90 results on '"H. BLUMER"'
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2. Relativistic Shapiro Delay Measurements of an Extremely Massive Millisecond Pulsar
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H T Cromartie, E Fonseca, S M Ransom, P B Demorest, Z Arzoumanian, H Blumer, P R Brook, M E DeCesar, T Dolch, J A Ellis, R D Ferdman, E C Ferrara, N Garver-Daniels, P Gentile, M L Jones, M T Lam, D R Lorimer, R S Lynch, M A McLaughlin, C Ng, D J Nice, T T Pennucci, R Spiewak, I H Stairs, K Stovall, J K Swiggum, and W W Zhu
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Astronomy - Abstract
Despite its importance to our understanding of physics at supranuclear densities, the equation of state (EoS) of matter deep within neutron stars remains poorly understood. Millisecond pulsars (MSPs) are among the most useful astrophysical objects in the Universe for testing fundamental physics, and place some of the most stringent constraints on this high-density EoS. Pulsar timing—the process of accounting for every rotation of a pulsar over long time periods—can precisely measure a wide variety of physical phenomena, including those that allow the measurement of the masses of the components of a pulsar binary system1. One of these, called relativistic Shapiro delay2, can yield precise masses for both an MSP and its companion; however, it is only easily observed in a small subset of high-precision, highly inclined (nearly edge-on) binary pulsar systems. By combining data from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) 12.5-yr data set with recent orbitalphase- specific observations using the Green Bank Telescope, we have measured the mass of the MSP J0740+6620 to be 2.14+0:10-0:09 M⊙ (68.3% credibility interval; the 95.4% credibility interval is 2.14+0:20-0:18 M⊙). It is highly likely to be the most massive neutron star yet observed, and serves as a strong constraint on the neutron star interior EoS.
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- 2019
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3. High-precision x-ray timing of three millisecond pulsars with NICER: Stability estimates and comparison with radio
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J S Deneva, P. S. Ray, A Lommen, S M Ransom, S Bogdanov, M. Kerr, K. S. Wood, Z Arzoumanian, K. Black, J. Doty, K C Gendreau, S. Guillot, A. Harding, N. Lewandowska, C Malacaria, C B Markwardt, S. Price, L Winternitz, M. T. Wolff, L. Guillemot, I. Cognard, P. T. Baker, H. Blumer, P R Brook, H T Cromartie, P B Demorest, M E DeCesar, T. Dolch, J. A. Ellis, R D Ferdman, E C Ferrara, E Fonseca, N Garver-Daniels, P A Gentile, M. L. Jones, M. T. Lam, D R Lorimer, R. S. Lynch, M. A. McLaughlin, C. Ng, D J Nice, T T Pennucci, R Spiewak, I H Stairs, K Stovall, J K Swiggum, S. J. Vigeland, and W. W. Zhu
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Astrophysics - Abstract
The Neutron Star Interior Composition Explorer (NICER) is an X-ray astrophysics payload on the International Space Station. It enables unprecedented high-precision timing of millisecond pulsars (MSPs) without the pulse broadening and delays due to dispersion and scattering within the interstellar medium that plague radio timing. We present initial timing results from a year of data on the MSPs PSR B1937+21 and PSR J0218+4232, and nine months of data on PSR B1821−24. NICER time-of-arrival uncertainties for the three pulsars are consistent with theoretical lower bounds and simulations based on their pulse shape templates and average source and background photon count rates. To estimate timing stability, we use the σz measure, which is based on the average of the cubic coefficients of polynomial fits to subsets of timing residuals. So far we are achieving timing stabilities σz≈3×10−14 for PSR B1937+21 and on the order of 10−12 for PSRs B1821−24 and J0218+4232. Within the span of our NICER data we do not yet see the characteristic break point in the slope of σz; detection of such a break would indicate that further improvement in the cumulative root-mean-square timing residual is limited by timing noise. We see this break point in our comparison radio data sets for PSR B1821−24 and PSR B1937+21 on timescales of >2 yr.
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- 2019
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4. PSR J2234+0611: A New Laboratory for Stellar Evolution
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K Stovall, P C C Freire, J Antoniadis, M Bagchi, J S Deneva, N Garver-Daniels, J G Martinez, M A McLaughlin, Z Arzoumanian, J H Blumer, P R Brook, H T Cromartie, P B Demorest, M E DeCesar, T Dolch, J A Ellis, R D Ferdman, E C Ferrara, E Fonseca, P A Gentile, M L Jones, M T Lam, D R Lorimer, R S Lynch, C Ng, D J Nice, T T Pennucci, S M Ransom, R Spiewak, I H Stairs, J K Swiggum, S J Vigeland, and W W Zhu
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Astronomy - Abstract
We report the timing results for PSR J2234+0611, a 3.6 ms pulsar in a 32 day, eccentric (e = 0.13) orbit with a helium white dwarf. The precise timing and eccentric nature of the orbit allow measurements of an unusual number of parameters: (a) a precise proper motion of 27.10(3) mas yr−1 and a parallax of 1.05(4) mas resulting in a pulsar distance of 0.95(4) kpc; enabling an estimate of the transverse velocity, 123(5) km s−1. Together with previously published spectroscopic measurements of the systemic radial velocity, this allows a 3D determination of the system’s velocity; (b) precise measurements of the rate of advance of periastron yields a total system mass of 1.6518 +0.0033-0.0035 Msun; (c) a Shapiro delay measurement, h3 = 82 ± 14 ns, despite the orbital inclination not being near 90°; combined with the measurement of the total mass yields a pulsar mass of 1.353 +0.014-0.017 Msun and a companion mass of 0.298 +0.015-0.0120 Msun; (d) we measure precisely the secular variation of the projected semimajor axis and detect a significant annual orbital parallax; together these allow a determination of the 3D orbital geometry of the system, including an unambiguous orbital inclination (i = 138.7 +2.5-2.2 deg) and a position angle for the line of nodes ( omega = 44 +5-4 deg). We discuss the component masses to investigate the hypotheses previously advanced to explain the origin of eccentric MSPs. The unprecedented determination of the 3D position, motion, and orbital orientation of the system, plus the precise pulsar and WD masses and the latter’s optical detection make this system a unique test of our understanding of white dwarfs and their atmospheres.
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- 2019
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5. Quantitative misfit dislocation characterization with electron channeling contrast imaging
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Tyler J. Grassman, Zak H. Blumer, Marzieh Baan, Jacob T. Boyer, and Ari N. Blumer
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Nuclear magnetic resonance ,Materials science ,Electron ,Dislocation ,Contrast imaging ,Instrumentation ,Characterization (materials science) - Published
- 2021
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6. Reduced Dislocation Introduction in III–V/Si Heterostructures with Glide-Enhancing Compressively Strained Superlattices
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Daniel L. Lepkowski, Tyler J. Grassman, Ari N. Blumer, Jacob T. Boyer, and Zak H. Blumer
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Materials science ,Condensed matter physics ,010405 organic chemistry ,Superlattice ,Heterojunction ,General Chemistry ,010402 general chemistry ,Condensed Matter Physics ,01 natural sciences ,0104 chemical sciences ,Condensed Matter::Materials Science ,General Materials Science ,Dislocation ,Computer Science::Information Theory - Abstract
The novel use of a GaAsyP1-y/GaP compressively-strained superlattice (CSS) to provide enhanced control over misfit dislocation (MD) evolution and threading dislocation density (TDD) during GaP/Si m...
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- 2020
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7. Exploring Multiple Pathways to Low TDD GaP/Si for III-V/Si Photovoltaics
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Tyler J. Grassman, Jacob T. Boyer, Zak H. Blumer, Steven A. Ringel, and Daniel L. Lepkowski
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Flexibility (engineering) ,Materials science ,Silicon ,chemistry ,Photovoltaics ,business.industry ,Photovoltaic system ,Scalability ,chemistry.chemical_element ,Dislocation ,business ,Engineering physics - Abstract
Threading dislocation density (TDD) is a key parameter that commonly limits the performance of epitaxially integrated III-V/Si photovoltaics. The GaP/Si epitaxial bridge is a widely studied III-V on Si integration pathway, and recent advances have realized low-106 cm-2 TDD in n-GaP/Si templates that can be integrated in III-V/Si PV designs amenable to efficiencies well beyond single-junction Si. However, continued development and scaling of III-V/Si PV will ultimately rely on a deeper understanding of dislocation evolution in GaP/Si and will require more process flexibility than has heretofore been demonstrated. Thus, this work demonstrates multiple pathways toward achieving-low 106 cm-2 TDD, through which we can gain both substantial fundamental understanding of GaP/Si integration and can achieve the needed process flexibility to enable scalable production.
