First search for gravitational wave bursts with a network of detectors
We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with more than two detectors observing simultaneously. No gravitational wave burst was detected. The false al...
Gespeichert in:
| Veröffentlicht in: | Physical review letters 2000-12, Vol.85 (24), p.5046-5050 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 5050 |
|---|---|
| container_issue | 24 |
| container_start_page | 5046 |
| container_title | Physical review letters |
| container_volume | 85 |
| creator | Allen, ZA Astone, P Baggio, L Busby, D Bassan, M Blair, DG Bonaldi, M Bonifazi, P Carelli, P Cerdonio, M Coccia, E Conti, L Cosmelli, C Crivelli Visconti V D'Antonio, S Fafone, V, V Falferi, P Fortini, P Frasca, S Hamilton, WO Heng, IS Ivanov, EN Johnson, WW Kingham, M Locke, CR Marini, A |
| description | We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with more than two detectors observing simultaneously. No gravitational wave burst was detected. The false alarm rate was lower than 1 per 10(4) yr when three or more detectors were operating simultaneously. The typical threshold was H approximately 4x10(-21) Hz-1 on the Fourier component at approximately 10(3) Hz of the gravitational wave strain amplitude. New upper limits for amplitude and rate of gravitational wave bursts have been set. |
| doi_str_mv | 10.1103/PhysRevLett.85.5046 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1859334127</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1859334127</sourcerecordid><originalsourceid>FETCH-LOGICAL-c303t-8babf4f482c326609a4b2ed8e324078a80de56264c892a0bacd47eb6f94d47123</originalsourceid><addsrcrecordid>eNpNkE1Lw0AURQdRbK3-AkFm6Sb1zUeSyVKKUaGgiK6HyeTFRtNOnZm09N-b0oKu3l2cex8cQq4ZTBkDcfe62IU33MwxxqlKpynI7ISMGeRFkjMmT8kYQLCkAMhH5CKELwBgPFPnZMSGAc6UGJOybH2INKDxdkEb5-mnN5s2mti6leno1myQVv3ABLpt44IausK4df6buobWGNFG58MlOWtMF_DqeCfko3x4nz0l85fH59n9PLECRExUZapGNlJxK3iWQWFkxbFWKLiEXBkFNaYZz6RVBTdQGVvLHKusKeQQGBcTcnvYXXv302OIetkGi11nVuj6oJlKCyEk4_mAigNqvQvBY6PXvl0av9MM9F6g_idQq1TvBQ6tm-ODvlpi_dc5GhO_-ZxvNA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1859334127</pqid></control><display><type>article</type><title>First search for gravitational wave bursts with a network of detectors</title><source>American Physical Society Journals</source><creator>Allen, ZA ; Astone, P ; Baggio, L ; Busby, D ; Bassan, M ; Blair, DG ; Bonaldi, M ; Bonifazi, P ; Carelli, P ; Cerdonio, M ; Coccia, E ; Conti, L ; Cosmelli, C ; Crivelli Visconti V ; D'Antonio, S ; Fafone, V, V ; Falferi, P ; Fortini, P ; Frasca, S ; Hamilton, WO ; Heng, IS ; Ivanov, EN ; Johnson, WW ; Kingham, M ; Locke, CR ; Marini, A</creator><creatorcontrib>Allen, ZA ; Astone, P ; Baggio, L ; Busby, D ; Bassan, M ; Blair, DG ; Bonaldi, M ; Bonifazi, P ; Carelli, P ; Cerdonio, M ; Coccia, E ; Conti, L ; Cosmelli, C ; Crivelli Visconti V ; D'Antonio, S ; Fafone, V, V ; Falferi, P ; Fortini, P ; Frasca, S ; Hamilton, WO ; Heng, IS ; Ivanov, EN ; Johnson, WW ; Kingham, M ; Locke, CR ; Marini, A</creatorcontrib><description>We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with more than two detectors observing simultaneously. No gravitational wave burst was detected. The false alarm rate was lower than 1 per 10(4) yr when three or more detectors were operating simultaneously. The typical threshold was H approximately 4x10(-21) Hz-1 on the Fourier component at approximately 10(3) Hz of the gravitational wave strain amplitude. New upper limits for amplitude and rate of gravitational wave bursts have been set.