Transient point source analyses in the ANTARES neutrino telescope

被引：0
作者：
Sanchez Losa, Agustin [1 ]
机构：
[1] Univ Valencia, CSIC, IFIC Inst Fis Corpuscular, Valencia 46071, Spain
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2014年 / 742卷
关键词：
ANTARES; Neutrino astronomy; Transient analysis; Micro-quasars; GRBs; AGNs; LARGE-AREA TELESCOPE; SEPTEMBER; CATALOG;
D O I：
10.1016/j.nima.2013.11.096
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
The ANTARES telescope, with a duty cycle close to unity and a full hemisphere of the sky at all the times visible, is well suited to detect neutrinos produced in astrophysical transient sources. Assuming a known neutrino production period, the background and the sensitivity can be drastically improved by selecting a narrow time window around it. GRBs, mu-quasars and AGNs are particularly attractive potential neutrino point sources since neutrinos and gamma-rays may be produced in hadronic interactions with the surrounding medium as they are the most likely sources of the observed ultra high energy cosmic rays. A strong correlation between the gamma-ray and the neutrino fluxes is expected in this scenario. ANTARES data has been analyzed in various transient source analyses with the goal of detecting cosmic neutrinos from GRBs, mu-quasars and AGNs. The sensitivity of a standard time-integrated point source search can be improved by a factor 2-3 by looking for neutrinos only during the most probable emission time. This information can be provided by the different satellite telescope types on the X-rays and gamma-rays wavelengths. The results of these different analyses will be presented. (C) 2013 Elsevier B.V. All rights reserved.
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页码：195 / 198
页数：4
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