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- 2021
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8. Recent Advances in GaAsP/Si Top Cell Enabling 27% Tandem Efficiency
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Daniel L. Lepkowski, Stephen Bremner, Jacob T. Boyer, Tyler J. Grassman, Hamid Mehrvarz, Mattias K. Juhl, Udo Römer, Zak H. Blumer, Anastasia Soeriyadi, Chuqi Yi, Tal Kasher, Steven A. Ringel, and Anita Ho-Baillie
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Materials science ,Tandem ,Tandem cell ,Energy conversion efficiency ,Fill factor ,Engineering physics - Abstract
Historically, the performance of monolithically-integrated GaAsP/Si tandem solar cells has been limited by the presence of elevated TDD in the GaAsP subcell. However, our recent development of low-TDD GaAsP/Si virtual substrates has greatly improved the near-term potential for achieving high efficiency devices. In this work, development efforts employing this new low-TDD platform will be presented. First, our current certified record GaAsP/Si tandem cell (23.4% AM1.5G) is briefly analyzed, identifying the root cause of critical fill factor losses, which in turn informs subsequent design and optimization efforts. Second, the experimental development of high performance GaAsP subcells is shown, following device design strategies that improve J SC and fill factor without sacrificing V OC . Finally, conversion efficiency projections demonstrate that the achieved top cell performance metrics, combined with those expected from the newest bottom cell iteration, should enable ~27% efficient tandems.
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- 2021
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9. Development of Low-TDD GaAsyP1-y/GaP/Si Metamorphic Materials for High-Efficiency III-V/Si Photovoltaics
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Jacob T. Boyer, Steven A. Ringel, Ari N. Blumer, Daniel L. Lepkowski, Zak H. Blumer, Tyler J. Grassman, and Francisco A. Rodriguez
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010302 applied physics ,Materials science ,Silicon ,business.industry ,Photovoltaic system ,chemistry.chemical_element ,Heterojunction ,02 engineering and technology ,021001 nanoscience & nanotechnology ,Epitaxy ,7. Clean energy ,01 natural sciences ,Gallium arsenide ,chemistry.chemical_compound ,chemistry ,Photovoltaics ,0103 physical sciences ,Optoelectronics ,Metalorganic vapour phase epitaxy ,Dislocation ,0210 nano-technology ,business - Abstract
Metamorphic III-V/Si materials with low threading dislocation density (TDD) are critical to realizing high-efficiency III-V/Si multijunction photovoltaics. In pursuit of a dual junction III-V/Si design with a GaAs 0.75 P 0.25 top junction epitaxially integrated on a Si bottom junction, we report on progress made in the development of GaP/Si and GaAsyP l-y /Si materials with significantly reduced TDD. Using a tightly integrated study of fundamental dislocation dynamics, rapid electron microscopy based feedback on dislocation populations, and MOCVD process development, we have fully re-engineered the GaP on Si growth process. Our new approach results in a TDD of 7x104 cm−2 for 50 nm thick films. Implementation of a novel dislocation glide enhancing heterostructure then enabled subsequent growth of fully-relaxed, 500 nm total thickness n-GaP with a TDD of 2.4×106 cm−2. When applied to the production of full GaAs 0.75 P 0.25 /Si tandem solar cell structures, but without any significant optimization thus far, this low TDD is effectively maintained, yielding a terminal TDD of only 3.0x106 cm−2, sufficient to support high photovoltaic performance.
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- 2020
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10. Loss Analysis and Design Strategies Enabling >23% GaAsP/Si Tandem Solar Cells
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Steven A. Ringel, Daniel Derkacs, Zak H. Blumer, Stephen Bremner, Anita Ho-Baillie, Chuqi Yi, Anastasia Soeriyadi, Daniel L. Lepkowski, Alex Stavrides, Tyler J. Grassman, Mattias K. Juhl, Chris Kerestes, Jacob T. Boyer, and Hamid Mehrvarz
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010302 applied physics ,Materials science ,Silicon ,Passivation ,Tandem ,Band gap ,business.industry ,chemistry.chemical_element ,02 engineering and technology ,021001 nanoscience & nanotechnology ,01 natural sciences ,Gallium arsenide ,chemistry.chemical_compound ,chemistry ,0103 physical sciences ,Optoelectronics ,Dislocation ,0210 nano-technology ,business ,Photonic crystal ,Voltage - Abstract
Detailed loss analysis of our previously reported 21.8% (unverified) monolithic GaAsP/Si tandem cells has identified and quantified three main mechanisms limiting cell performance: dislocation mediated voltage and current losses, improper bandgap profile, and insufficient rear passivation. This analysis was recently used to redesign the device structure, yielding a substantial performance improvement to 23.4% AM1.5G. The largest area of improvement was in the Voc of 1.73V, an increase of 70 mV versus our previous results, enabled by an -2x reduction in threading dislocation density (TDD) and a more ideal top cell bandgap.
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- 2020
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11. The Green Bank Northern Celestial Cap Pulsar Survey. VI. Discovery and Timing of PSR J1759+5036: A Double Neutron Star Binary Pulsar
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G. Y. Agazie, M. G. Mingyar, M. A. McLaughlin, J. K. Swiggum, D. L. Kaplan, H. Blumer, P. Chawla, M. DeCesar, P. B. Demorest, W. Fiore, E. Fonseca, J. D. Gelfand, V. M. Kaspi, V. I. Kondratiev, M. LaRose, J. van Leeuwen, L. Levin, E. F. Lewis, R. S. Lynch, A. E. McEwen, H. Al Noori, E. Parent, S. M. Ransom, M. S. E. Roberts, A. Schmiedekamp, C. Schmiedekamp, X. Siemens, R. Spiewak, I. H. Stairs, and M. Surnis
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010308 nuclear & particles physics ,Space and Planetary Science ,Astrophysics::High Energy Astrophysical Phenomena ,0103 physical sciences ,Astronomy and Astrophysics ,010303 astronomy & astrophysics ,01 natural sciences - Abstract
The Green Bank North Celestial Cap survey is a 350 MHz all-sky survey for pulsars and fast radio transients using the Robert C. Byrd Green Bank Telescope. To date, the survey has discovered over 190 pulsars, including 33 millisecond pulsars and 24 rotating radio transients. Several exotic pulsars have been discovered in the survey, including PSR J1759+5036, a binary pulsar with a 176 ms spin period in an orbit with a period of 2.04 days, an eccentricity of 0.3, and a projected semi-major axis of 6.8 light seconds. Using seven years of timing data, we are able to measure one post–Keplerian parameter, advance of periastron, which has allowed us to constrain the total system mass to 2.62 ± 0.03 M ⊙. This constraint, along with the spin period and orbital parameters, suggests that this is a double neutron star system, although we cannot entirely rule out a pulsar-white dwarf binary. This pulsar is only detectable in roughly 45% of observations, most likely due to scintillation. However, additional observations are required to determine whether there may be other contributing effects.
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- 2021
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12. Correlation of early-stage growth process conditions with dislocation evolution in MOCVD-based GaP/Si heteroepitaxy
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Jacob T. Boyer, Daniel L. Lepkowski, Zak H. Blumer, Tyler J. Grassman, and Ari N. Blumer
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Inorganic Chemistry ,Materials science ,Annealing (metallurgy) ,Chemical physics ,Materials Chemistry ,Nucleation ,Atomic layer epitaxy ,Chemical vapor deposition ,Metalorganic vapour phase epitaxy ,Dislocation ,Condensed Matter Physics ,Order of magnitude ,Stacking fault - Abstract
To identify the complex relationships between early-stage growth processes and the resultant defect microstructure in GaP/Si heteroepitaxy, a holistic study of several key metal–organic chemical vapor deposition (MOCVD) parameters was conducted, focusing on Si surface preparation and GaP atomic layer epitaxy (ALE) based nucleation processes. Crystalline defects related to the lattice mismatch and/or interfacial heterovalency, namely misfit dislocations (MD), threading dislocations (TD), and stacking fault pyramids (SFP), were quantitatively characterized via electron channeling contrast imaging (ECCI) and correlated against the different process variations. Choice of Si surface preparation method between the two examined (dilute SiH4 annealing versus Si2H6 based homoepitaxy) had little impact on resultant GaP film morphology and defect content, whereas differing GaP ALE nucleation conditions produced much more substantial changes. In particular, the initial precursor species (tert-butylphosphine versus triethygallium) and ALE cycle purge times both yielded significant influence over threading dislocation densities (TDD) in thin (100 nm), post-critical thickness GaP/Si films, with TDD spanning two orders of magnitude, from 6.7 × 107 cm−2 to 7.1 × 105 cm−2, depending on the specific process conditions employed. SFP densities were also found to follow a similar trend, ranging from 2.0 × 107 cm−2 to 1.8 × 105 cm−2, but with no apparent causal relationship between SFP density and TDD. To help explain the dramatic differences observed, detailed, large-area MD network characterization was used to provide statistically-relevant quantitative analyses of the critical dislocation dynamics (introduction rates and glide velocities) associated with the different process variants. These extracted values are then correlated against the ALE process variants to provide insight into the potential mechanistic roles of the different growth processes.
