SEARCHES FOR PERIODIC NEUTRINO EMISSION FROM BINARY SYSTEMS WITH 22 AND 40 STRINGS OF ICECUBE

SEARCHES FOR PERIODIC NEUTRINO EMISSION FROM BINARY SYSTEMS WITH 22 AND 40 STRINGS OF ICECUBE
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DOI:
10.1088/0004-637x/748/2/118
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发表时间:
2011-08
期刊:
The Astrophysical Journal
影响因子:
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通讯作者:
R. Abbasi;Y. Abdou;T. Abu-Zayyad;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Allen;D. Altmann;K. Andeen;K. Andeen;J. Auffenberg;X. Bai;X. Bai;M. Baker;S. Barwick;R. Bay;J. Alba;K. Beattie;J. Beatty;S. Bechet;J. K. Becker;K. Becker;M. Benabderrahmane;S. BenZvi;J. Berdermann;P. Berghaus;D. Berley;E. Bernardini;D. Bertrand;D. Besson;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;D. Bose;S. Böser;O. Botner;A. Brown;S. Buitink;K. Caballero-Mora;M. Carson;D. Chirkin;B. Christy;F. Clevermann;S. Cohen;C. Colnard;D. Cowen;A. H. C. Silva;M. D'Agostino;M. Danninger;J. Daughhetee;J. Davis;C. Clercq;T. Degner;L. Demirörs;F. Descamps;P. Desiati;G. Vries-Uiterweerd;T. DeYoung;J. C. D'iaz-V'elez;M. Dierckxsens;J. Dreyer;J. Dumm;M. Dunkman;J. Eisch;R. Ellsworth;O. Engdegård;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;T. Feusels;K. Filimonov;C. Finley;T. Fischer-Wasels;B. Fox;A. Franckowiak;R. Franke;T. Gaisser;J. Gallagher;L. Gerhardt;L. Gerhardt;L. Gladstone;T. Gluesenkamp;A. Goldschmidt;J. Goodman;D. G'ora;D. Grant;T. Griesel;A. Gross;A. Gross;S. Grullon;M. Gurtner;C. Ha;A. H. Ismail;A. Hallgren;F. Halzen;K. Han;K. Hanson;K. Hanson;D. Heinen;K. Helbing;R. Hellauer;S. Hickford;G. Hill;K. Hoffman;B. Hoffmann;A. Homeier;K. Hoshina;W. Huelsnitz;W. Huelsnitz;J. P. Huelss;P. O. Hulth;K. Hultqvist;S. Hussain;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;H. Johansson;K. Kampert;A. Kappes;T. Karg;A. Karle;P. Kenny;J. Kiryluk;J. Kiryluk;F. Kislat;S. Klein;S. Klein;J. Koehne;G. Kohnen;H. Kolanoski;L. Köpke;S. Kopper;D. Koskinen;M. Kowalski;T. Kowarik;M. Krasberg;G. Kroll;N. Kurahashi;T. Kuwabara;M. Labare;K. Laihem;H. Landsman;M. Larson;R. Lauer;J. Lünemann;J. Madsen;A. Marotta;R. Maruyama;K. Mase;H. Matis;K. Meagher;M. Merck;P. Mészáros;T. Meures;S. Miarecki;S. Miarecki;E. Middell;N. Milke;J. Miller;T. Montaruli;R. Morse;S. Movit;R. Nahnhauer;J. Nam;U. Naumann;D. Nygren;S. Odrowski;A. Olivas;M. Olivo;A. O'Murchadha;S. Panknin;L. Paul;C. Heros;J. Petrovic;A. Piegsa;D. Pieloth;R. Porrata;J. Posselt;P. Price;G. Przybylski;K. Rawlins;P. Redl;E. Resconi;W. Rhode;M. Ribordy;M. Richman;J. Rodrigues;F. Rothmaier;C. Rott;T. Ruhe;D. Rutledge;B. Ruzybayev;D. Ryckbosch;H. Sander;M. Santander