, F.
 46 Aufmuth, P.
 47 Aultoneal, K.
 48 Austin, C.
 49 Avendano, V.
 50 Babak, S.
 51 Badaracco, F.
 52 Bader, M. K. M.
 53 Bae, S.
 54 Baer, A. M.
 55 Bagnasco, S.
 56 Baird, J.
 57 Ball, M.
 58 Ballardin, G.
 59 Ballmer, S. W.
 60 Bals, A.
 61 Balsamo, A.
 62 Baltus, G.
 63 Banagiri, S.
 64 Bankar, D.
 65 Bankar, R. S.
 66 Barayoga, J. C.
 67 Barbieri, C.
 68 Barish, B. C.
 69 Barker, D.
 70 Barneo, P.
 71 Barnum, S.
 72 Barone, F.
 73 Barr, B.
 74 Barsotti, L.
 75 Barsuglia, M.
 76 Barta, D.
 77 Bartlett, J.
 78 Bartos, I.
 79 Bassiri, R.
 80 Basti, A.
 81 Bawaj, M.
 82 Bayley, J. C.
 83 Bazzan, M.
 84 Becher, B. R.
 85 Bécsy, B.
 86 Bedakihale, V. M.
 87 Bejger, M.
 88 Belahcene, I.
 89 Beniwal, D.
 90 Benjamin, M. G.
 91 Benkel, R.
 92 Bennett, T. F.
 93 Bentley, J. D.
 94 Bergamin, F.
 95 Berger, B. K.
 96 Bergmann, G.
 97 Bernuzzi, S.
 98 Berry, C. P. L.
 99 Bersanetti, D.
100 Bertolini, A.
101 Betzwieser, J.
102 Bhandare, R.
103 Bhandari, A. V.
104 Bhattacharjee, D.
105 Bidler, J.
106 Bilenko, I. A.
107 Billingsley, G.
108 Birney, R.
109 Birnholtz
110 O. .
Resume Identifier  1
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 15 8JMKD3MGP5W/3C9JJ2A
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 15 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation  1
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 15 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address  1
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 15 odylio.aguiar@gmail.com
JournalAstrophysical Journal
Volume921
Number1
Pagese80
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
History (UTC)2021-11-16 13:57:19 :: simone -> administrator ::
2022-04-03 19:24:06 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
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Content TypeExternal Contribution
Version Typepublisher
AbstractWe 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.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Searches for Continuous...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/45QF2N2
zipped data URLhttp://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/45QF2N2
Languageen
Target FileAbbott_2021_ApJ_921_80.pdf
User Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 2
sid.inpe.br/mtc-m21/2012/07.13.14.57.26 2
URL (untrusted data)https://www.scopus.com/inward/record.uri?eid=2-s2.0-85108209768&doi=10.1103%2fPhysRevD.103.122002&partnerID=40&md5=2afc88279299b10b56e641010b5e8e79
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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