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Search for Gravitational Wave Bursts from Six Magnetars
Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitatio...
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Published in: | Astrophysical journal. Letters 2011-06, Vol.734 (2), p.L35-jQuery1323917158755='48' |
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container_title | Astrophysical journal. Letters |
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creator | Abernathy, M Affeldt, C Amariutei, D Aston, S. M Barnum, S Bilenko, I. A Biswas, R Black, E Blackburn, L Bland, B Boschi, V Braginsky, V. B Bulik, T Bulten, H. J Burguet-Castell, J Campsie, P Capano, C Cavalier, F Cella, G Clark, J Colla, A Das, K Day, R Dent, T Fiore, L. Di Dietz, A Farr, B. F Franc, J Frasconi, F Fulda, P Gáspár, M. E Giazotto, A Gill, C Goßler, S Guidi, G. M Gustafson, E. K Harms, J Hooper, S Howell, E. J Huttner, S. H Katsavounidis, E Katzman, W Keppel, D. G Klimenko, S Krishnan, B Leaci, P Leroy, N Liguori, N Mandel, I Márka, Z Maros, E Martin, I. W Meadors, G Mehmet, M Meyer, M. S Minenkov, Y Moscatelli, V Nash, T Nishida, E Ottens, R. S Patel, P Penn, S Perreca, A Phelps, M Pietka, M Plissi, M. V Postiglione, F Quetschke, V Rakhmanov, M Rankins, B Robinet, F Rocchi, A Romano, R Romie, J. H Ruggi, P Salit, M de la Jordana, L. Sancho Santamaría, L Schilling, R Schnabel, R Searle, A. C Sengupta, A. S Shihan Weerathunga, T Shoemaker, D. H Singer, L Soto, J Steplewski, S Sung, M Sutton, P. J Tarabrin, S. P Taylor, R Toncelli, A Travasso, F Vass, S Willke, B Yamamoto, H Zhang, Z Frederiks, D. D Kouveliotou, C Tashiro, M. S |
description | Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0--5408, gave a burst with an estimated isotropic energy >1044 erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 X 1044 d 2 1 erg and 1.4 X 1047 d 2 1 erg, respectively, where and d 0501 is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time. |
doi_str_mv | 10.1088/2041-8205/734/2/L35 |
format | article |
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M ; Barnum, S ; Bilenko, I. A ; Biswas, R ; Black, E ; Blackburn, L ; Bland, B ; Boschi, V ; Braginsky, V. B ; Bulik, T ; Bulten, H. J ; Burguet-Castell, J ; Campsie, P ; Capano, C ; Cavalier, F ; Cella, G ; Clark, J ; Colla, A ; Das, K ; Day, R ; Dent, T ; Fiore, L. Di ; Dietz, A ; Farr, B. F ; Franc, J ; Frasconi, F ; Fulda, P ; Gáspár, M. E ; Giazotto, A ; Gill, C ; Goßler, S ; Guidi, G. M ; Gustafson, E. K ; Harms, J ; Hooper, S ; Howell, E. J ; Huttner, S. H ; Katsavounidis, E ; Katzman, W ; Keppel, D. G ; Klimenko, S ; Krishnan, B ; Leaci, P ; Leroy, N ; Liguori, N ; Mandel, I ; Márka, Z ; Maros, E ; Martin, I. W ; Meadors, G ; Mehmet, M ; Meyer, M. S ; Minenkov, Y ; Moscatelli, V ; Nash, T ; Nishida, E ; Ottens, R. S ; Patel, P ; Penn, S ; Perreca, A ; Phelps, M ; Pietka, M ; Plissi, M. V ; Postiglione, F ; Quetschke, V ; Rakhmanov, M ; Rankins, B ; Robinet, F ; Rocchi, A ; Romano, R ; Romie, J. H ; Ruggi, P ; Salit, M ; de la Jordana, L. Sancho ; Santamaría, L ; Schilling, R ; Schnabel, R ; Searle, A. C ; Sengupta, A. S ; Shihan Weerathunga, T ; Shoemaker, D. H ; Singer, L ; Soto, J ; Steplewski, S ; Sung, M ; Sutton, P. J ; Tarabrin, S. P ; Taylor, R ; Toncelli, A ; Travasso, F ; Vass, S ; Willke, B ; Yamamoto, H ; Zhang, Z ; Frederiks, D. D ; Kouveliotou, C ; Tashiro, M. S</creator><creatorcontrib>Abernathy, M ; Affeldt, C ; Amariutei, D ; Aston, S. M ; Barnum, S ; Bilenko, I. A ; Biswas, R ; Black, E ; Blackburn, L ; Bland, B ; Boschi, V ; Braginsky, V. B ; Bulik, T ; Bulten, H. J ; Burguet-Castell, J ; Campsie, P ; Capano, C ; Cavalier, F ; Cella, G ; Clark, J ; Colla, A ; Das, K ; Day, R ; Dent, T ; Fiore, L. Di ; Dietz, A ; Farr, B. F ; Franc, J ; Frasconi, F ; Fulda, P ; Gáspár, M. E ; Giazotto, A ; Gill, C ; Goßler, S ; Guidi, G. M ; Gustafson, E. K ; Harms, J ; Hooper, S ; Howell, E. J ; Huttner, S. H ; Katsavounidis, E ; Katzman, W ; Keppel, D. 