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- 2021
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13. Si-matched BxGa1−xP grown via hybrid solid- and gas-source molecular beam epitaxy
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Daniel L. Lepkowski, Ari N. Blumer, Zak H. Blumer, Tyler J. Grassman, and Jacob T. Boyer
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010302 applied physics ,Materials science ,Physics and Astronomy (miscellaneous) ,business.industry ,Relaxation (NMR) ,BCL3 ,02 engineering and technology ,Substrate (electronics) ,021001 nanoscience & nanotechnology ,01 natural sciences ,Transmission electron microscopy ,0103 physical sciences ,Ultimate tensile strength ,Optoelectronics ,Dislocation ,0210 nano-technology ,business ,Molecular beam epitaxy - Abstract
The growth of BxGa1−xP alloys by hybrid solid/gas-source molecular beam epitaxy, with B supplied via the BCl3 gas precursor, is demonstrated. Compositional control ranging from pure GaP to B0.045Ga0.955P has thus far been achieved. Slightly tensile-strained B0.031Ga0.969P grown on nearly pseudomorphic, compressively strained GaP/Si was used to produce an effectively strain-free (0.06% tensile misfit at growth temperature) 160 nm total III–V thickness BxGa1−xP/Si virtual substrate with a threading dislocation density of
- Published
- 2020
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14. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, E. J. Ahn, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, E. Arganda, S. Argir, K. Arisaka, F. Arneodo, F. Arqueros, T. Asch, H. Asorey, P. Assis, J. Aublin, M. Ave, G. Avila, A. Bacher, T. Backer, D. Badagnani, K. B. Barber, A. F. Barbosa, H. J. M. Barbosa, N. Barenthien, S. L. C. Barroso, B. Baughman, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, A. Belletoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, C. Bleve, H. Blumer, M. Bohacova, E. Bollmann, H. Bolz, C. Bonifazi, R. Bonino, N. Borodai, F. Bracci, J. Brack, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, D. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, J. Castro, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chudoba, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordero, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. W. Cronin, J. Cuautle, A. Curutiu, S. Dagoret Campagne, R. Dallier, F. Daudo, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, G. Decerprit, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, P. N. Diep, C. Dobrigkeit, J. C. D’Olivo, P. N. Dong, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. Du Vernois, R. Engel, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, A. Ferrero, B. Fick, A. Filevich, A. Filipcic, I. Fleck, S. Fliescher, R. Fonte, C. E. Fracchiolla, E. D. Fraenkel, W. Fulgione, R. F. Gama rra, S. Gambetta, B. Garcıa, D. Garcıa Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmekeai, P. L. Ghia, U. Giaccari, K. Gibbs, M. Giller, J. Gitto, H. Glass, L. M. Goggin, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, P. F. Gomez Vitale, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, E. Grashorn, V. Grassi, S. Grebe, M. Grigat, A. F. Grillo, J. Grygar, Y. Guardincerri, N. Guardone, C. Guerard, F. Guarino, R. Gumbsheimer, G. P. Guedes, J. Gutierrez, J. D. Hague, V. Halenka, P. Hansen, D. Harari, S. Harmsma, S. Hartmann, J. L. Harton, A. Haungs, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, G. Hofman, J. R. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, H. Hucker, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, S. Jiraskova, M. Kaducak, K. H. Kampert, T. Karova, P. Kasper, B. Ke, B. Keilhauer, E. Kempq, H. Kern, R. M. Kieckhafer, H. O. Klages, M. . Kleifges, J. Kleinfeller, R. Knapik, J. Knapp, D. H. Koang, A. Kopmann, A. Krieger, O. Kromer, D. Kruppke Hansen, D. Kuempel, N. Kunka, A. Kusenko, G. La Rosa, C. Lachaud, B. L. Lago, P. Lautridou, M. S. A. B. Leao, D. Lebrun, P. Lebrun, J. Lee, M. A. Leiguide Oliveira, A. Lemiere, A. Letessier Selvon, M. Leuthold, I. Lhenry Yvon, R. Lopez, A. Lopez Aguera, K. Louedec, J. Lozano Bahilo, A. Lucero, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, M. Malek, D. Mandat, P. Mantsch, F. Marchetto, A. G. Mariazzi, I. C. Maris, H. R. Marquez Falcon, O. Martineau, O. Martınez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurizio, P. O. Mazur, M. McEwen, R. R. McNeil, G. Medina Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, R. Meyhandan, M. I. Micheletti, G. Miele, W. Miller, L. Miramonti, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, J. C. Moreno, C. Morris, M. Mostafa, C. A. Moura, M. Mucchi, S. Mueller, M. . A. Muller, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, F. Nerling, C. Newman Holmes, D. Newton, P. T. Nhung, D. Nicotra, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nozka, M. Nyklicek, J. Oehlschlager, A. Olinto, P. Oliva, V. M. Olmos Gilbaja, M. Ortiz, F. Ortolani, B. Oßwald, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, G. Parente, E. Parizot, S. Parlati, S. Pastor, M. Patel, T. Paul, V. Pavlidou, K. Payet, M. Pech, J. Pekala, I. M. Pepe, R. Pesce, E. Petermann, S. Petrera, P. Petrinca, A. Petrolini, Y. Petrov, J. Petrovic, C. Pfendner, A. Pichel, R. Piegaia, T. Pierog, M. Pimenta, T. Pinto, V. Pirronello, O. Pisanti, M. Platino, J. Pochon, V. H. Ponce, M. Pontz, J. Pouryamout, L. Prado J.r., P. Privitera, M. Prouza, E. J. Quel, G. Raia, J. Rautenberg, O. Ravel, D. Ravignani, A. Redondo, H. C. Reis, S. Reucroft, B. Revenu, F. A. S. Rezendem, J. Ridky, S. Riggi, M. Risse, C. Riviere, V. Rizi, C. Robledo, M. D. Roberts, G. Rodriguez, J. Ro driguez Martino, J. Rodriguez Rojo, I. Rodriguez Cabo, M. D. Rodrıguez Frias, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouille d’Orfeuil, E. Roulet, A. C. Rovero, F. Salamida, H. Salazar, G. Salina, F. Sanchez, M. Santander, C. E. Santo, E. M. Santos, F. Sarazin, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, G. Schleif, A. Schmidt, F. Schmidt, T. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovanek, F. Schroeder, S. Schulte, F. Schussler, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, D. Semikoz, G. Sequieros, M. Settimo, R. C. Shellard, I. Sidelnik, B. B. Siffert, A. Smiakowski, R. Smıda, A. G. K. Smith, B. E. Smith, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, E. Strazzeri, A. Stutz, F. Suarez, T. Suomijarvi, A. D. Supanitsky, M. S. Sutherland, J. Swain, Z. Szadkowski, A. Tamashiro, A. Tamburro, T. Tarutina, O. Tascau, R. Tcaciuc, D. Tcherniakhovski, N. T. Thao, D. Thomas, R. Ticona, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, B. Tome, A. Tonachini, I. Torres, P. Trapani, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, V. Tuci, M. Tueros, E. Tusi, R. Ulrich, M. Unger, M. Urban, J. F. Valdes Galicia, I. Valino, L. Valore, A. M. van den Berg, J. R. Vazquez, R. A. Vazquez, D. Veberic, A. Velarde, T. Venters, V. Verzi, M. Videla, L. Villasenor, G. Vitali, S. Vorobiov, L. Voyvodic, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Warner, S. Westerhoff, B. J. Whelan, N. Wild, C. Wiebusch, G. Wieczorek, L. Wiencke, B. Wilczynska, H. Wilczynski, C. Wileman, M. G. Winnick, G. Worner, H. Wuac, B. Wundheiler, T. Yamamoto, P. Younk, G. Yuan, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, M. Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, KVI - Center for Advanced Radiation Technology, Research unit Astroparticle Physics, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, P., Abreu, M., Aglietta, E. J., Ahn, I. F. M., Albuquerque, D., Allard, I., Allekotte, J., Allen, P., Allison, J., Alvarez Castillo, J., Alvarez Muñiz, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, T., Anti??i??, A., Anzalone, Aramo, Carla, E., Arganda, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, T., Bäcker, M., Balzer, K. B., Barber, A. F., Barbosa, R., Bardenet, S. L. C., Barroso, B., Baughman, J., Bäuml, J. J., Beatty, B. R., Becker, K. H., Becker, A., Bellétoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, F., Blanco, M., Blanco, C., Bleve, H., Blümer, M., Bohá??ová, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, K. S., Caballero Mora, L., Caramete, R., Caruso, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, S. H., Cheng, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, R. W., Clay, M. R., Coluccia, R., Conceição, F., Contrera, H., Cook, M. J., Cooper, J., Coppen, A., Cordier, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., Dagoret Campagne, R., Dallier, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, I., De Mitri, V., de Souza, K. D., de Vrie, G., Decerprit, L., del Peral, M., del Río, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, J. C., Diaz, M. L., Díaz Castro, P. N., Diep, C., Dobrigkeit, W., Docter, J. C., D???olivo, P. N., Dong, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D???urso, I., Dutan, J., Ebr, R., Engel, M., Erdmann, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, I., Fajardo Tapia, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, A., Ferrero, B., Fick, A., Filevich, A., Filip??i??, S., Fliescher, C. E., Fracchiolla, E. D., Fraenkel, U., Fröhlich, B., Fuch, R., Gaior, R. F., Gamarra, S., Gambetta, B., García, D., García Gámez, D., Garcia Pinto, A., Gascon, H., Gemmeke, K., Gesterling, P. L., Ghia, U., Giaccari, M., Giller, H., Gla, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gómez Berisso, P., Gonçalve, D., Gonzalez, J. G., Gonzalez, B., Gookin, D., Góra, A., Gorgi, P., Gouffon, S. R., Gozzini, E., Grashorn, S., Grebe, N., Griffith, M., Grigat, A. F., Grillo, Y., Guardincerri, Guarino, Fausto, G. P., Guede, A., Guzman, J. D., Hague, P., Hansen, D., Harari, S., Harmsma, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, A. E., Herve, C., Hojvat, N., Hollon, V. C., Holme, P., Homola, J. R., Hörandel, A., Horneffer, M., Hrabovský, T., Huege, A., Insolia, F., Ionita, A., Italiano, C., Jarne, S., Jiraskova, M., Josebachuili, K., Kadija, K. H., Kampert, P., Karhan, P., Kasper, B., Kégl, B., Keilhauer, A., Keivani, J. L., Kelley, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, J., Knapp, D. H., Koang, K., Kotera, N., Krohm, O., Krömer, D., Kruppke Hansen, F., Kuehn, D., Kuempel, J. K., Kulbartz, N., Kunka, G., La Rosa, C., Lachaud, P., Lautridou, M. S. A. B., Leão, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Lemiere, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., López, A., Lopez Agüera, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, D., Mandat, P., Mantsch, A. G., Mariazzi, J., Marin, V., Marin, I. C., Mari, H. R., Marquez Falcon, G., Marsella, D., Martello, L., Martin, H., Martinez, O., Martínez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, P., Mertsch, C., Meurer, S., Mi??anovi??, M. I., Micheletti, W., Miller, L., Miramonti, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, E., Moreno, J. C., Moreno, C., Morri, M., Mostafá, C. A., Moura, S., Mueller, M. A., Muller, G., Müller, M., Münchmeyer, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, P. T., Nhung, L., Niemietz, N., Nierstenhoefer, D., Nitz, D., Nosek, L., No??ka, M., Nyklicek, J., Oehlschläger, A., Olinto, P., Oliva, V. M., Olmos Gilbaja, M., Ortiz, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, E., Parizot, A., Parra, R. D., Parson, S., Pastor, T., Paul, M., Pech, J., Pe¸kala, R., Pelayo, I. M., Pepe, L., Perrone, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, N., Phan, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, V. H., Ponce, M., Pontz, P., Privitera, M., Prouza, E. J., Quel, S., Querchfeld, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, H., Rivera, V., Rizi, J., Robert, C., Robledo, W., Rodrigues de Carvalho, G., Rodriguez, J., Rodriguez Martino, J., Rodriguez Rojo, I., Rodriguez Cabo, M. D., Rodríguez Fría, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouillé d???Orfeuil, E., Roulet, A. C., Rovero, C., Rühle, F., Salamida, H., Salazar, G., Salina, F., Sánchez, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, A., Schmidt, F., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovánek, F., Schröder, S., Schulte, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, H. H., Silva Lopez, A., ??mia??kowski, R., ??mída, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, S., Stanic, J., Stapleton, J., Stasielak, M., Stephan, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijärvi, A. D., Supanitsky, T., ??u??a, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, A., Tamashiro, A., Tapia, M., Tartare, O., Ta??c??u, C. G., Tavera Ruiz, R., Tcaciuc, D., Tegolo, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, D. K., Tiwari, W., Tkaczyk, C. J., Todero Peixoto, B., Tomé, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J. F., Valdés Galicia, I., Valiño, Valore, Laura, A. M., van den Berg, E., Varela, B., Vargas Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberi??, V., Verzi, J., Vicha, M., Videla, L., Villaseñor, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Walz, D., Warner, A. A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, S., Westerhoff, B. J., Whelan, G., Wieczorek, L., Wiencke, B., Wilczy??ska, H., Wilczy??ski, M., Will, C., William, T., Winchen, M. G., Winnick, M., Wommer, B., Wundheiler, T., Yamamoto, T., Yapici, P., Younk, G., Yuan, Yushkov, Alexey, B., Zamorano, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, M., Zimbres Silva, M., Ziolkowski, J., Abraham, C., Aguirre, J., Alvarez Muniz, C., Aramo, S., Argir, K., Arisaka, F., Arneodo, T., Asch, A., Bacher, T., Backer, D., Badagnani, H. J. M., Barbosa, N., Barenthien, P., Bauleo, T., Beau, A., Belletoile, O., Blanch Biga, H., Blumer, M., Bohacova, E., Bollmann, H., Bolz, F., Bracci, N. G., Busca, D., Camin, W., Carvalho, J., Castro, J., Chye, P. D. J., Clark, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, B., Connolly, A., Cordero, U., Cotti, J. W., Cronin, J., Cuautle, F., Daudo, DE MITRI, Ivan, A., Della Selva, C., Delle Fratte, J. C., D’Olivo, D., Dornic, D., D’Urso, M. A., Du Vernoi, F., Ferrer, A., Filipcic, I., Fleck, R., Fonte, W., Fulgione, R. F., Gama rra, B., Garcıa, D., Garcıa Gamez, X., Garrido, H., Geenen, G., Gelmini, H., Gemmekeai, K., Gibb, J., Gitto, L. M., Goggin, M., Gomez Berisso, P. F., Gomez Vitale, P., Goncalve, M., Goncalves do Amaral, D., Gora, V., Grassi, J., Grygar, N., Guardone, C., Guerard, F., Guarino, R., Gumbsheimer, J., Gutierrez, V., Halenka, S., Hartmann, M. D., Healy, G., Hebrero, G., Hofman, J. R., Horandel, M., Horvat, M., Hrabovsky, H., Hucker, M., Hussain, M., Iarlori, M., Kaducak, T., Karova, B., Ke, E., Kempq, H., Kern, Kleifges, M., R., Knapik, A., Kopmann, A., Krieger, O., Kromer, A., Kusenko, B. L., Lago, M. S. A. B., Leao, J., Lee, M. A., Leiguide Oliveira, M., Leuthold, R., Lopez, A., Lopez Aguera, M., Malek, F., Marchetto, Marsella, Giovanni, Martello, Daniele, O., Martineau, O., Martınez Bravo, M., Mcewen, R. R., Mcneil, R., Meyhandan, G., Miele, M., Mostafa, M., Mucchi, M. . A., Muller, F., Nerling, C., Newman Holme, D., Newton, D., Nicotra, L., Nozka, J., Oehlschlager, F., Ortolani, B., Oßwald, S., Parlati, M., Patel, V., Pavlidou, K., Payet, J., Pekala, Perrone, Lorenzo, A., Pichel, T., Pinto, O., Pisanti, J., Pochon, J., Pouryamout, L. Prado J., R., G., Raia, A., Redondo, H. C., Rei, S., Reucroft, F. A. S., Rezendem, C., Riviere, M. D., Robert, J., Ro driguez Martino, M. D., Rodrıguez Fria, B., Rouille