KM3NeT/ARCA Sensitivity to Starburst Galaxies

被引:0
|
作者
Ambrosone, A. [1 ,2 ]
Ibnsalih, W. I. [2 ,3 ]
Marinelli, A. [1 ,2 ,5 ]
Miele, G. [1 ,2 ,4 ]
Migliozzi, P. [2 ]
Musone, M. R. [2 ,3 ]
机构
[1] Complesso Univ Monte S Angelo, Univ Napoli Federico II, Dipartimento Fis Ettore Pancini, I-80126 Naples, Italy
[2] Complesso Univ Monte S Angelo, INFN, Sez Napoli, I-80126 Naples, Italy
[3] Univ Campania Luigi Vanvitelli, Naples, Italy
[4] Univ Napoli Federico II, Scuola Super Merid, Largo San Marcellino 10, I-80138 Naples, Italy
[5] INAF Osservatorio Astron Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
关键词
D O I
10.1051/epjconf/202328003001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work, the expectations of the full detector KM3NeT/ARCA are presented for particular starburst galaxies signals. For the point-like search approach, we considered the most promising local starburst galaxies to be observed as point-like neutrino excesses: NGC 1068, the Small Magellanic Cloud and the Circinus Galaxy. In both cases, we provide the energy-integrated sensitivity for two ARCA building blocks in the energy range 100 GeV 10 PeV. In the diffuse scenario, both track and shower events were considered. For the point like analysis, only v charge current events were taken into account. Interestingly, ARCA has the potential to constrain the selected phenomenological scenarios, providing evidence of the link between star-forming processes and hadronic emissions.
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页数:4
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