;S. Sarkar;K. Schatto;T. Schmidt;A. Schönwald;A. Schukraft;A. Schultes;O. Schulz;M. Schunck;D. Seckel;B. Semburg;S. Seo;Y. Sestayo;S. Seunarine;A. Silvestri;G. Spiczak;C. Spiering;M. Stamatikos;M. Stamatikos;T. Stanev;T. Stezelberger;R. Stokstad;A. Stößl;E. Strahler;R. Strom;M. Stüer;G. Sullivan;Q. Swillens;H. Taavola;I. Taboada;A. Tamburro;A. Tepe;S. Ter-Antonyan;S. Tilav;P. Toale;S. Toscano;D. Tosi;N. Eijndhoven;J. Vandenbroucke;A. Overloop;J. Santen;M. Vehring;M. Voge;C. Walck;T. Waldenmaier;M. Wallraff;M. Walter;C. Weaver;C. Wendt;S. Westerhoff;N. Whitehorn;K. Wiebe;C. Wiebusch;D. Williams;R. Wischnewski;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;C. Xu;D. Xu;X. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;M. Zoll
R. Abbasi;Y. Abdou;T. Abu-Zayyad;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Allen;D. Altmann;K. Andeen;K. Andeen;J. Auffenberg;X. Bai;X. Bai;M. Baker;S. Barwick;R. Bay;J. Alba;K. Beattie;J. Beatty;S. Bechet;J. K. Becker;K. Becker;M. Benabderrahmane;S. BenZvi;J. Berdermann;P. Berghaus;D. Berley;E. Bernardini;D. Bertrand;D. Besson;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;D. Bose;S. Böser;O. Botner;A. Brown;S. Buitink;K. Caballero-Mora;M. Carson;D. Chirkin;B. Christy;F. Clevermann;S. Cohen;C. Colnard;D. Cowen;A. H. C. Silva;M. D'Agostino;M. Danninger;J. Daughhetee;J. Davis;C. Clercq;T. Degner;L. Demirörs;F. Descamps;P. Desiati;G. Vries-Uiterweerd;T. DeYoung;J. C. D'iaz-V'elez;M. Dierckxsens;J. Dreyer;J. Dumm;M. Dunkman;J. Eisch;R. Ellsworth;O. Engdegård;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;T. Feusels;K. Filimonov;C. Finley;T. Fischer-Wasels;B. Fox;A. Franckowiak;R. Franke;T. Gaisser;J. Gallagher;L. Gerhardt;L. Gerhardt;L. Gladstone;T. Gluesenkamp;A. Goldschmidt;J. Goodman;D. G'ora;D. Grant;T. Griesel;A. Gross;A. Gross;S. Grullon;M. Gurtner;C. Ha;A. H. Ismail;A. Hallgren;F. Halzen;K. Han;K. Hanson;K. Hanson;D. Heinen;K. Helbing;R. Hellauer;S. Hickford;G. Hill;K. Hoffman;B. Hoffmann;A. Homeier;K. Hoshina;W. Huelsnitz;W. Huelsnitz;J. P. Huelss;P. O. Hulth;K. Hultqvist;S. Hussain;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;H. Johansson;K. Kampert;A. Kappes;T. Karg;A. Karle;P. Kenny;J. Kiryluk;J. Kiryluk;F. Kislat;S. Klein;S. Klein;J. Koehne;G. Kohnen;H. Kolanoski;L. Köpke;S. Kopper;D. Koskinen;M. Kowalski;T. Kowarik;M. Krasberg;G. Kroll;N. Kurahashi;T. Kuwabara;M. Labare;K. Laihem;H. Landsman;M. Larson;R. Lauer;J. Lünemann;J. Madsen;A. Marotta;R. Maruyama;K. Mase;H. Matis;K. Meagher;M. Merck;P. Mészáros;T. Meures;S. Miarecki;S. Miarecki;E. Middell;N. Milke;J. Miller;T. Montaruli;R. Morse;S. Movit;R. Nahnhauer;J. Nam;U. Naumann;D. Nygren;S. Odrowski;A. Olivas;M. Olivo;A. O'Murchadha;S. Panknin;L. Paul;C. Heros;J. Petrovic;A. Piegsa;D. Pieloth;R. Porrata;J. Posselt;P. Price;G. Przybylski;K. Rawlins;P. Redl;E. Resconi;W. Rhode;M. Ribordy;M. Richman;J. Rodrigues;F. Rothmaier;C. Rott;T. Ruhe;D. Rutledge;B. Ruzybayev;D. Ryckbosch;H. Sander;M. Santander;S. Sarkar;K. Schatto;T. Schmidt;A. Schönwald;A. Schukraft;A. Schultes;O. Schulz;M. Schunck;D. Seckel;B. Semburg;S. Seo;Y. Sestayo;S. Seunarine;A. Silvestri;G. Spiczak;C. Spiering;M. Stamatikos;M. Stamatikos;T. Stanev;T. Stezelberger;R. Stokstad;A. Stößl;E. Strahler;R. Strom;M. Stüer;G. Sullivan;Q. Swillens;H. Taavola;I. Taboada;A. Tamburro;A. Tepe;S. Ter-Antonyan;S. Tilav;P. Toale;S. Toscano;D. Tosi;N. Eijndhoven;J. Vandenbroucke;A. Overloop;J. Santen;M. Vehring;M. Voge;C. Walck;T. Waldenmaier;M. Wallraff;M. Walter;C. Weaver;C. Wendt;S. Westerhoff;N. Whitehorn;K. Wiebe;C. Wiebusch;D. Williams;R. Wischnewski;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;C. Xu;D. Xu;X. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;M. Zoll
中科院分区:
其他
文献类型:
--
作者:
R. Abbasi;Y. Abdou;T. Abu-Zayyad;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Allen;D. Altmann;K. Andeen;K. Andeen;J. Auffenberg;X. Bai;X. Bai;M. Baker;S. Barwick;R. Bay;J. Alba;K. Beattie;J. Beatty;S. Bechet;J. K. Becker;K. Becker;M. Benabderrahmane;S. BenZvi;J. Berdermann;P. Berghaus;D. Berley;E. Bernardini;D. Bertrand;D. Besson;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;D. Bose;S. Böser;O. Botner;A. Brown;S. Buitink;K. Caballero-Mora;M. Carson;D. Chirkin;B. Christy;F. Clevermann;S. Cohen;C. Colnard;D. Cowen;A. H. C. Silva;M. D'Agostino;M. Danninger;J. Daughhetee;J. Davis;C. Clercq;T. Degner;L. Demirörs;F. Descamps;P. Desiati;G. Vries-Uiterweerd;T. DeYoung;J. C. D'iaz-V'elez;M. Dierckxsens;J. Dreyer;J. Dumm;M. Dunkman;J. Eisch;R. Ellsworth;O. Engdegård;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;T. Feusels;K. Filimonov;C. Finley;T. Fischer-Wasels;B. Fox;A. Franckowiak;R. Franke;T. Gaisser;J. Gallagher;L. Gerhardt;L. Gerhardt;L. Gladstone;T. Gluesenkamp;A. Goldschmidt;J. Goodman;D. G'ora;D. Grant;T. Griesel;A. Gross;A. Gross;S. Grullon;M. Gurtner;C. Ha;A. H. Ismail;A. Hallgren;F. Halzen;K. Han;K. Hanson;K. Hanson;D. Heinen;K. Helbing;R. Hellauer;S. Hickford;G. Hill;K. Hoffman;B. Hoffmann;A. Homeier;K. Hoshina;W. Huelsnitz;W. Huelsnitz;J. P. Huelss;P. O. Hulth;K. Hultqvist;S. Hussain;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;H. Johansson;K. Kampert;A. Kappes;T. Karg;A. Karle;P. Kenny;J. Kiryluk;J. Kiryluk;F. Kislat;S. Klein;S. Klein;J. Koehne;G. Kohnen;H. Kolanoski;L. Köpke;S. Kopper;D. Koskinen;M. Kowalski;T. Kowarik