Searching for neutrino bursts in the galaxy: 36 years of exposure
Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Ov...
Ausführliche Beschreibung
Autor*in: |
Novoseltsev, Yu. F. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2017 |
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Anmerkung: |
© Pleiades Publishing, Inc. 2017 |
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Übergeordnetes Werk: |
Enthalten in: Journal of experimental and theoretical physics - Pleiades Publishing, 1993, 125(2017), 1 vom: Juli, Seite 73-79 |
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Übergeordnetes Werk: |
volume:125 ; year:2017 ; number:1 ; month:07 ; pages:73-79 |
Links: |
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DOI / URN: |
10.1134/S1063776117070226 |
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Katalog-ID: |
OLC2043176854 |
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10.1134/S1063776117070226 doi (DE-627)OLC2043176854 (DE-He213)S1063776117070226-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Novoseltsev, Yu. F. verfasserin aut Searching for neutrino bursts in the galaxy: 36 years of exposure 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2017 Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. Boliev, M. M. aut Volchenko, V. I. aut Volchenko, G. V. aut Dzaparova, I. M. aut Kochkarov, M. M. aut Novoseltseva, R. V. aut Petkov, V. B. aut Yanin, A. F. aut Enthalten in Journal of experimental and theoretical physics Pleiades Publishing, 1993 125(2017), 1 vom: Juli, Seite 73-79 (DE-627)131188410 (DE-600)1146369-7 (DE-576)032622368 1063-7761 nnns volume:125 year:2017 number:1 month:07 pages:73-79 https://doi.org/10.1134/S1063776117070226 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 33.00 VZ AR 125 2017 1 07 73-79 |
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10.1134/S1063776117070226 doi (DE-627)OLC2043176854 (DE-He213)S1063776117070226-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Novoseltsev, Yu. F. verfasserin aut Searching for neutrino bursts in the galaxy: 36 years of exposure 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2017 Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. Boliev, M. M. aut Volchenko, V. I. aut Volchenko, G. V. aut Dzaparova, I. M. aut Kochkarov, M. M. aut Novoseltseva, R. V. aut Petkov, V. B. aut Yanin, A. F. aut Enthalten in Journal of experimental and theoretical physics Pleiades Publishing, 1993 125(2017), 1 vom: Juli, Seite 73-79 (DE-627)131188410 (DE-600)1146369-7 (DE-576)032622368 1063-7761 nnns volume:125 year:2017 number:1 month:07 pages:73-79 https://doi.org/10.1134/S1063776117070226 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 33.00 VZ AR 125 2017 1 07 73-79 |
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10.1134/S1063776117070226 doi (DE-627)OLC2043176854 (DE-He213)S1063776117070226-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Novoseltsev, Yu. F. verfasserin aut Searching for neutrino bursts in the galaxy: 36 years of exposure 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2017 Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. Boliev, M. M. aut Volchenko, V. I. aut Volchenko, G. V. aut Dzaparova, I. M. aut Kochkarov, M. M. aut Novoseltseva, R. V. aut Petkov, V. B. aut Yanin, A. F. aut Enthalten in Journal of experimental and theoretical physics Pleiades Publishing, 1993 125(2017), 1 vom: Juli, Seite 73-79 (DE-627)131188410 (DE-600)1146369-7 (DE-576)032622368 1063-7761 nnns volume:125 year:2017 number:1 month:07 pages:73-79 https://doi.org/10.1134/S1063776117070226 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 33.00 VZ AR 125 2017 1 07 73-79 |
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10.1134/S1063776117070226 doi (DE-627)OLC2043176854 (DE-He213)S1063776117070226-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Novoseltsev, Yu. F. verfasserin aut Searching for neutrino bursts in the galaxy: 36 years of exposure 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2017 Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. Boliev, M. M. aut Volchenko, V. I. aut Volchenko, G. V. aut Dzaparova, I. M. aut Kochkarov, M. M. aut Novoseltseva, R. V. aut Petkov, V. B. aut Yanin, A. F. aut Enthalten in Journal of experimental and theoretical physics Pleiades Publishing, 1993 125(2017), 1 vom: Juli, Seite 73-79 (DE-627)131188410 (DE-600)1146369-7 (DE-576)032622368 1063-7761 nnns volume:125 year:2017 number:1 month:07 pages:73-79 https://doi.org/10.1134/S1063776117070226 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 33.00 VZ AR 125 2017 1 07 73-79 |
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10.1134/S1063776117070226 doi (DE-627)OLC2043176854 (DE-He213)S1063776117070226-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Novoseltsev, Yu. F. verfasserin aut Searching for neutrino bursts in the galaxy: 36 years of exposure 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Inc. 2017 Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. Boliev, M. M. aut Volchenko, V. I. aut Volchenko, G. V. aut Dzaparova, I. M. aut Kochkarov, M. M. aut Novoseltseva, R. V. aut Petkov, V. B. aut Yanin, A. F. aut Enthalten in Journal of experimental and theoretical physics Pleiades Publishing, 1993 125(2017), 1 vom: Juli, Seite 73-79 (DE-627)131188410 (DE-600)1146369-7 (DE-576)032622368 1063-7761 nnns volume:125 year:2017 number:1 month:07 pages:73-79 https://doi.org/10.1134/S1063776117070226 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 33.00 VZ AR 125 2017 1 07 73-79 |
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Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. © Pleiades Publishing, Inc. 2017 |
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Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. © Pleiades Publishing, Inc. 2017 |
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Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level. © Pleiades Publishing, Inc. 2017 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2043176854</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504104145.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2017 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/S1063776117070226</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2043176854</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)S1063776117070226-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">33.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Novoseltsev, Yu. F.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Searching for neutrino bursts in the galaxy: 36 years of exposure</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2017</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Inc. 2017</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The Baksan Underground Scintillation Telescope has operated within the program of searching for neutrino bursts since the mid-1980s. We present the current status of the experiment and some results related to the investigation of background events and the stability of facility operation. Over the period from June 30, 1980, to December 31, 2016, the pure observation time was 31.27 years. No neutrino burst candidate event from the explosion of a core-collapse supernova in the Galaxy was recorded in this time. This sets an upper bound of 0.074 $ yr^{–1} $ on the mean frequency of gravitational stellar collapses in the Galaxy at a 90% confidence level.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Boliev, M. M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Volchenko, V. I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Volchenko, G. 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