Optical and X-ray early follow-up of ANTARES neutrino alerts
Optical and X-ray early follow-up of ANTARES neutrino alerts
复制标题
ANTARES 中微子警报的光学和 X 射线早期跟踪
DOI：
10.1088/1475-7516/2016/02/062
复制
发表时间：
2015
影响因子：
6.4
通讯作者：
D. Coward
中科院分区：
文献类型：
--
作者：
S. Adrián;M. Ageron;A. Albert;I. A. Samarai;M. André;G. Anton;M. Ardid;J. Aubert;B. Baret;J. Barrios;S. Basa;V. Bertin;S. Biagi;C. Bogazzi;R. Bormuth;M. Bou;M. Bouwhuis;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;J. Carr;T. Chiarusi;M. Circella;R. Coniglione;H. Costantini;P. Coyle;A. Creusot;I. Dekeyser;A. Deschamps;G. Bonis;C. Distefano;C. Donzaud;C. Donzaud;D. Dornic;D. Drouhin;A. Dumas;T. Eberl;D. Elsässer;A. Enzenhöfer;K. Fehn;I. Felis;P. Fermani;F. Folger;L. Fusco;S. Galata;S. Geißelsöder;K. Geyer;V. Giordano;A. Gleixner;R. Gracia;K. Graf;H. Haren;A. Heijboer;Y. Hello;J. Hernández;A. Herrero;J. Hössl;J. Hofestädt;C. Hugon;C. James;M. Jong;M. Kadler;O. Kalekin;U. Katz;D. Kiessling;P. Kooijman;P. Kooijman;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;G. Lambard;D. Lattuada;D. Lefèvre;E. Leonora;S. Loucatos;S. Mangano;M. Marcelin;A. Margiotta;J. Martínez;S. Martini;A. Mathieu;T. Michael;P. Migliozzi;A. Moussa;Cornelia Mueller;M. Neff;E. Nezri;G. Pǎvǎlaş;C. Pellegrino;C. Perrina;P. Piattelli;V. Popa;T. Pradier;C. Racca;G. Riccobene;R. Richter;K. Roensch;A. Rostovtsev;M. Saldaña;D. Samtleben;M. Sanguineti;P. Sapienza;J. Schmid;J. Schnabel;S. Schulte;F. Schüssler;T. Seitz;C. Sieger;M. Spurio;J. Steijger;T. Stolarczyk;A. Sánchez;M. Taiuti;C. Tamburini;A. Trovato;M. Tselengidou;C. Tönnis;D. Turpin;D. Turpin;D. Turpin;B. Vallage;C. Vallée;V. Elewyck;M. Vecchi;E. Visser;D. Vivolo;S. Wagner;J. Wilms;J. Zornoza;J. Zúñiga;A. Klotz;A. Klotz;M. Boër;A. L. V. Suu;C. Akerlof;W. Zheng;P. Evans;N. Gehrels;J. Kennea;J. Osborne;D. Coward
高能中微子可以在带电宇宙射线与天体物理源周围的物质或辐射的相互作用中产生。即使最近通过冰立方实验探测到地外高能中微子，也没有发现任何天体物理中微子源。瞬态源，如伽马射线暴、核心坍缩超新星或活动星系核都是很有希望的候选者。多信使程序提供了一个独特的机会来检测这些瞬态源。通过将ANTARES中微子望远镜提供的信息与来自其他天文台的信息相结合，探测到源的可能性提高了，从而有可能从单个探测到的事件中识别出中微子祖。在ANTARES合作中开发了一种基于光学和x射线跟踪高能中微子警报的方法。这种方法不需要对中微子和光子光谱之间的关系作任何假设，只需要时间相关。这个程序，被称为TAToO，在中微子探测后触发机器人光学望远镜（TAROT和ROTSE）和Swift-XRT网络，延迟只有几秒钟，因此非常适合寻找快速瞬态源。为了识别中微子信号的光学或x射线对应物，后续观测提供的图像用专用管道进行分析。总共有42个光学警报和7个x射线警报，在中微子触发器分析后最长延迟24小时拍摄。没有发现与中微子触发器相关的光学或x射线对应物，并且推导了瞬态源大小的上限。对每个警报都计算了拒绝伽玛暴起源假设的概率。
High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. Even with the recent detection of extraterrestrial high-energy neutrinos by the IceCube experiment, no astrophysical neutrino source has yet been discovered. Transient sources, such as gamma-ray bursts, core-collapse supernovae, or active galactic nuclei are promising candidates. Multi-messenger programs offer a unique opportunity to detect these transient sources. By combining the information provided by the ANTARES neutrino telescope with information coming from other observatories, the probability of detecting a source is enhanced, allowing the possibility of identifying a neutrino progenitor from a single detected event. A method based on optical and X-ray follow-ups of high-energy neutrino alerts has been developed within the ANTARES collaboration. This method does not require any assumptions on the relation between neutrino and photon spectra other than time-correlation. This program, denoted as TAToO, triggers a network of robotic optical telescopes (TAROT and ROTSE) and the Swift-XRT with a delay of only a few seconds after a neutrino detection, and is therefore well-suited to search for fast transient sources. To identify an optical or X-ray counterpart to a neutrino signal, the images provided by the follow-up observations are analysed with dedicated pipelines. A total of 42 alerts with optical and 7 alerts with X-ray images taken with a maximum delay of 24 hours after the neutrino trigger have been analysed. No optical or X-ray counterparts associated to the neutrino triggers have been found, and upper limits on transient source magnitudes have been derived. The probability to reject the gamma-ray burst origin hypothesis has been computed for each alert.
影响因子：
6.5
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. Boeser;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. Demiroers;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. Góra;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;P. Herquet;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. Koepke;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. Luenemann;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. Schoenwald;A. Schukraft;A. Schultes;O. Schulz;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. Stoessl;E. Strahler;R. Strom;M. Stueer;G. Sullivan;Q. Swillens;H. Taavola;I. Taboada;A. Tamburro;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;Chun Xu;D. Xu;X. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;M. Zoll;C. Akerlof;S. Pandey;Fang Yuan;W. Zheng
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. Boeser;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. Demiroers;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. Góra;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;P. Herquet;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. Koepke;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. Luenemann;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. Schoenwald;A. Schukraft;A. Schultes;O. Schulz;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. Stoessl;E. Strahler;R. Strom;M. Stueer;G. Sullivan;Q. Swillens;H. Taavola;I. Taboada;A. Tamburro;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;Chun Xu;D. Xu;X. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;M. Zoll;C. Akerlof;S. Pandey;Fang Yuan;W. Zheng
影响因子：
8.6
作者：
Aartsen, M. G.;Ackermann, M.;Zoll, M.
通讯作者：
Zoll, M.
影响因子：
8.6
作者：
S. Hümmer;P. Baerwald;W. Winter
通讯作者：
S. Hümmer;P. Baerwald;W. Winter