;M. Krasberg;G. Kroll;N. Kurahashi;T. Kuwabara;M. Labare;K. Laihem;H. Landsman;M. Larson;R. Lauer;J. Lünemann;J. Madsen;A. Marotta;R. Maruyama;K. Mase;H. Matis;K. Meagher;M. Merck;P. Mészáros;T. Meures;S. Miarecki;S. Miarecki;E. Middell;N. Milke;J. Miller;T. Montaruli;R. Morse;S. Movit;R. Nahnhauer;J. Nam;U. Naumann;D. Nygren;S. Odrowski;A. Olivas;M. Olivo;A. O'Murchadha;S. Panknin;L. Paul;C. Heros;J. Petrovic;A. Piegsa;D. Pieloth;R. Porrata;J. Posselt;P. Price;G. Przybylski;K. Rawlins;P. Redl;E. Resconi;W. Rhode;M. Ribordy;M. Richman;J. Rodrigues;F. Rothmaier;C. Rott;T. Ruhe;D. Rutledge;B. Ruzybayev;D. Ryckbosch;H. Sander;M. Santander;S. Sarkar;K. Schatto;T. Schmidt;A. Schönwald;A. Schukraft;A. Schultes;O. Schulz;M. Schunck;D. Seckel;B. Semburg;S. Seo;Y. Sestayo;S. Seunarine;A. Silvestri;G. Spiczak;C. Spiering;M. Stamatikos;M. Stamatikos;T. Stanev;T. Stezelberger;R. Stokstad;A. Stößl;E. Strahler;R. Strom;M. Stüer;G. Sullivan;Q. Swillens;H. Taavola;I. Taboada;A. Tamburro;A. Tepe;S. Ter-Antonyan;S. Tilav;P. Toale;S. Toscano;D. Tosi;N. Eijndhoven;J. Vandenbroucke;A. Overloop;J. Santen;M. Vehring;M. Voge;C. Walck;T. Waldenmaier;M. Wallraff;M. Walter;C. Weaver;C. Wendt;S. Westerhoff;N. Whitehorn;K. Wiebe;C. Wiebusch;D. Williams;R. Wischnewski;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;C. Xu;D. Xu;X. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;M. Zoll

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在本文中,我们展示了从双星系统目录中搜索周期性中微子发射的结果。在光子通量中观察到的这种调制是由这些系统的几何形状引起的。在分析中,周期由这些光子观测固定,而中微子发射的相位和持续时间被视为自由参数以与数据拟合。如果发射发生在总周期的 ∼20% 或更少的时间内,则该分析比时间积分分析具有更好的灵敏度。我们使用2007年5月31日至2008年4月5日的22串配置以及2008年4月5日至2009年5月20日的40串配置的IceCube数据。没有发现中微子发射的证据,在考虑试验后,天鹅座 X-3 出现了最强的中微子发射,显着性为 2.1σ。提供了周期性和时间积分发射的中微子通量上限。
In this paper, we present the results of searches for periodic neutrino emission from a catalog of binary systems. Such modulation, observed in the photon flux, would be caused by the geometry of these systems. In the analysis, the period is fixed by these photon observations, while the phase and duration of the neutrino emission are treated as free parameters to be fit with the data. If the emission occurs during ∼20% or less of the total period, this analysis achieves better sensitivity than a time-integrated analysis. We use the IceCube data taken from 2007 May 31 to 2008 April 5 with its 22 string configuration and from 2008 April 5 to 2009 May 20 with its 40 string configuration. No evidence for neutrino emission is found, with the strongest excess occurring for Cygnus X-3 at 2.1σ significance after accounting for trials. Neutrino flux upper limits for both periodic and time-integrated emission are provided.