d’Orfeuil, F., Sanchez, M., Santander, G., Schleif, T., Schmidt, P., Schovanek, F., Schroeder, F., Schussler, D., Semikoz, G., Sequiero, B. B., Siffert, A., Smiakowski, R., Smıda, A. G. K., Smith, B. E., Smith, T., Suomijarvi, A., Tamburro, T., Tarutina, O., Tascau, D., Tcherniakhovski, R., Ticona, B., Tome, I., Torre, P., Trapani, V., Tuci, E., Tusi, J. F., Valdes Galicia, I., Valino, L., Valore, J. R., Vazquez, R. A., Vazquez, D., Veberic, A., Velarde, T., Venter, L., Villasenor, G., Vitali, S., Vorobiov, L., Voyvodic, N., Wild, C., Wiebusch, B., Wilczynska, H., Wilczynski, C., Wileman, G., Worner, H., Wuac, A., Yushkov, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), APC - Astrophysique des Hautes Energies (APC - AHE), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Abreu, P., Aglietta, M., Ahn, E., Albuquerque, I., Allard, D., Allekotte, I., Allen, J., Allison, P., Alvarez Castillo, J., Alvarez-Muñiz, J., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Antičić, T., Anzalone, A., Aramo, C., Arganda, E., Arqueros, F., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Bäcker, T., Balzer, M., Barber, K., Barbosa, A., Bardenet, R., Barroso, S., Baughman, B., Bäuml, J., Beatty, J., Becker, B., Becker, K., Bellétoile, A., Bellido, J., Benzvi, S., Berat, C., Bertou, X., Biermann, P., Billoir, P., Blanco, F., Blanco, M., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brogueira, P., Brown, W., Bruijn, R., Buchholz, P., Bueno, A., Burton, R., Caballero-Mora, K., Caramete, L., Caruso, R., Castellina, A., Catalano, O., Cataldi, G., Cazon, L., Cester, R., Chauvin, J., Cheng, S., Chiavassa, A., Chinellato, J., Chou, A., Chudoba, J., Clay, R., Coluccia, M., Conceião, R., Contreras, F., Cook, H., Cooper, M., Coppens, J., Cordier, A., Coutu, S., Covault, C., Creusot, A., Criss, A., Cronin, J., Curutiu, A., Dagoret-Campagne, S., Dallier, R., Dasso, S., Daumiller, K., Dawson, B., De Almeida, R., De Domenico, M., De Donato, C., De Jong, S., De La Vega, G., De Mello Junior, W., De Mello Neto, J., De Mitri, I., De Souza, V., De Vries, K., Decerprit, G., Del Peral, L., Del Río, M., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Diaz, J., Díaz Castro, M., Diep, P., Dobrigkeit, C., Docters, W., D'Olivo, J., Dong, P., Dorofeev, A., Dos Anjos, J., Dova, M., D'Urso, D., Dutan, I., Ebr, J., Engel, R., Erdmann, M., Escobar, C., Espadanal, J., Etchegoyen, A., Facal San Luis, P., Fajardo Tapia, I., Falcke, H., Farrar, G., Fauth, A., Fazzini, N., Ferguson, A., Ferrero, A., Fick, B., Filevich, A., Filipčič, A., Fliescher, S., Fracchiolla, C., Fraenkel, E., Fröhlich, U., Fuchs, B., Gaior, R., Gamarra, R., Gambetta, S., García, B., García Gámez, D., Garcia-Pinto, D., Gascon, A., Gemmeke, H., Gesterling, K., Ghia, P., Giaccari, U., Giller, M., Glass, H., Gold, M., Golup, G., Gomez Albarracin, F., Gómez Berisso, M., 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[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Field (physics) ,Astronomy ,ultra-high energy cosmic rays ,Pierre Auger Observatory ,arrival directions ,FOS: Physical sciences ,Cosmic ray ,Astrophysics ,01 natural sciences ,Cosmic Ray ,Auger ,Position (vector) ,0103 physical sciences ,FIELD ,Pierre auger observatory ,010303 astronomy & astrophysics ,Ultra-high energy cosmic ray ,DETECTOR ,Ciencias Exactas ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Arrival directions ,010308 nuclear & particles physics ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Isotropy ,Física ,Astronomy and Astrophysics ,ASTROFÍSICA ,Ultra-high energy cosmic rays ,Magnetic field ,Experimental High Energy Physics ,Data analysis ,ComputingMethodologies_DOCUMENTANDTEXTPROCESSING ,Física nuclear ,Astrophysics - High Energy Astrophysical Phenomena ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,RAIOS CÓSMICOS ,Arrival direction ,Ultra-High Energy Cosmic Ray - Abstract
We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or ‘multiplets’) which exhibit a correlation between arrival direc- tion and the inverse of the energy. These signatures are expected from sets of events coming from the same source after having been deflected by intervening coherent magnetic fields. The observation of several events from the same source would open the possibility to accurately reconstruct the position of the source and also measure the integral of the component of the magnetic field orthogonal to the trajectory of the cos- mic rays. We describe the largest multiplets found and compute the probability that they appeared by chance from an isotropic distribution. We find no statistically significant evidence for the presence of mul- tiplets arising from magnetic deflections in the present data., Facultad de Ciencias Exactas
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- 2012
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15. The Primary Proton Spectrum of Cosmic Rays Measured with Single Hadrons at Ground Level
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T. Antoni, W. D. Apel, F. Badea, K. Bekk, A. Bercuci, H. Blumer, H. Bozdog, I. M. Brancus, C. Buttner, A. Chilingarian, K. Daumiller, P. Doll, R. Engel, J. Engler, F. Fesler, H. J. Gils, R. Glasstetter, A. Haungs, D. Heck, J. R. Horandel, K.‐H. Kampert, H. O. Klages, G. Maier, H. J. Mathes, H. J. Mayer, J. Milke, M. Muller, R. Obenland, J. Oehlschlager, S. Ostapchenko, M. Petcu, H. Rebel, A. Risse, M. Risse, M. Roth, G. Schatz, H. Schieler, J. Scholz, T. Thouw, H. Ulrich, J. van Buren, A. Vardanyan, A. Weindl, J. Wochele, and J. Zabierowski
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Physics ,Proton ,Calorimeter (particle physics) ,Astrophysics::High Energy Astrophysical Phenomena ,Hadron ,Flux ,Astronomy and Astrophysics ,Cosmic ray ,Astrophysics ,Power law ,Nuclear physics ,Atmosphere ,KASCADE ,Space and Planetary Science ,High Energy Physics::Experiment - Abstract
The flux of cosmic-ray induced single hadrons near sea level has been measured with the large hadron calorimeter of the KASCADE experiment. The measurement corroborates former results obtained with detectors of smaller size if the enlarged veto of the 304 m^2 calorimeter surface is encounted for. The program CORSIKA/QGSJET is used to compute the cosmic-ray flux above the atmosphere. Between E_0=300 GeV and 1 PeV the primary proton spectrum can be described with a power law parametrized as dJ/dE_0=(0.15+-0.03)*E_0^{-2.78+-0.03} m^-2 s^-1 sr^-1 TeV^-1. In the TeV region the proton flux compares well with the results from recent measurements of direct experiments.
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- 2004
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16. Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, E. J. Ahn, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, E. Arganda, S. Argir, K. Arisaka, F. Arneodo, F. Arqueros, T. Asch, H. Asorey, P. Assis, J. Aublin, M. Ave, G. Avila, A. Bacher, T. Backer, D. Badagnani, K. B. Barber, A. F. Barbosa, H. J. M. Barbosa, N. Barenthien, S. L. C. Barroso, B. Baughman, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, A. Belletoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, C. Bleve, H. Blumer, M. Bohacova, E. Bollmann, H. Bolz, C. Bonifazi, R. Bonino, N. Borodai, F. Bracci, J. Brack, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, D. