[PDF] Top 20 Search for GRB neutrino emission according to the photospheric model with the ANTARES telescope
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Search for GRB neutrino emission according to the photospheric model with the ANTARES telescope
... of neutrino detectors goes back to the 1950s, when Clyde Cowan and Frederick Reines first detected neutrinos from a nuclear reactor [ 1 ...In the following years scientists detected ... Voir le document complet
120
New constraints on all flavor Galactic diffuse neutrino emission with the ANTARES telescope
... cut-off model) as obtained from Monte Carlo simulation, depend on the differential neutrino fluxes pre- dicted by the reference models folded with the detector response to ... Voir le document complet
10
Stacked search for time shifted high energy neutrinos from gamma ray bursts with the Antares neutrino telescope
... Delay The approach presented in this paper aims at be- ing as model independent as ...possible. The max- imum time shift anticipated from the astrophysi- cal processes mentionned in section ... Voir le document complet
18
The Search for Neutrinos from TXS 0506+056 with the ANTARES Telescope
... The ANTARES [6] telescope is a deep-sea Cherenkov neutrino detector, lo- cated 40 km off shore from Toulon, France, in the Mediterranean ...Sea. The telescope aims ... Voir le document complet
11
ANTARES upper limits on the multi-TeV neutrino emission from the GRBs detected by IACTs
... Conclusions The offline ANTARES neutrino searches presented here yields no neutrinos observed in correlation with the three GRBs detected so far by ground-based gamma-ray facilities ... Voir le document complet
13
Search for a diffuse flux of high-energy νμ with the ANTARES neutrino telescope
... of the detector In the simulation of the digitized signal, the main features of the PMTs and of the ARSs are taken into ...account. The simulated photons arriving on each ... Voir le document complet
8
First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope
... searches for neutrinos from G RBs have been perform ed in th e N o rth ern hem i sphere by AM ANDA [3] and IceC ube [4, 5] at sim ilar energies (TeV -PeV ) and by A N ITA [6] a t higher energies (> P eV ...o ... Voir le document complet
16
Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope
... by the three GW pipelines online and offline, but with low significance before the updated ...blind search for prompt neutrino emission correlated with the ... Voir le document complet
13
First Search for Point Sources of High Energy Cosmic Neutrinos with the ANTARES Neutrino Telescope
... is the neutrino energy. The median of this angular error is ...degrees. For the subset of data in which the full 12-line detector was operational, the resolution is ... Voir le document complet
17
First combined search for neutrino point-sources in the Southern Hemisphere with the ANTARES and IceCube neutrino telescopes
... the background of atmospheric muons and neutrinos only (Aartsen et ...2013c,b). The specific origin of these events is currently ...of the flux may have a galactic origin (Ahlers et ...on the ... Voir le document complet
25
Search for neutrinos from the tidal disruption events AT2019dsg and AT2019fdr with the ANTARES telescope
... expected to accumulate around the source position. The energy information helps to distinguish signal from background, as a softer energy spectrum is predicted for atmospheric neutrinos ... Voir le document complet
10
All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the Antares neutrino telescope
... Carlo to accurately reproduce the evolution of the event rate observed in the data from one run to ...Due to the low number of events passing the optimized quality ... Voir le document complet
12
Search for Neutrino Emission from Gamma-Ray Flaring Blazars with the ANTARES Telescope
... Abstract The ANTARES telescope is well-suited to detect neutrinos produced in astrophys- ical transient sources as it can observe a full hemisphere of the sky at all times with a ... Voir le document complet
16
Search for Relativistic Magnetic Monopoles with the ANTARES Neutrino Telescope
... of the same velocity. Moreover, be- low the Cherenkov threshold β th = ...leading to indirect Cherenkov emission from knock off electrons (δ−rays) produced along its path ...shows the ... Voir le document complet
16
Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
... used to search for these particles: pro- duction at particle accelerators [3] , direct detection of the recoil from collisions with nuclei [4] or indirect detection by means of ... Voir le document complet
7
A Search for Neutrino Emission from the Fermi Bubbles with the ANTARES Telescope
... in the period from May 2008, when the detector started to operate in its complete con- figuration, until December 2011 are ...used. The total livetime selected for this analysis amounts ... Voir le document complet
13
Search for relativistic magnetic monopoles with five years of the ANTARES detector data
... 2 The ANTARES telescope The ANTARES detector [16] is an undersea neutrino telescope anchored 2475 m below the surface of the Mediterranean Sea and 40 km ... Voir le document complet
23
Model-independent search for neutrino sources with the ANTARES neutrino telescope
... Due to the fact that the method is independent of neutrino emission models or assumptions on the topology of emission regions, this analysis is not intended to ... Voir le document complet
33
First all-flavor neutrino pointlike source search with the ANTARES neutrino telescope
... atmospheric neutrino flux. The simulation of the amount of optical background ( 40 K and biolu- minescence) is performed according to the collected data in order to ... Voir le document complet
25
Search for high energy neutrinos from the Galactic plane with the ANTARES neutrino telescope
... , the source location was ideal for the Pierre Auger ...Observatory. With a source located in the upward-going ield of view of A or I C , we can expect a luence sensitivity 5 to ... Voir le document complet
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