[PDF] Top 20 La formación de docentes en TIC en la Universidad Católica de Colombia

... The ANTARES strategy for the study of an enhanced diffuse flux is different with respect to that for the search for point-like ...a cosmic signal (either point-like or diffuse) is expected to be ... See full document

... use neutrino emission from the bulk of unresolved astrophysical neutrino sources ...a cosmic neutrino flux would emerge from the background of atmospheric ...the IceCube signal ... See full document

... Abstract. Antares, the first undersea neutrino telescope, has been continuously operating since 2007 in the Mediterranean ...of neutrino events of all ...for neutrino source searches, in a ... See full document

... candidate cosmic ray ...observed neutrino flux comes from these ...from ANTARES limit the contribution from a single Galactic source, such as the Galactic center [9], but do not ... See full document

... the neutrino fluxes, plus one for the DOM ...astrophysical flux, the cosmic-ray spectral index, and the K/π and ν/ν ratio for conventional neutrinos, and the as- trophysical flux spectral ... See full document

... The IceCube project is an ice-based neutrino detector residing at the geographic south pole in ...astrophysical neutrino production. Construction first started on IceCube in 2005 with the ... See full document

... return flux: neutral hydrogen atoms crossing the (collisionless) shock towards downstream can suffer a charge exchange reaction with a hot ion downstream of the ... See full document

... for neutrino energies above 2 GeV, while the blue band shows a fit to the data between 100MeV and 30GeV when fixing the spectrum to the ...the neutrino flux derived from Poisson statistics for half a ... See full document

... Ultra-high energy cosmic rays are observed via the exten- sive air showers (EAS) they induce in the atmosphere. The EAS can be observed in their longitudinal development through telescopes that detect the ... See full document

... astrophysical neutrino spectrum is expected to follow the source proton spec- trum because the entire energy of a primary proton is transferred to the pions produced in the ...of neutrino source spectral ... See full document

... and cosmic rays by using radio telescopes to search for short pulses from the ...a neutrino or cosmic ray impinges on the Moon and interacts below the lunar ...the neutrino flux above ... See full document

... of IceCube-170922A with a flaring blazar? To answer this question a Monte Carlo sample representative of the IceCube realtime EHE stream was ...energy flux in the monthly bin overlapping with the ... See full document

... from IceCube-InIce, and the IceTop result at ...the IceCube-InIce result at simi- lar energies, but is derived from significantly more ...of cosmic rays at those ...of cosmic rays is planned ... See full document

... existing neutrino telescopes is the charged current ν channel because the target volume is increased by interactions outside the detector, with high energy muons propagating several kilometers before crossing the ... See full document

... MEASUREMENT OF THE GALACTIC COSMIC RAY ANTIPROTON FLUX FROM 0 25 GEV TO 3 11 GEV WITH THE ISOTOPE MATTER ANTIMA TIER EXPERIMENT (IMAX) Thesis by Allan Wayne Labrador In Partial Fulfillment of the Requ[.] ... See full document

... Although the SD of the Pierre Auger Observatory is primarily an UHECR detector, air showers induced by UHE neutrinos can also be e ffi ciently identified above 10 17 eV in the background of UHECR [11]. The iden- ... See full document

... and cosmic rays have been our only probes for that task, but this has ...energy cosmic neutrinos by IceCube [1, 2] and the discovery of gravitational waves by LIGO experiment ...energy cosmic ... See full document

... The ANTARES detector is currently the largest undersea neutrino ...for cosmic neutrinos for more than 10 years. High-energy cosmic neutrino production is strongly linked with ... See full document

... 90% confidence interval of the upper limit, showing the level of variation within each region. The average values were obtained as geometric averages, which better re- present the upper limit values as they are ... See full document

... A line supports 25 mechanical frames, so called storeys, instrumented with three photo-multipliers each. In addition a 13th line, the Instrumentation Line (IL), is used for environmental monitoring and multidisciplinary ... See full document