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, J. Castro, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chudoba, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordero, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. W. Cronin, J. Cuautle, A. Curutiu, S. Dagoret Campagne, R. Dallier, F. Daudo, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, G. Decerprit, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, P. N. Diep, C. Dobrigkeit, J. C. D’Olivo, P. N. Dong, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. Du Vernois, R. Engel, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, A. Ferrero, B. Fick, A. Filevich, A. Filipcic, I. Fleck, S. Fliescher, R. Fonte, C. E. Fracchiolla, E. D. Fraenkel, W. Fulgione, R. F. Gama rra, S. Gambetta, B. Garcıa, D. Garcıa Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmekeai, P. L. Ghia, U. Giaccari, K. Gibbs, M. Giller, J. Gitto, H. Glass, L. M. Goggin, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, P. F. Gomez Vitale, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, E. Grashorn, V. Grassi, S. Grebe, M. Grigat, A. F. Grillo, J. Grygar, Y. Guardincerri, N. Guardone, C. Guerard, F. Guarino, R. Gumbsheimer, G. P. Guedes, J. Gutierrez, J. D. Hague, V. Halenka, P. Hansen, D. Harari, S. Harmsma, S. Hartmann, J. L. Harton, A. Haungs, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, G. Hofman, J. R. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, H. Hucker, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, S. Jiraskova, M. Kaducak, K. H. Kampert, T. Karova, P. Kasper, B. Ke, B. Keilhauer, E. Kempq, H. Kern, R. M. Kieckhafer, H. O. Klages, M. . Kleifges, J. Kleinfeller, R. Knapik, J. Knapp, D. H. Koang, A. Kopmann, A. Krieger, O. Kromer, D. Kruppke Hansen, D. Kuempel, N. Kunka, A. Kusenko, G. La Rosa, C. Lachaud, B. L. Lago, P. Lautridou, M. S. A. B. Leao, D. Lebrun, P. Lebrun, J. Lee, M. A. Leiguide Oliveira, A. Lemiere, A. Letessier Selvon, M. Leuthold, I. Lhenry Yvon, R. Lopez, A. Lopez Aguera, K. Louedec, J. Lozano Bahilo, A. Lucero, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, M. Malek, D. Mandat, P. Mantsch, F. Marchetto, A. G. Mariazzi, I. C. Maris, H. R. Marquez Falcon, O. Martineau, O. Martınez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurizio, P. O. Mazur, M. McEwen, R. R. McNeil, G. Medina Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, R. Meyhandan, M. I. Micheletti, G. Miele, W. Miller, L. Miramonti, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, J. C. Moreno, C. Morris, M. Mostafa, C. A. Moura, M. Mucchi, S. Mueller, M. . A. Muller, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, F. Nerling, C. Newman Holmes, D. Newton, P. T. Nhung, D. Nicotra, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nozka, M. Nyklicek, J. Oehlschlager, A. Olinto, P. Oliva, V. M. Olmos Gilbaja, M. Ortiz, F. Ortolani, B. Oßwald, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, G. Parente, E. Parizot, S. Parlati, S. Pastor, M. Patel, T. Paul, V. Pavlidou, K. Payet, M. Pech, J. Pekala, I. M. Pepe, R. Pesce, E. Petermann, S. Petrera, P. Petrinca, A. Petrolini, Y. Petrov, J. Petrovic, C. Pfendner, A. Pichel, R. Piegaia, T. Pierog, M. Pimenta, T. Pinto, V. Pirronello, O. Pisanti, M. Platino, J. Pochon, V. H. Ponce, M. Pontz, J. Pouryamout, L. Prado J.r., P. Privitera, M. Prouza, E. J. Quel, G. Raia, J. Rautenberg, O. Ravel, D. Ravignani, A. Redondo, H. C. Reis, S. Reucroft, B. Revenu, F. A. S. Rezendem, J. Ridky, S. Riggi, M. Risse, C. Riviere, V. Rizi, C. Robledo, M. D. Roberts, G. 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Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, Guarino, Fausto, D'Urso, Domenico, Valore, Laura, M., Ambrosio, Aramo, Carla, The Pierre Auger, C. o. l. l. a. b. o. r. a. t. i. o. n. ., KVI - Center for Advanced Radiation Technology, Research unit Astroparticle Physics, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Physique Nucléaire d'Orsay (IPNO), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), PIERRE AUGER, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, Abreu, P, Aglietta, M, Ahn, E.J, Albuquerque, I.F.M, Allard, D, Allekotte, I, Allen, J, Allison, P, Alvarez Castillo, J, Alvarez-Muñiz, J, Ambrosio, M, Aminaei, A, Anchordoqui, L, Andringa, S, Antičić, T, Aramo, C, Arganda, E, Arqueros, F, Asorey, H, Assis, P, Aublin, J, Ave, M, Avenier, M, Avila, G, Bäcker, T, Balzer, M, Barber, K.B, Barbosa, A.F, Bardenet, R, Barroso, S.L.C, Baughman, B, Beatty, J.J, Becker, B.R, Becker, K.H, Bellido, J.A, Benzvi, S, Berat, C, Bertou, X, Biermann, P.L, Billoir, P, Blanco, F, Blanco, M, Bleve, C, Blümer, H, Boháčová, M, Boncioli, D, Bonifazi, C, Bonino, R, Borodai, N, Brack, J, Brogueira, P, Brown, W.C, Bruijn, R, Buchholz, P, Bueno, A, Burton, R.E, Caballero-Mora, K.S, Caramete, L, Caruso, R, Castellina, A, Cataldi, G, Cazon, L, Cester, R, Chauvin, J, Chiavassa, A, Chinellato, J.A, Chou, A, Chudoba, J, Clay, R.W, Coluccia, M.R, Conceião, R, Contreras, F, Cook, H, Cooper, M.J, Coppens, J, Cordier, A, Cotti, U, Coutu, S, Covault, C.E, Creusot, A, Criss, A, Cronin, J, Curutiu, A, Dagoret-Campagne, S, Dallier, R, Dasso, S, Daumiller, K, Dawson, B.R, De Almeida, R.M, De Domenico, M, De Donato, C, De Jong, S.J, De La Vega, G, De Mello Jr, W.J.M, De Mello Neto, J.R.T, De Mitri, I, De Souza, V, De Vries, K.D, Decerprit, G, Del Peral, L, Deligny, O, Dembinski, H, Denkiewicz, A, Di Giulio, C, Diaz, J.C, Díaz Castro, M.L, Diep, P.N, Dobrigkeit, C, D'Olivo, J.C, Dong, P.N, Dorofeev, A, Dos Anjos, J.C, Dova, M.T, D'Urso, D, Dutan, I, Ebr, J, Engel, R, Erdmann, M, Escobar, C.O, Etchegoyen, A, Facal San Luis, P, Falcke, H, Farrar, G, Fauth, A.C, Fazzini, N, Ferguson, A.P, Ferrero, A, Fick, B, Filevich, A, Filipčič, A, Fliescher, S, Fracchiolla, C.E, Fraenkel, E.D, Fröhlich, U, Fuchs, B, Gamarra, R.F, Gambetta, S, García, B, García Gámez, D, Garcia-Pinto, D, Gascon, A, Gemmeke, H, Gesterling, K, Ghia, P.L, Giaccari, U, Giller, M, Glass, H, Gold, M.S, Golup, G, Gomez Albarracin, F, Gómez Berisso, M, Gonalves, P, Gonzalez, D, Gonzalez, J.G, Gookin, B, Góra, D, Gorgi, A, Gouffon, P, Gozzini, S.R, Grashorn, E, Grebe, S, Griffith, N, Grigat, M, Grillo, A.F, Guardincerri, Y, Guarino, F, Guedes, G.P, Hague, J.D, Hansen, P, Harari, D, Harmsma, S, Harton, J.L, Haungs, A, Hebbeker, T, Heck, D, Herve, A.E, Hojvat, C, Holmes, V.C, Homola, P, Hörandel, J.R, Horneffer, A, Hrabovský, M, Huege, T, Insolia, A, Ionita, F, Italiano, A, Jiraskova, S, Kadija, K, Kampert, K.H, Karhan, P, Karova, T, Kasper, P, Kégl, B, Keilhauer, B, Keivani, A, Kelley, J.L, Kemp, E, Kieckhafer, R.M, Klages, H.O, Kleifges, M, Kleinfeller, J, Knapp, J, Koang, D.-H, Kotera, K, Krohm, N, Krömer, O, Kruppke-Hansen, D, Kuehn, F, Kuempel, D, Kulbartz, J.K, Kunka, N, La Rosa, G, Lachaud, C, Lautridou, P, Leão, M.S.A.B, Lebrun, D, Lebrun, P, Leigui De Oliveira, M.A, Lemiere, A, Letessier-Selvon, A, Lhenry-Yvon, I, Link, K, López, R, Lopez Agüera, A, Louedec, K, Lozano Bahilo, J, Lucero, A, Ludwig, M, Lyberis, H, MacOlino, C, Maldera, S, Mandat, D, Mantsch, P, Mariazzi, A.G, Marin, V, Maris, I.C, Marquez Falcon, H.R, Marsella, G, Martello, D, Martin, L, Martínez Bravo, O, Mathes, H.J, Matthews, J, Matthews, J.A.J, Matthiae, G, Maurizio, D, Mazur, P.O, Medina-Tanco, G, Melissas, M, Melo, D, Menichetti, E, Menshikov, A, Mertsch, P, Meurer, C, Mićanović, S, Micheletti, M.I, Miller, W, Miramonti, L, Mollerach, S, Monasor, M, Monnier Ragaigne, D, Montanet, F, Morales, B, Morello, C, Moreno, E, Moreno, J.C, Morris, C, Mostafá, M, Moura, C.A, Mueller, S, Muller, M.A, Müller, G, Münchmeyer, M, Mussa, R, Navarra, G, Navarro, J.L, Navas, S, Necesal, P, Nellen, L, Nelles, A, Nhung, P.T, Nierstenhoefer, N, Nitz, D, Nosek, D, Nožka, L, Nyklicek, M, Oehlschläger, J, Olinto, A, Oliva, P, Olmos-Gilbaja, V.M, Ortiz, M, Pacheco, N, Pakk Selmi-Dei, D, Palatka, M, Pallotta, J, Palmieri, N, Parente, G, Parizot, E, Parra, A, Parrisius, J, Parsons, R.D, Pastor, S, Paul, T, Pech, M, Pȩkala, J, Pelayo, R, Pepe, I.M, Perrone, L, Pesce, R, Petermann, E, Petrera, S, Petrinca, P, Petrolini, A, Petrov, Y, Petrovic, J, Pfendner, C, Phan, N, Piegaia, R, Pierog, T, Pieroni, P, Pimenta, M, Pirronello, V, Platino, M, Ponce, V.H, Pontz, M, Privitera, P, Prouza, M, Quel, E.J, Rautenberg, J, Ravel, O, Ravignani, D, Revenu, B, Ridky, J, Risse, M, Ristori, P, Rivera, H, Rivire, C, Rizi, V, Robledo, C, Rodrigues De Carvalho, W, Rodriguez, G, Rodriguez Martino, J, Rodriguez