scholarly journals Study of the high-energy neutrino diffuse flux with the ANTARES neutrino telescope

2019 ◽  
Author(s):  
Luigi Antonio Fusco ◽  
Federico Versari ◽  
2002 ◽  
Vol 13 (4) ◽  
pp. 590-597 ◽  
Author(s):  
Alessandro Gabrielli ◽  
Enzo Gandolfi ◽  
Pierpaolo Ricci

2021 ◽  
Vol 84 (4) ◽  
pp. 513-518
Author(s):  
A. D. Avrorin ◽  
A. V. Avrorin ◽  
V. M. Aynutdinov ◽  
R. Bannasch ◽  
Z. Bardáčová ◽  
...  

2003 ◽  
Author(s):  
S. W. Barwick ◽  
J. Ahrens ◽  
X. Bai ◽  
T. Becka ◽  
K.-H. Becker ◽  
...  

2009 ◽  
Vol 79 (4) ◽  
Author(s):  
Stefan Schönert ◽  
Thomas K. Gaisser ◽  
Elisa Resconi ◽  
Olaf Schulz

Science ◽  
2018 ◽  
Vol 361 (6398) ◽  
pp. eaat1378 ◽  
Author(s):  
◽  
Mark Aartsen ◽  
Markus Ackermann ◽  
Jenni Adams ◽  
Juan Antonio Aguilar ◽  
...  

Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neutrinos remain unidentified. On 22 September 2017, we detected a high-energy neutrino, IceCube-170922A, with an energy of ~290 tera–electron volts. Its arrival direction was consistent with the location of a known γ-ray blazar, TXS 0506+056, observed to be in a flaring state. An extensive multiwavelength campaign followed, ranging from radio frequencies to γ-rays. These observations characterize the variability and energetics of the blazar and include the detection of TXS 0506+056 in very-high-energy γ-rays. This observation of a neutrino in spatial coincidence with a γ-ray–emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.


2021 ◽  
Vol 47 (2) ◽  
pp. 94-104
Author(s):  
A. V. Avrorin ◽  
A. D. Avrorin ◽  
V. M. Aynutdinov ◽  
R. Bannasch ◽  
Z. Bardáčová ◽  
...  

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