[PDF] Top 20 Commissioning and performance of the CMS silicon strip tracker with cosmic ray muons
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Commissioning and performance of the CMS silicon strip tracker with cosmic ray muons
... algorithms The two main algorithms used to reconstruct tracks from cosmic ray muons in CRAFT data are the Combinatorial Track Finder (CTF) and the Cosmic Track ... Voir le document complet
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Commissioning and performance of the CMS pixel tracker with cosmic ray muons
... selection and simulation The CMS collaboration conducted a month-long data taking exercise known as the Cosmic Run At Four Tesla (CRAFT) during October–November 2008, with ... Voir le document complet
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Alignment of the CMS tracker with LHC and cosmic ray data
... obtain the best possible track reconstruction performance, the tracker geometry is carefully monitored as a function of time, so that corrections can be applied upon movements large ... Voir le document complet
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Commissioning of the CMS experiment and the cosmic run at four tesla
... Trigger and Data Acquisition The typical Level-1 trigger rate during CRAFT was 600 ...below the 100 kHz design limit for the central data acquisition (DAQ) system and is composed ... Voir le document complet
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Alignment of the CMS muon system with cosmic-ray and beam-halo muons
... With the first LHC collisions, groups of CSCs will be interaligned using (b) and these rigid- body groups will be aligned relative to the tracker with ...comparisons ... Voir le document complet
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Commissioning of the CMS High-Level Trigger with cosmic rays
... 2008 the CMS Collaboration conducted a month-long data taking exercise known as the Cosmic Run At Four Tesla (CRAFT) with the goal of commissioning the ... Voir le document complet
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Alignment of the CMS silicon tracker during commissioning with cosmic rays
... Introduction The main goal of the CMS experiment [1] is to explore physics at the TeV energy scale exploit- ing the proton-proton collisions delivered by the Large Hadron ... Voir le document complet
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Cosmic-ray astronomy at the highest energies with ten years of data of the Pierre Auger observatory
... techniques The two methods described above are the two main ones used for detecting ...proposed and are currently under test. Detecting radio emission from the shower particles in the ... Voir le document complet
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Radiodetection of Cosmic Ray Extensive Air Showers: upgrade of the CODALEMA experiment
... Using the position and the timing differences between antennas, it was also possible to perform the trajectory reconstruction of the electromagnetic plane wave using a triangu- ... Voir le document complet
5
Commissioning twin houses for assessing the performance of energy conserving technologies
... Benchmarking the space heating consumption, theoretically the more challenging exercise, turned out to be simpler in that the results confirmed that the objective of the design ... Voir le document complet
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Performance of the first prototype of the CALICE scintillator strip electromagnetic calorimeter
... The CALICE scintillator strip-based ECAL (ScECAL) achieves the required granularity with a scintillator strip ...Each strip is individually read out by a Multi Pixel Photon ... Voir le document complet
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A criterion to discriminate between solar and cosmic ray forcing of the terrestrial climate
... for the 22-year cycle comes from varves, i.e. pairs of thin layers of ...sediment. The first varve layer is usually light and composed of sand, pollen, and 15 spores, ... Voir le document complet
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The Cerenkov effect in cosmic ray air showers
... In the event of a three or four fold scintillation counter coincidence the direction of the shower could be determined from measurements of the differences in the arriv[r] ... Voir le document complet
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Radio Detection of Cosmic Ray Extensive Air Showers
... mechanisms of electromagnetic pulse generation have been identified (Allan ...is the negative charge excess in the shower. This contribution to the total electric field depends only from ... Voir le document complet
5
Determining the jet opening angle of cosmic gamma-ray bursts
... Swift gives even more rapid timescales for hurst localizations, allowing great r olpportilli y to observe the burst afterglow with grolnd and( space-}ase(l 1 elesope(([r] ... Voir le document complet
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Ultimate precision in cosmic-ray radio detection — the SKA
... As of 2023, the low-frequency part of the Square Kilometre Array will go online in ...constitute the largest and most powerful low-frequency radio- astronomical observatory to ... Voir le document complet
7
The cosmic ray muon energy spectum via Čerenkov radiation
... I con- structed a signal chain for measurement, collected data for muon energies with the goal of constructing the muon energy spectrum from different Cerenkov spec[r] ... Voir le document complet
55
X-ray multilayer monochromator with enhanced performance
... to the principles of a multilayer monochro- mator with an improved resolution and a low specu- lar background, based on a ...3 and 4 deal with the techniques of ... Voir le document complet
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MATISSE Instrument Performance Report: Commissioning Report. V1.1
... The low resolution (LR) N band data of HD 45677 were recorded simultaneously to its L/M band data within the commisioning run 1C in December 1-14, ...2018. The N band interferograms were ... Voir le document complet
106
Performance enhancement of a BSDF test bench using an algorithm fed with laser-tracker measurements
... In the field of earth-observation, on-board calibration is often necessary to guarantee the radiometric accuracy of space ...front of the instrument, illuminated with a ... Voir le document complet
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