SEARCHES FOR TIME-DEPENDENT NEUTRINO SOURCES WITH ICECUBE DATA FROM 2008 TO 2012
SEARCHES FOR TIME-DEPENDENT NEUTRINO SOURCES WITH ICECUBE DATA FROM 2008 TO 2012
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DOI：
10.1088/0004-637x/807/1/46
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发表时间：
2015-03
期刊：
影响因子：
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通讯作者：
M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;T. Anderson;C. Arguelles;T. Arlen;J. Auffenberg;X. Bai;M. Baker;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;P. Berghaus;D. Berley;E. Bernardini;A. Bernhard;D. Besson;G. Binder;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;F. Bos;D. Bose;S. Boser;O. Botner;L. Brayeur;H. Bretz;A. Brown;N. Buzinsky;J. Casey;M. Casier;E. Cheung;D. Chirkin;A. Christov;B. Christy;K. Clark;L. Classen;F. Clevermann;S. Coenders;D. Cowen;A. H. C. Silva;J. Daughhetee;J. Davis;M. Day;J. Andr'e;C. Clercq;H. Dembinski;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;J. C. D'iaz-V'elez;J. Dumm;M. Dunkman;R. Eagan;B. Eberhardt;T. Ehrhardt;B. Eichmann;J. Eisch;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;J. Felde;K. Filimonov;C. Finley;T. Fischer-Wasels;S. Flis;K. Frantzen;T. Fuchs;T. Gaisser;R. Gaior;J. Gallagher;L. Gerhardt;D. Gier;L. Gladstone;T. Glusenkamp;A. Goldschmidt;G. Golup;J. G. Gonzalez;J. Goodman;D. G'ora;D. Grant;P. Gretskov;J. Groh;A. Gross;C. Ha;C. Haack;A. H. Ismail;P. Hallen;A. Hallgren;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;D. Heinen;K. Helbing;R. Hellauer;D. Hellwig;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;A. Homeier;K. Hoshina;F. Huang;W. Huelsnitz;P. O. Hulth;K. Hultqvist;S. In;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;K. Jero;M. Jurkovič;B. Kaminsky;A. Kappes;T. Karg;A. Karle;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kiryluk;J. Klas;S. Klein;J. Kohne;G. Kohnen;H. Kolanoski;A. Koob;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;A. Kriesten;K. Krings;G. Kroll;M. Kroll;J. Kunnen;N. Kurahashi;T. Kuwabara;M. Labare;J. Lanfranchi;D. T. Larsen;M. Larson;M. Lesiak-Bzdak;M. Leuermann;J. Lunemann;J. Madsen;G. Maggi;K. Mahn;R. Maruyama;K. Mase;H. Matis;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Meli;T. Meures;S. Miarecki;E. Middell;E. Middlemas;N. Milke;J. Miller;L. Mohrmann;T. Montaruli;R. Morse;R. Nahnhauer;U. Naumann;H. Niederhausen;S. Nowicki;D. Nygren;A. Obertacke;A. Olivas;A. Omairat;A. O'Murchadha;T. Palczewski;L. Paul;O. Penek;J. Pepper;C. Heros;C. Pfendner;D. Pieloth;E. Pinat;J. Posselt;P. Price;G. Przybylski;J. Putz;M. Quinnan;L. Radel;M. Rameez;K. Rawlins;P. Redl;I. Rees;R. Reimann;M. Relich;E. Resconi;W. Rhode;M. Richman;B. Riedel;S. Robertson;J. Rodrigues;M. Rongen;C. Rott;T. Ruhe;B. Ruzybayev;D. Ryckbosch;S. M. Saba;H. Sander;J. Sandroos;M. Santander;S. Sarkar;K. Schatto;F. Scheriau;T. Schmidt;M. Schmitz;S. Schoenen;S. Schoneberg;A. Schonwald;A. Schukraft;L. Schulte;O. Schulz;D. Seckel;Y. Sestayo;S. Seunarine;R. Shanidze;M. Smith;D. Soldin;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;N. Stanisha;Alexander Stasik;T. Stezelberger;R. Stokstad;A. Stossl;E. Strahler;R. Strom;N. Strotjohann;G. Sullivan;M. Sutherland;H. Taavola;I. Taboada;A. Tamburro;S. Ter-Antonyan;A. Terliuk;G. Tevsi'c;S. Tilav;P. Toale;M. Tobin;D. Tosi;M. Tselengidou;E. Unger;M. Usner;S. Vallecorsa;N. Eijndhoven;J. Vandenbroucke;J. Santen;S. Vanheule;M. Vehring;M. Voge;M. Vraeghe;C. Walck;M. Wallraff;C. Weaver;M. Wellons;C. Wendt;S. Westerhoff;B. Whelan;N. Whitehorn;C. Wichary;K. Wiebe;C. Wiebusch;D. Williams;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;J. Ziemann;M. Zoll
中科院分区：
文献类型：
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作者：
