[PDF] Top 20 Results and Perspectives of the Auger Engineering Radio Array

... AERA radio detectors (circles filled with color corresponding to the measured value) and fitted with the azimuthally asymmetric, two-dimensional signal distribution function (background ...the Auger surface ... See full document

... Pierre Auger Observatory for a diffuse flux of neutrinos in the period 1 Jan 2004 - 31 March ...in Auger using hybrid events, the blue dashed boxes mark the systematic uncertainties of this ...by ... See full document

... Abstract. The Pierre Auger Observatory is the largest ultrahigh-energy cosmic ray ob- servatory in the world. The huge amount of high quality data collected since 2004 up to now led to great improvements in our ... See full document

... for radio and microwave detection of UHE air showers is un- der ...the Auger Engineering Radio Array (AERA) has started [7] and several GHz-antennas are installed and taking data ... See full document

... two Auger and two TA SD stations for EASs observed in ...the Auger (South) and TA SD stations for EASs landing near the CLF that triggered the TA ...the Auger (South) and TA SD station response for a ... See full document

... the radio signals was ...reliminary results are illustrated in ...the Radio Detector) is plotted as a function of the muon number (as obtained with the water- ˇ Cerenkov ... See full document

... Pierre Auger Observatory is taking place at the moment, including the deployment of scintillators on top of each surface detector, small PMTs to increase the dynamic range, radio antennas and new ...surface ... See full document

... the Radio Detector) is plotted as a function of the muon number (as obtained with the water-Cherenkov de- ...the radio upgrade such as mass resolution, energy resolution, e ff ective aperture as a function ... See full document

... allows radio measurements up to ultra-high energies, and yields very complementary information to that provided by the water-Cherenkov detectors of the ...a radio antenna on top of each water-Cherenkov de- ... See full document

... tion [7] in an air shower with reconstructed energy of (9.54 ± 0.39 ± 0.18) × 10 17 eV and zenith angle of (21.8 ± 0.4) ◦ is shown in fig. 10. Both air shower ar- rival geometry and energy were obtained from the surface ... See full document

... Radio detection of ultra high energy cosmic rays with the Auger Engineering Radio Array. 10:00 - 10:30 Abigail Vieregg[r] ... See full document

... the radio emission from air showers in the frequency range 30 to 80 ...the radio antenna will be passed to the read-out electronics of the Surface Scintillator Detector/water-Cherenkovdetector system (UUB) ... See full document

... that Auger electron peaks stand out clearly over a slowly varying background of secondary ...the Auger signal and the use of the standard LEED system for detection, made the method attractive for surface ... See full document

... In [1], a possible hint of a correlation between the arrival directions of UHECR and HE neutrinos was reported, us- ing a simple and model-independent method. A first up- date published in [2] lowered the significance of ... See full document

... Pierre Auger Observatory [1], conceived to characterize the properties of the UHECRs, is a hybrid instrument for air shower ...an array of particle detectors, the Surface Detector array (SD) [2], to ... See full document

... the radio loud AGN from the 2FHL catalog (Fermi−LAT, 360 sources), from which 17 within 250 Mpc were extracted, selected according to their γ−ray flux above 50 ...the radio flux for the AGNs and the ... See full document

... In-BnDTPA-F3 were performed in 231-H2N xenograft-bearing mice. In tumor growth delay studies, 111 In-BnDTPA- F3 (3 μ g, 6 MBq/ μ g) was administered intravenously to 231-H2N xenograft-bearing mice once weekly for 3 ... See full document

... of radio SNRs and their local envirnments in the direc- tion of NGC 300 and the Small Magellanic Cloud ...Compact Array (ATCA) and Very Long Array observations, 18 radio SNRs (with 3 ... See full document

... the Auger, HiRes, Telescope Array (TA) and Yakutsk ...experimental results and to try to discuss the measurements in terms of the cosmic ray mass ...from Auger are shallower and less ... See full document

... power combination of delayed paths. Due to the additional spatial dimension, both multipath fading and MAI are bet- ter mitigated, leading to the increased channel capacity and improved output SINR [6]. When constructing ... See full document