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S ; The LIGO Scientific Collaboration and the Virgo Collaboration</creatorcontrib><description>Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0--5408, gave a burst with an estimated isotropic energy >1044 erg which is comparable to the giant flares. 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Letters</title><description>Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0--5408, gave a burst with an estimated isotropic energy >1044 erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 X 1044 d 2 1 erg and 1.4 X 1047 d 2 1 erg, respectively, where and d 0501 is the distance to SGR 0501+4516. 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S</creator><general>IOP Publishing</general><general>Bristol : IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TV</scope><scope>C1K</scope><scope>KL.</scope><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-4551-2902</orcidid><orcidid>https://orcid.org/0000-0003-2786-1516</orcidid><orcidid>https://orcid.org/0000-0002-1890-1128</orcidid><orcidid>https://orcid.org/0000-0003-3768-9908</orcidid><orcidid>https://orcid.org/0000-0001-6487-5197</orcidid><orcidid>https://orcid.org/0000-0003-3332-2615</orcidid><orcidid>https://orcid.org/0000-0003-4344-7227</orcidid><orcidid>https://orcid.org/0000-0002-1180-4050</orcidid><orcidid>https://orcid.org/0000-0001-7469-4250</orcidid><orcidid>https://orcid.org/0000-0002-3658-7240</orcidid><orcidid>https://orcid.org/0000-0002-2321-1017</orcidid><orcidid>https://orcid.org/0000-0003-0589-9687</orcidid><orcidid>https://orcid.org/0000-0002-1840-5095</orcidid><orcidid>https://orcid.org/0000-0002-9704-6472</orcidid><orcidid>https://orcid.org/0000-0002-2002-1701</orcidid><orcidid>https://orcid.org/0000-0002-1377-1272</orcidid><orcidid>https://orcid.org/0000-0002-1019-6911</orcidid><orcidid>https://orcid.org/0000-0002-4918-0247</orcidid><orcidid>https://orcid.org/0000-0002-8859-5453</orcidid></search><sort><creationdate>20110620</creationdate><title>Search for Gravitational Wave Bursts from Six Magnetars</title><author>Abernathy, M ; Affeldt, C ; Amariutei, D ; Aston, S. M ; Barnum, S ; Bilenko, I. A ; Biswas, R ; Black, E ; Blackburn, L ; Bland, B ; Boschi, V ; Braginsky, V. B ; Bulik, T ; Bulten, H. J ; Burguet-Castell, J ; Campsie, P ; Capano, C ; Cavalier, F ; Cella, G ; Clark, J ; Colla, A ; Das, K ; Day, R ; Dent, T ; Fiore, L. Di ; Dietz, A ; Farr, B. F ; Franc, J ; Frasconi, F ; Fulda, P ; Gáspár, M. E ; Giazotto, A ; Gill, C ; Goßler, S ; Guidi, G. M ; Gustafson, E. K ; Harms, J ; Hooper, S ; Howell, E. J ; Huttner, S. H ; Katsavounidis, E ; Katzman, W ; Keppel, D. G ; Klimenko, S ; Krishnan, B ; Leaci, P ; Leroy, N ; Liguori, N ; Mandel, I ; Márka, Z ; Maros, E ; Martin, I. W ; Meadors, G ; Mehmet, M ; Meyer, M. S ; Minenkov, Y ; Moscatelli, V ; Nash, T ; Nishida, E ; Ottens, R. S ; Patel, P ; Penn, S ; Perreca, A ; Phelps, M ; Pietka, M ; Plissi, M. V ; Postiglione, F ; Quetschke, V ; Rakhmanov, M ; Rankins, B ; Robinet, F ; Rocchi, A ; Romano, R ; Romie, J. H ; Ruggi, P ; Salit, M ; de la Jordana, L. Sancho ; Santamaría, L ; Schilling, R ; Schnabel, R ; Searle, A. C ; Sengupta, A. S ; Shihan Weerathunga, T ; Shoemaker, D. H ; Singer, L ; Soto, J ; Steplewski, S ; Sung, M ; Sutton, P. J ; Tarabrin, S. P ; Taylor, R ; Toncelli, A ; Travasso, F ; Vass, S ; Willke, B ; Yamamoto, H ; Zhang, Z ; Frederiks, D. D ; Kouveliotou, C ; Tashiro, M. S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c464t-f4fedcf776dca600dd88ac4afab23e2bcf07a5fb421f33d93d39bd3306f6599b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Acoustic waves</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>COSMIC GAMMA BURSTS</topic><topic>COSMIC RADIATION</topic><topic>COSMIC RADIO SOURCES</topic><topic>EMISSION</topic><topic>Emissions</topic><topic>Galaxies</topic><topic>Gamma-radiation</topic><topic>Gamma-ray bursts</topic><topic>General Relativity and Quantum Cosmology</topic><topic>GRAVITATIONAL WAVES</topic><topic>Gravity waves</topic><topic>IONIZING RADIATIONS</topic><topic>MAGNETIC FIELDS</topic><topic>NEUTRON STARS</topic><topic>Noise pollution</topic><topic>Physics</topic><topic>PRIMARY COSMIC RADIATION</topic><topic>PULSARS</topic><topic>RADIATIONS</topic><topic>STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abernathy, M</creatorcontrib><creatorcontrib>Affeldt, C</creatorcontrib><creatorcontrib>Amariutei, D</creatorcontrib><creatorcontrib>Aston, S. M</creatorcontrib><creatorcontrib>Barnum, S</creatorcontrib><creatorcontrib>Bilenko, I. A</creatorcontrib><creatorcontrib>Biswas, R</creatorcontrib><creatorcontrib>Black, E</creatorcontrib><creatorcontrib>Blackburn, L</creatorcontrib><creatorcontrib>Bland, B</creatorcontrib><creatorcontrib>Boschi, V</creatorcontrib><creatorcontrib>Braginsky, V. B</creatorcontrib><creatorcontrib>Bulik, T</creatorcontrib><creatorcontrib>Bulten, H. J</creatorcontrib><creatorcontrib>Burguet-Castell, J</creatorcontrib><creatorcontrib>Campsie, P</creatorcontrib><creatorcontrib>Capano, C</creatorcontrib><creatorcontrib>Cavalier, F</creatorcontrib><creatorcontrib>Cella, G</creatorcontrib><creatorcontrib>Clark, J</creatorcontrib><creatorcontrib>Colla, A</creatorcontrib><creatorcontrib>Das, K</creatorcontrib><creatorcontrib>Day, R</creatorcontrib><creatorcontrib>Dent, T</creatorcontrib><creatorcontrib>Fiore, L. Di</creatorcontrib><creatorcontrib>Dietz, A</creatorcontrib><creatorcontrib>Farr, B. 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H</creatorcontrib><creatorcontrib>Singer, L</creatorcontrib><creatorcontrib>Soto, J</creatorcontrib><creatorcontrib>Steplewski, S</creatorcontrib><creatorcontrib>Sung, M</creatorcontrib><creatorcontrib>Sutton, P. J</creatorcontrib><creatorcontrib>Tarabrin, S. P</creatorcontrib><creatorcontrib>Taylor, R</creatorcontrib><creatorcontrib>Toncelli, A</creatorcontrib><creatorcontrib>Travasso, F</creatorcontrib><creatorcontrib>Vass, S</creatorcontrib><creatorcontrib>Willke, B</creatorcontrib><creatorcontrib>Yamamoto, H</creatorcontrib><creatorcontrib>Zhang, Z</creatorcontrib><creatorcontrib>Frederiks, D. D</creatorcontrib><creatorcontrib>Kouveliotou, C</creatorcontrib><creatorcontrib>Tashiro, M. S</creatorcontrib><creatorcontrib>The LIGO Scientific Collaboration and the Virgo Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Pollution Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abernathy, M</au><au>Affeldt, C</au><au>Amariutei, D</au><au>Aston, S. M</au><au>Barnum, S</au><au>Bilenko, I. A</au><au>Biswas, R</au><au>Black, E</au><au>Blackburn, L</au><au>Bland, B</au><au>Boschi, V</au><au>Braginsky, V. B</au><au>Bulik, T</au><au>Bulten, H. J</au><au>Burguet-Castell, J</au><au>Campsie, P</au><au>Capano, C</au><au>Cavalier, F</au><au>Cella, G</au><au>Clark, J</au><au>Colla, A</au><au>Das, K</au><au>Day, R</au><au>Dent, T</au><au>Fiore, L. Di</au><au>Dietz, A</au><au>Farr, B. F</au><au>Franc, J</au><au>Frasconi, F</au><au>Fulda, P</au><au>Gáspár, M. E</au><au>Giazotto, A</au><au>Gill, C</au><au>Goßler, S</au><au>Guidi, G. M</au><au>Gustafson, E. K</au><au>Harms, J</au><au>Hooper, S</au><au>Howell, E. J</au><au>Huttner, S. H</au><au>Katsavounidis, E</au><au>Katzman, W</au><au>Keppel, D. G</au><au>Klimenko, S</au><au>Krishnan, B