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.85.5046</identifier><identifier>PMID: 11102183</identifier><language>eng</language><publisher>United States</publisher><ispartof>Physical review letters, 2000-12, Vol.85 (24), p.5046-5050</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c303t-8babf4f482c326609a4b2ed8e324078a80de56264c892a0bacd47eb6f94d47123</citedby><cites>FETCH-LOGICAL-c303t-8babf4f482c326609a4b2ed8e324078a80de56264c892a0bacd47eb6f94d47123</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,2863,2864,27901,27902</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/11102183$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Allen, ZA</creatorcontrib><creatorcontrib>Astone, P</creatorcontrib><creatorcontrib>Baggio, L</creatorcontrib><creatorcontrib>Busby, D</creatorcontrib><creatorcontrib>Bassan, M</creatorcontrib><creatorcontrib>Blair, DG</creatorcontrib><creatorcontrib>Bonaldi, M</creatorcontrib><creatorcontrib>Bonifazi, P</creatorcontrib><creatorcontrib>Carelli, P</creatorcontrib><creatorcontrib>Cerdonio, M</creatorcontrib><creatorcontrib>Coccia, E</creatorcontrib><creatorcontrib>Conti, L</creatorcontrib><creatorcontrib>Cosmelli, C</creatorcontrib><creatorcontrib>Crivelli Visconti V</creatorcontrib><creatorcontrib>D'Antonio, S</creatorcontrib><creatorcontrib>Fafone, V, V</creatorcontrib><creatorcontrib>Falferi, P</creatorcontrib><creatorcontrib>Fortini, P</creatorcontrib><creatorcontrib>Frasca, S</creatorcontrib><creatorcontrib>Hamilton, WO</creatorcontrib><creatorcontrib>Heng, IS</creatorcontrib><creatorcontrib>Ivanov, EN</creatorcontrib><creatorcontrib>Johnson, WW</creatorcontrib><creatorcontrib>Kingham, M</creatorcontrib><creatorcontrib>Locke, CR</creatorcontrib><creatorcontrib>Marini, A</creatorcontrib><title>First search for gravitational wave bursts with a network of detectors</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with more than two detectors observing simultaneously. No gravitational wave burst was detected. The false alarm rate was lower than 1 per 10(4) yr when three or more detectors were operating simultaneously. The typical threshold was H approximately 4x10(-21) Hz-1 on the Fourier component at approximately 10(3) Hz of the gravitational wave strain amplitude. New upper limits for amplitude and rate of gravitational wave bursts have been set.</description><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNpNkE1Lw0AURQdRbK3-AkFm6Sb1zUeSyVKKUaGgiK6HyeTFRtNOnZm09N-b0oKu3l2cex8cQq4ZTBkDcfe62IU33MwxxqlKpynI7ISMGeRFkjMmT8kYQLCkAMhH5CKELwBgPFPnZMSGAc6UGJOybH2INKDxdkEb5-mnN5s2mti6leno1myQVv3ABLpt44IausK4df6buobWGNFG58MlOWtMF_DqeCfko3x4nz0l85fH59n9PLECRExUZapGNlJxK3iWQWFkxbFWKLiEXBkFNaYZz6RVBTdQGVvLHKusKeQQGBcTcnvYXXv302OIetkGi11nVuj6oJlKCyEk4_mAigNqvQvBY6PXvl0av9MM9F6g_idQq1TvBQ6tm-ODvlpi_dc5GhO_-ZxvNA</recordid><startdate>20001211</startdate><enddate>20001211</enddate><creator>Allen, ZA</creator><creator>Astone, P</creator><creator>Baggio, L</creator><creator>Busby, D</creator><creator>Bassan, M</creator><creator>Blair, DG</creator><creator>Bonaldi, M</creator><creator>Bonifazi, P</creator><creator>Carelli, P</creator><creator>Cerdonio, M</creator><creator>Coccia, E</creator><creator>Conti, L</creator><creator>Cosmelli, C</creator><creator>Crivelli Visconti V</creator><creator>D'Antonio, S</creator><creator>Fafone, V, V</creator><creator>Falferi, P</creator><creator>Fortini, P</creator><creator>Frasca, S</creator><creator>Hamilton, WO</creator><creator>Heng, IS</creator><creator>Ivanov, EN</creator><creator>Johnson, WW</creator><creator>Kingham, M</creator><creator>Locke, CR</creator><creator>Marini, A</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>20001211</creationdate><title>First search for gravitational wave bursts with a network of detectors</title><author>Allen, ZA ; Astone, P ; Baggio, L ; Busby, D ; Bassan, M ; Blair, DG ; Bonaldi, M ; Bonifazi, P ; Carelli, P ; Cerdonio, M ; Coccia, E ; Conti, L ; Cosmelli, C ; Crivelli Visconti V ; D'Antonio, S ; Fafone, V, V ; Falferi, P ; Fortini, P ; Frasca, S ; Hamilton, WO ; Heng, IS ; Ivanov, EN ; Johnson, WW ; Kingham, M ; Locke, CR ; Marini, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c303t-8babf4f482c326609a4b2ed8e324078a80de56264c892a0bacd47eb6f94d47123</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Allen, ZA</creatorcontrib><creatorcontrib>Astone, P</creatorcontrib><creatorcontrib>Baggio, L</creatorcontrib><creatorcontrib>Busby, D</creatorcontrib><creatorcontrib>Bassan, M</creatorcontrib><creatorcontrib>Blair, DG</creatorcontrib><creatorcontrib>Bonaldi, M</creatorcontrib><creatorcontrib>Bonifazi, P</creatorcontrib><creatorcontrib>Carelli, P</creatorcontrib><creatorcontrib>Cerdonio, M</creatorcontrib><creatorcontrib>Coccia, E</creatorcontrib><creatorcontrib>Conti, L</creatorcontrib><creatorcontrib>Cosmelli, C</creatorcontrib><creatorcontrib>Crivelli Visconti V</creatorcontrib><creatorcontrib>D'Antonio, S</creatorcontrib><creatorcontrib>Fafone, V, V</creatorcontrib><creatorcontrib>Falferi, P</creatorcontrib><creatorcontrib>Fortini, P</creatorcontrib><creatorcontrib>Frasca, S</creatorcontrib><creatorcontrib>Hamilton, WO</creatorcontrib><creatorcontrib>Heng, IS</creatorcontrib><creatorcontrib>Ivanov, EN</creatorcontrib><creatorcontrib>Johnson, WW</creatorcontrib><creatorcontrib>Kingham, M</creatorcontrib><creatorcontrib>Locke, CR</creatorcontrib><creatorcontrib>Marini, A</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Allen, ZA</au><au>Astone, P</au><au>Baggio, L</au><au>Busby, D</au><au>Bassan, M</au><au>Blair, DG</au><au>Bonaldi, M</au><au>Bonifazi, P</au><au>Carelli, P</au><au>Cerdonio, M</au><au>Coccia, E</au><au>Conti, L</au><au>Cosmelli, C</au><au>Crivelli Visconti V</au><au>D'Antonio, S</au><au>Fafone, V, V</au><au>Falferi, P</au><au>Fortini, P</au><au>Frasca, S</au><au>Hamilton, WO</au><au>Heng, IS</au><au>Ivanov, EN</au><au>Johnson, WW</au><au>Kingham, M</au><au>Locke, CR</au><au>Marini, A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>First search for gravitational wave bursts with a network of detectors</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2000-12-11</date><risdate>2000</risdate><volume>85</volume><issue>24</issue><spage>5046</spage><epage>5050</epage><pages>5046-5050</pages><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We report the initial results from a search for bursts of gravitational radiation by a network of five cryogenic resonant detectors during 1997 and 1998. This is the first significant search with more than two detectors observing simultaneously. No gravitational wave burst was detected. The false alarm rate was lower than 1 per 10(4) yr when three or more detectors were operating simultaneously. The typical threshold was H approximately 4x10(-21) Hz-1 on the Fourier component at approximately 10(3) Hz of the gravitational wave strain amplitude. New upper limits for amplitude and rate of gravitational wave bursts have been set.</abstract><cop>United States</cop><pmid>11102183</pmid><doi>10.1103/PhysRevLett.85.5046</doi><tpages>5</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2000-12, Vol.85 (24), p.5046-5050 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1859334127 |
| source | American Physical Society Journals |
| title | First search for gravitational wave bursts with a network of detectors |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T23%3A16%3A03IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=First%20search%20for%20gravitational%20wave%20bursts%20with%20a%20network%20of%20detectors&rft.jtitle=Physical%20review%20letters&rft.au=Allen,%20ZA&rft.date=2000-12-11&rft.volume=85&rft.issue=24&rft.spage=5046&rft.epage=5050&rft.pages=5046-5050&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.85.5046&rft_dat=%3Cproquest_cross%3E1859334127%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1859334127&rft_id=info:pmid/11102183&rfr_iscdi=true |