M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;T. Anderson;C. Arguelles;T. Arlen;J. Auffenberg;X. Bai;M. Baker;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;P. Berghaus;D. Berley;E. Bernardini;A. Bernhard;D. Besson;G. Binder;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;F. Bos;D. Bose;S. Boser;O. Botner;L. Brayeur;H. Bretz;A. Brown;N. Buzinsky;J. Casey;M. Casier;E. Cheung;D. Chirkin;A. Christov;B. Christy;K. Clark;L. Classen;F. Clevermann;S. Coenders;D. Cowen;A. H. C. Silva;J. Daughhetee;J. Davis;M. Day;J. Andr'e;C. Clercq;H. Dembinski;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;J. C. D'iaz-V'elez;J. Dumm;M. Dunkman;R. Eagan;B. Eberhardt;T. Ehrhardt;B. Eichmann;J. Eisch;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;J. Felde;K. Filimonov;C. Finley;T. Fischer-Wasels;S. Flis;K. Frantzen;T. Fuchs;T. Gaisser;R. Gaior;J. Gallagher;L. Gerhardt;D. Gier;L. Gladstone;T. Glusenkamp;A. Goldschmidt;G. Golup;J. G. Gonzalez;J. Goodman;D. G'ora;D. Grant;P. Gretskov;J. Groh;A. Gross;C. Ha;C. Haack;A. H. Ismail;P. Hallen;A. Hallgren;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;D. Heinen;K. Helbing;R. Hellauer;D. Hellwig;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;A. Homeier;K. Hoshina;F. Huang;W. Huelsnitz;P. O. Hulth;K. Hultqvist;S. In;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;K. Jero;M. Jurkovič;B. Kaminsky;A. Kappes;T. Karg;A. Karle;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kiryluk;J. Klas;S. Klein;J. Kohne;G. Kohnen;H. Kolanoski;A. Koob;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;A. Kriesten;K. Krings;G. Kroll;M. Kroll;J. Kunnen;N. Kurahashi;T. Kuwabara;M. Labare;J. Lanfranchi;D. T. Larsen;M. Larson;M. Lesiak-Bzdak;M. Leuermann;J. Lunemann;J. Madsen;G. Maggi;K. Mahn;R. Maruyama;K. Mase;H. Matis;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Meli;T. Meures;S. Miarecki;E. Middell;E. Middlemas;N. Milke;J. Miller;L. Mohrmann;T. Montaruli;R. Morse;R. Nahnhauer;U. Naumann;H. Niederhausen;S. Nowicki;D. Nygren;A. Obertacke;A. Olivas;A. Omairat;A. O'Murchadha;T. Palczewski;L. Paul;O. Penek;J. Pepper;C. Heros;C. Pfendner;D. Pieloth;E. Pinat;J. Posselt;P. Price;G. Przybylski;J. Putz;M. Quinnan;L. Radel;M. Rameez;K. Rawlins;P. Redl;I. Rees;R. Reimann;M. Relich;E. Resconi;W. Rhode;M. Richman;B. Riedel;S. Robertson;J. Rodrigues;M. Rongen;C. Rott;T. Ruhe;B. Ruzybayev;D. Ryckbosch;S. M. Saba;H. Sander;J. Sandroos;M. Santander;S. Sarkar;K. Schatto;F. Scheriau;T. Schmidt;M. Schmitz;S. Schoenen;S. Schoneberg;A. Schonwald;A. Schukraft;L. Schulte;O. Schulz;D. Seckel;Y. Sestayo;S. Seunarine;R. Shanidze;M. Smith;D. Soldin;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;N. Stanisha;Alexander Stasik;T. Stezelberger;R. Stokstad;A. Stossl;E. Strahler;R. Strom;N. Strotjohann;G. Sullivan;M. Sutherland;H. Taavola;I. Taboada;A. Tamburro;S. Ter-Antonyan;A. Terliuk;G. Tevsi'c;S. Tilav;P. Toale;M. Tobin;D. Tosi;M. Tselengidou;E. Unger;M. Usner;S. Vallecorsa;N. Eijndhoven;J. Vandenbroucke;J. Santen;S. Vanheule;M. Vehring;M. Voge;M. Vraeghe;C. Walck;M. Wallraff;C. Weaver;M. Wellons;C. Wendt;S. Westerhoff;B. Whelan;N. Whitehorn;C. Wichary;K. Wiebe;C. Wiebusch;D. Williams;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;J. Ziemann;M. Zoll
本文介绍了用冰立方中微子望远镜寻找耀斑中微子源和周期性发射源的情况。与时间积分搜索相比，假设稳定发射，这里提出的分析寻找一个依赖于时间的中微子信号，使用中微子到达时间的信息，以提高发现的潜力。研究人员搜索了中微子到达时间和方向之间的相关性，以及随时间变化的光变曲线、零星发射或候选源的周期性之后的中微子发射。这些包括活动星系核、软γ射线中继器、超新星遗迹、微类星体和X射线双星。这里介绍的工作更新并扩展了以前发表的结果，涵盖了从2008年4月5日到2012年5月16日的4年数据，包括完成的86弦探测器运行的第一年。分析没有发现任何显著的随时间变化的中微子点源，结果被用来设定候选源中微子通量的上限。
In this paper searches for flaring astrophysical neutrino sources and sources with periodic emission with the IceCube neutrino telescope are presented. In contrast to time-integrated searches, where steady emission is assumed, the analyses presented here look for a time-dependent signal of neutrinos using the information from the neutrino arrival times to enhance the discovery potential. A search was performed for correlations between neutrino arrival times and directions, as well as neutrino emission following time-dependent light curves, sporadic emission, or periodicities of candidate sources. These include active galactic nuclei, soft γ-ray repeaters, supernova remnants hosting pulsars, microquasars, and X-ray binaries. The work presented here updates and extends previously published results to a longer period that covers 4 years of data from 2008 April 5 to 2012 May 16, including the first year of operation of the completed 86 string detector. The analyses did not find any significant time-dependent point sources of neutrinos, and the results were used to set upper limits on the neutrino flux from source candidates.