</au><au>Leaci, P</au><au>Leroy, N</au><au>Liguori, N</au><au>Mandel, I</au><au>Márka, Z</au><au>Maros, E</au><au>Martin, I. W</au><au>Meadors, G</au><au>Mehmet, M</au><au>Meyer, M. S</au><au>Minenkov, Y</au><au>Moscatelli, V</au><au>Nash, T</au><au>Nishida, E</au><au>Ottens, R. S</au><au>Patel, P</au><au>Penn, S</au><au>Perreca, A</au><au>Phelps, M</au><au>Pietka, M</au><au>Plissi, M. V</au><au>Postiglione, F</au><au>Quetschke, V</au><au>Rakhmanov, M</au><au>Rankins, B</au><au>Robinet, F</au><au>Rocchi, A</au><au>Romano, R</au><au>Romie, J. H</au><au>Ruggi, P</au><au>Salit, M</au><au>de la Jordana, L. Sancho</au><au>Santamaría, L</au><au>Schilling, R</au><au>Schnabel, R</au><au>Searle, A. C</au><au>Sengupta, A. S</au><au>Shihan Weerathunga, T</au><au>Shoemaker, D. H</au><au>Singer, L</au><au>Soto, J</au><au>Steplewski, S</au><au>Sung, M</au><au>Sutton, P. J</au><au>Tarabrin, S. P</au><au>Taylor, R</au><au>Toncelli, A</au><au>Travasso, F</au><au>Vass, S</au><au>Willke, B</au><au>Yamamoto, H</au><au>Zhang, Z</au><au>Frederiks, D. D</au><au>Kouveliotou, C</au><au>Tashiro, M. S</au><aucorp>The LIGO Scientific Collaboration and the Virgo Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for Gravitational Wave Bursts from Six Magnetars</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2011-06-20</date><risdate>2011</risdate><volume>734</volume><issue>2</issue><spage>L35</spage><epage>jQuery1323917158755='48'</epage><pages>L35-jQuery1323917158755='48'</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0--5408, gave a burst with an estimated isotropic energy >1044 erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 X 1044 d 2 1 erg and 1.4 X 1047 d 2 1 erg, respectively, where and d 0501 is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time.</abstract><cop>United States</cop><pub>IOP Publishing</pub><doi>10.1088/2041-8205/734/2/L35</doi><orcidid>https://orcid.org/0000-0002-4551-2902</orcidid><orcidid>https://orcid.org/0000-0003-2786-1516</orcidid><orcidid>https://orcid.org/0000-0002-1890-1128</orcidid><orcidid>https://orcid.org/0000-0003-3768-9908</orcidid><orcidid>https://orcid.org/0000-0001-6487-5197</orcidid><orcidid>https://orcid.org/0000-0003-3332-2615</orcidid><orcidid>https://orcid.org/0000-0003-4344-7227</orcidid><orcidid>https://orcid.org/0000-0002-1180-4050</orcidid><orcidid>https://orcid.org/0000-0001-7469-4250</orcidid><orcidid>https://orcid.org/0000-0002-3658-7240</orcidid><orcidid>https://orcid.org/0000-0002-2321-1017</orcidid><orcidid>https://orcid.org/0000-0003-0589-9687</orcidid><orcidid>https://orcid.org/0000-0002-1840-5095</orcidid><orcidid>https://orcid.org/0000-0002-9704-6472</orcidid><orcidid>https://orcid.org/0000-0002-2002-1701</orcidid><orcidid>https://orcid.org/0000-0002-1377-1272</orcidid><orcidid>https://orcid.org/0000-0002-1019-6911</orcidid><orcidid>https://orcid.org/0000-0002-4918-0247</orcidid><orcidid>https://orcid.org/0000-0002-8859-5453</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2041-8205 |
ispartof | Astrophysical journal. Letters, 2011-06, Vol.734 (2), p.L35-jQuery1323917158755='48' |
issn | 2041-8205 2041-8213 |
language | eng |
recordid | cdi_hal_primary_oai_HAL_in2p3_00608259v1 |
source | Free E-Journal (出版社公開部分のみ) |
subjects | Acoustic waves ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC GAMMA BURSTS COSMIC RADIATION COSMIC RADIO SOURCES EMISSION Emissions Galaxies Gamma-radiation Gamma-ray bursts General Relativity and Quantum Cosmology GRAVITATIONAL WAVES Gravity waves IONIZING RADIATIONS MAGNETIC FIELDS NEUTRON STARS Noise pollution Physics PRIMARY COSMIC RADIATION PULSARS RADIATIONS STARS |
title | Search for Gravitational Wave Bursts from Six Magnetars |
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