17 research outputs found
UHE tau neutrino flux regeneration while skimming the Earth
The detection of Earth-skimming tau neutrinos has turned into a very
promising strategy for the observation of ultra-high energy cosmic neutrinos.
The sensitivity of this channel crucially depends on the parameters of the
propagation of the tau neutrinos through the terrestrial crust, which governs
the flux of emerging tau leptons that can be detected. One of the
characteristics of this propagation is the possibility of regeneration through
multiple conversions, which are often neglected
in the standard picture. In this paper, we solve the transport equations
governing the propagation and compare the flux of emerging tau
leptons obtained allowing regeneration or not. We discuss the validity of the
approximation of neglecting the regeneration using different
scenarios for the neutrino-nucleon cross-sections and the tau energy losses.Comment: 8 pages, 8 figure
Tau energy losses at ultra-high energy: continuous versus stochastic treatment
We study the energy losses of the tau lepton in matter through
electromagnetic processes at ultra-high energy (UHE). We use both a stochastic
and a continuous framework to treat these interactions and compare the flux of
tau leptons propagated after some amount of matter. We discuss the accuracy of
the approximation of continuous energy losses by studying the propagation in
standard rock of taus with both mono-energetic and power law injection spectra.Comment: 7 pages, 8 figure
Development of the photomultiplier tube readout system for the first Large-Sized Telescope of the Cherenkov Telescope Array
The Cherenkov Telescope Array (CTA) is the next generation ground-based very
high energy gamma-ray observatory. The Large-Sized Telescope (LST) of CTA
targets 20 GeV -- 1 TeV gamma rays and has 1855 photomultiplier tubes (PMTs)
installed in the focal plane camera. With the 23 m mirror dish, the night sky
background (NSB) rate amounts to several hundreds MHz per pixel. In order to
record clean images of gamma-ray showers with minimal NSB contamination, a fast
sampling of the signal waveform is required so that the signal integration time
can be as short as the Cherenkov light flash duration (a few ns). We have
developed a readout board which samples waveforms of seven PMTs per board at a
GHz rate. Since a GHz FADC has a high power consumption, leading to large heat
dissipation, we adopted the analog memory ASIC "DRS4". The sampler has 1024
capacitors per channel and can sample the waveform at a GHz rate. Four channels
of a chip are cascaded to obtain deeper sampling depth with 4096 capacitors.
After a trigger is generated in a mezzanine on the board, the waveform stored
in the capacitor array is subsequently digitized with a low speed (33 MHz) ADC
and transferred via the FPGA-based Gigabit Ethernet to a data acquisition
system. Both a low power consumption (2.64 W per channel) and high speed
sampling with a bandwidth of 300 MHz have been achieved. In addition, in
order to increase the dynamic range of the readout we adopted a two gain system
achieving from 0.2 up to 2000 photoelectrons in total. We finalized the board
design for the first LST and proceeded to mass production. Performance of
produced boards are being checked with a series of quality control (QC) tests.
We report the readout board specifications and QC results.Comment: In Proceedings of the 34th International Cosmic Ray Conference
(ICRC2015), The Hague, The Netherlands. All CTA contributions at
arXiv:1508.0589
GammapyVersion 0.19
Gammapy is a community-developed, open-source Python package for gamma-ray astronomy built on Numpy, Scipy and Astropy. It is the core library for the CTA science tools and can also be used to analyse data from existing imaging atmospheric Cherenkov telescopes (IACTs), such as H.E.S.S., MAGIC and VERITAS. It also provides some support for Fermi-LAT and HAWC data analysis