Rojo, J, Rodriguez-Cabo, I, Rodríguez-Frías, M.D, Ros, G, Rosado, J, Rossler, T, Roth, M, Rouillé-D'Orfeuil, B, Roulet, E, Rovero, A.C, Rühle, C, Salamida, F, Salazar, H, Salina, G, Sánchez, F, Santander, M, Santo, C.E, Santos, E, Santos, E.M, Sarazin, F, Sarkar, S, Sato, R, Scharf, N, Scherini, V, Schieler, H, Schiffer, P, Schmidt, A, Schmidt, F, Schmidt, T, Scholten, O, Schoorlemmer, H, Schovancova, J, Schovánek, P, Schroeder, F, Schulte, S, Schuster, D, Sciutto, S.J, Scuderi, M, Segreto, A, Semikoz, D, Settimo, M, Shadkam, A, Shellard, R.C, Sidelnik, I, Sigl, G, Śmiałkowski, A, Šmída, R, Snow, G.R, Sommers, P, Sorokin, J, Spinka, H, Squartini, R, Stapleton, J, Stasielak, J, Stephan, M, Stutz, A, Suarez, F, Suomijärvi, T, Supanitsky, A.D, Šuša, T, Sutherland, M.S, Swain, J, Szadkowski, Z, Szuba, M, Tamashiro, A, Tapia, A, Tacu, O, Tcaciuc, R, Tegolo, D, Thao, N.T, Thomas, D, Tiffenberg, J, Timmermans, C, Tiwari, D.K, Tkaczyk, W, Todero Peixoto, C.J, Tomé, B, Tonachini, A, Travnicek, P, Tridapalli, D.B, Tristram, G, Trovato, E, Tueros, M, Ulrich, R, Unger, M, Urban, M, Valdés Galicia, J.F, Valiño, I, Valore, L, Van Den Berg, A.M, Vargas Cárdenas, B, Vázquez, J.R, Vázquez, R.A, Veberič, D, Verzi, V, Videla, M, Villaseñor, L, Wahlberg, H, Wahrlich, P, Wainberg, O, Warner, D, Watson, A.A, Weber, M, Weidenhaupt, K, Weindl, A, Westerhoff, S, Whelan, B.J, Wieczorek, G, Wiencke, L, Wilczyńska, B, Wilczyński, H, Will, M, Williams, C, Winchen, T, Winders, L, Winnick, M.G, Wommer, M, Wundheiler, B, Yamamoto, T, Younk, P, Yuan, G, Zamorano, B, Zas, E, Zavrtanik, D, Zavrtanik, M, Zaw, I, Zepeda, A, Ziolkowski, M., J., Abraham, P., Abreu, M., Aglietta, C., Aguirre, E. J., Ahn, D., Allard, I., Allekotte, J., Allen, P., Allison, J., Alvarez Muniz, L., Anchordoqui, S., Andringa, A., Anzalone, C., Aramo, E., Arganda, S., Argir, K., Arisaka, F., Arneodo, F., Arquero, T., Asch, H., Asorey, P., Assi, J., Aublin, M., Ave, G., Avila, A., Bacher, T., Backer, D., Badagnani, K. B., Barber, A. F., Barbosa, H. J. M., Barbosa, N., Barenthien, S. L. C., Barroso, B., Baughman, P., Bauleo, J. J., Beatty, T., Beau, B. R., Becker, K. H., Becker, A., Belletoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, O., Blanch Biga, F., Blanco, C., Bleve, H., Blumer, M., Bohacova, E., Bollmann, H., Bolz, C., Bonifazi, R., Bonino, N., Borodai, F., Bracci, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, N. G., Busca, K. S., Caballero Mora, D., Camin, L., Caramete, R., Caruso, W., Carvalho, A., Castellina, J., Castro, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, J., Chye, P. D. J., Clark, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, B., Connolly, F., Contrera, J., Coppen, A., Cordero, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J. W., Cronin, J., Cuautle, A., Curutiu, S., Dagoret Campagne, R., Dallier, F., Daudo, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, G., Decerprit, L., del Peral, O., Deligny, A., Della Selva, C., Delle Fratte, H., Dembinski, C., Di Giulio, J. C., Diaz, P. N., Diep, C., Dobrigkeit, J. C., D’Olivo, P. N., Dong, D., Dornic, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, I., Dutan, M. A., Du Vernoi, R., Engel, M., Erdmann, C. O., Escobar, A., Etchegoyen, P., Facal San Lui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, F., Ferrer, A., Ferrero, B., Fick, A., Filevich, A., Filipcic, I., Fleck, S., Fliescher, R., Fonte, C. E., Fracchiolla, E. D., Fraenkel, W., Fulgione, R. F., Gama rra, S., Gambetta, B., Garcıa, D., Garcıa Gamez, D., Garcia Pinto, X., Garrido, H., Geenen, G., Gelmini, H., Gemmekeai, P. L., Ghia, U., Giaccari, K., Gibb, M., Giller, J., Gitto, H., Gla, L. M., Goggin, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gomez Berisso, P. F., Gomez Vitale, P., Goncalve, M., Goncalves do Amaral, D., Gonzalez, J. G., Gonzalez, D., Gora, A., Gorgi, P., Gouffon, E., Grashorn, V., Grassi, S., Grebe, M., Grigat, A. F., Grillo, J., Grygar, Y., Guardincerri, N., Guardone, C., Guerard, F., Guarino, R., Gumbsheimer, G. P., Guede, J., Gutierrez, J. D., Hague, V., Halenka, P., Hansen, D., Harari, S., Harmsma, S., Hartmann, J. L., Harton, A., Haung, M. D., Healy, T., Hebbeker, G., Hebrero, D., Heck, C., Hojvat, V. C., Holme, P., Homola, G., Hofman, J. R., Horandel, A., Horneffer, M., Horvat, M., Hrabovsky, H., Hucker, T., Huege, M., Hussain, M., Iarlori, A., Insolia, F., Ionita, A., Italiano, S., Jiraskova, M., Kaducak, K. H., Kampert, T., Karova, P., Kasper, B., Ke, B., Keilhauer, E., Kempq, H., Kern, R. M., Kieckhafer, H. O., Klage, Kleifges, M., J., Kleinfeller, R., Knapik, J., Knapp, D. H., Koang, A., Kopmann, A., Krieger, O., Kromer, D., Kruppke Hansen, D., Kuempel, N., Kunka, A., Kusenko, G., La Rosa, C., Lachaud, B. L., Lago, P., Lautridou, M. S. A. B., Leao, D., Lebrun, P., Lebrun, J., Lee, M. A., Leiguide Oliveira, A., Lemiere, A., Letessier Selvon, M., Leuthold, I., Lhenry Yvon, R., Lopez, A., Lopez Aguera, K., Louedec, J., Lozano Bahilo, A., Lucero, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, M., Malek, D., Mandat, P., Mantsch, F., Marchetto, A. G., Mariazzi, I. C., Mari, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, O., Martineau, O., Martınez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, M., Mcewen, R. R., Mcneil, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, R., Meyhandan, M. I., Micheletti, G., Miele, W., Miller, L., Miramonti, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, J. C., Moreno, C., Morri, M., Mostafa, C. A., Moura, M., Mucchi, S., Mueller, M. . A., Muller, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, F., Nerling, C., Newman Holme, D., Newton, P. T., Nhung, D., Nicotra, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nozka, M., Nyklicek, J., Oehlschlager, A., Olinto, P., Oliva, V. M., Olmos Gilbaja, M., Ortiz, F., Ortolani, B., Oßwald, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, G., Parente, E., Parizot, S., Parlati, S., Pastor, M., Patel, T., Paul, V., Pavlidou, K., Payet, M., Pech, J., Pekala, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, A., Pichel, R., Piegaia, T., Pierog, M., Pimenta, T., Pinto, V., Pirronello, O., Pisanti, M., Platino, J., Pochon, V. H., Ponce, M., Pontz, J., Pouryamout, L. Prado J., R., P., Privitera, M., Prouza, E. J., Quel, G., Raia, J., Rautenberg, O., Ravel, D., Ravignani, A., Redondo, H. C., Rei, S., Reucroft, B., Revenu, F. A. S., Rezendem, J., Ridky, S., Riggi, M., Risse, C., Riviere, V., Rizi, C., Robledo, M. D., Robert, G., Rodriguez, J., Ro driguez Martino, J., Rodriguez Rojo, I., Rodriguez Cabo, M. D., Rodrıguez Fria, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouille d’Orfeuil, E., Roulet, A. C., Rovero, F., Salamida, H., Salazar, G., Salina, F., Sanchez, M., Santander, C. E., Santo, E. M., Santo, F., Sarazin, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, G., Schleif, A., Schmidt, F., Schmidt, T., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovanek, F., Schroeder, S., Schulte, F., Schussler, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, D., Semikoz, G., Sequiero, M., Settimo, R. C., Shellard, I., Sidelnik, B. B., Siffert, A., Smiakowski, R., Smıda, A. G. K., Smith, B. E., Smith, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijarvi, A. D., Supanitsky, M. S., Sutherland, J., Swain, Z., Szadkowski, A., Tamashiro, A., Tamburro, T., Tarutina, O., Tascau, R., Tcaciuc, D., Tcherniakhovski, N. T., Thao, D., Thoma, R., Ticona, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, B., Tome, A., Tonachini, I., Torre, P., Trapani, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, V., Tuci, M., Tuero, E., Tusi, R., Ulrich, M., Unger, M., Urban, J. F., Valdes Galicia, I., Valino, L., Valore, A. M., van den Berg, J. R., Vazquez, R. A., Vazquez, D., Veberic, A., Velarde, T., Venter, V., Verzi, M., Videla, L., Villasenor, G., Vitali, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, S., Westerhoff, B. J., Whelan, N., Wild, C., Wiebusch, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., Wileman, M. G., Winnick, G., Worner, H., Wuac, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, M., Ziolkowski, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik
- Subjects
Large scale anisotripies ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Auger Experiment ,Astronomy ,Astrophysics::High Energy Astrophysical Phenomena ,Phase (waves) ,FOS: Physical sciences ,Cosmic ray ,Astrophysics ,anisotropy ,SURFACE DETECTOR ,01 natural sciences ,Cosmic Ray ,Auger ,Large scale anisotropies ,Observatory ,Large scale anisotropie ,0103 physical sciences ,010303 astronomy & astrophysics ,Ultra-high energy cosmic ray ,Ciencias Exactas ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Pierre Auger Observatory ,FÍSICA DE PARTÍCULAS ,Ultra High Energy Cosmic Rays ,010308 nuclear & particles physics ,ORIGIN ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Astrophysics::Instrumentation and Methods for Astrophysics ,Física ,Astronomy and Astrophysics ,Ultra-high energy cosmic rays ,ENERGY-SPECTRUM ,Radiación cósmica ,Anisotropía ,Amplitude ,Harmonics ,Experimental High Energy Physics ,ComputingMethodologies_DOCUMENTANDTEXTPROCESSING ,ARRAY ,Física nuclear ,Right ascension ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations., We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Ministério de Ciência e Tecnologia (MCT), Brazil; AVCR, AV0Z10100502 and AV0Z10100522, GAAV, KJB300100801 and KJB100100904, MSMT-CRLA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l’Univers (SDU-INSU/CNRS), France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden – Württemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung,Nordrhein-Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-Württemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Astrofisica (INAF), Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR), Gran Sasso Center for Astroparticle Physics (CFA), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. 1 P03 D 014 30 and N N202 207238, Poland; Fundação para a Ciência e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejería de Educación de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovación and Consolider-Ingenio 2010 (CPAN), Generalitat Valenciana, Junta de Andalucía, Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract Nos. DE-AC02-07CH11359, DE-FR02-04ER41300, National Science Foundation, Grant No. 0450696, The Grainger Foundation, USA; ALFA-EC/ HELEN, European Union 6th Framework Program, Grant No. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO.
- Published
- 2011
- Full Text
- View/download PDF
17. Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory
- Author
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, E. J. Ahn, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, E. Arganda, S. Argir, K. Arisaka, F. Arneodo, F. Arqueros, T. Asch, H. Asorey, P. Assis, J. Aublin, M. Ave, G. Avila, A. Bacher, T. Backer, D. Badagnani, K. B. Barber, A. F. Barbosa, H. J. M. Barbosa, N. Barenthien, S. L. C. Barroso, B. Baughman, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, A. Belletoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, C. Bleve, H. Blumer, M. Bohacova, E. Bollmann, H. Bolz, C. Bonifazi, R. Bonino, N. Borodai, F. Bracci, J. Brack, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, D. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, J. Castro, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chudoba, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordero, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. W. Cronin, J. Cuautle, A. Curutiu, S. Dagoret Campagne, R. Dallier, F. Daudo, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, G. Decerprit, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, P. N. Diep, C. Dobrigkeit, J. C. D’Olivo, P. N. Dong, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. Du Vernois, R. Engel, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, A. Ferrero, B. Fick, A. Filevich, A. Filipcic, I. Fleck, S. Fliescher, R. Fonte, C. E. Fracchiolla, E. D. Fraenkel, W. Fulgione, R. F. Gama rra, S. Gambetta, B. Garcıa, D. Garcıa Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmekeai, P. L. Ghia, U. Giaccari, K. Gibbs, M. Giller, J. Gitto, H. Glass, L. M. Goggin, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, P. F. Gomez Vitale, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, E. Grashorn, V. Grassi, S. Grebe, M. Grigat, A. F. Grillo, J. Grygar, Y. Guardincerri, N. Guardone, C. Guerard, F. Guarino, R. Gumbsheimer, G. P. Guedes, J. Gutierrez, J. D. Hague, V. Halenka, P. Hansen, D. Harari, S. Harmsma, S. Hartmann, J. L. Harton, A. Haungs, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, G. Hofman, J. R. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, H. Hucker, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, S. Jiraskova, M. Kaducak, K. H. Kampert, T. Karova, P. Kasper, B. Ke, B. Keilhauer, E. Kempq, H. Kern, R. M. Kieckhafer, H. O. Klages, M. . Kleifges, J. Kleinfeller, R. Knapik, J. Knapp, D. H. Koang, A. Kopmann, A. Krieger, O. Kromer, D. Kruppke Hansen, D. Kuempel, N. Kunka, A. Kusenko, G. La Rosa, C. Lachaud, B. L. Lago, P. Lautridou, M. S. A. B. Leao, D. Lebrun, P. Lebrun, J. Lee, M. A. Leiguide Oliveira, A. Lemiere, A. Letessier Selvon, M. Leuthold, I. Lhenry Yvon, R. Lopez, A. Lopez Aguera, K. Louedec, J. Lozano Bahilo, A. Lucero, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, M. Malek, D. Mandat, P. Mantsch, F. Marchetto, A. G. Mariazzi, I. C. Maris, H. R. Marquez Falcon, O. Martineau, O. Martınez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurizio, P. O. Mazur, M. McEwen, R. R. McNeil, G. Medina Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, R. Meyhandan, M. I. Micheletti, G. Miele, W. Miller, L. Miramonti, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, J. C. Moreno, C. Morris, M. Mostafa, C. A. Moura, M. Mucchi, S. Mueller, M. . A. Muller, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, F. Nerling, C. Newman Holmes, D. Newton, P. T. Nhung, D. Nicotra, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nozka, M. Nyklicek, J. Oehlschlager, A. Olinto, P. Oliva, V. M. Olmos Gilbaja, M. Ortiz, F. Ortolani, B. Oßwald, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, G. Parente, E. Parizot, S. Parlati, S. Pastor, M. Patel, T. Paul, V. Pavlidou, K. Payet, M. Pech, J. Pekala, I. M. Pepe, R. Pesce, E. Petermann, S. Petrera, P. Petrinca, A. Petrolini, Y. Petrov, J. Petrovic, C. Pfendner, A. Pichel, R. Piegaia, T. Pierog, M. Pimenta, T. Pinto, V. Pirronello, O. Pisanti, M. Platino, J. Pochon, V. H. Ponce, M. Pontz, J. Pouryamout, L. Prado J.r., P. Privitera, M. Prouza, E. J. Quel, G. Raia, J. Rautenberg, O. Ravel, D. Ravignani, A. Redondo, H. C. Reis, S. Reucroft, B. Revenu, F. A. S. Rezendem, J. Ridky, S. Riggi, M. Risse, C. Riviere, V. Rizi, C. Robledo, M. D. Roberts, G. Rodriguez, J. Ro driguez Martino, J. Rodriguez Rojo, I. Rodriguez Cabo, M. D. Rodrıguez Frias, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouille d’Orfeuil, E. Roulet, A. C. Rovero, F. Salamida, H. Salazar, G. Salina, F. Sanchez, M. Santander, C. E. Santo, E. M. Santos, F. Sarazin, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, G. Schleif, A. Schmidt, F. Schmidt, T. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovanek, F. Schroeder, S. Schulte, F. Schussler, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, D. Semikoz, G. Sequieros, M. Settimo, R. C. Shellard, I. Sidelnik, B. B. Siffert, A. Smiakowski, R. Smıda, A. G. K. Smith, B. E. Smith, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, E. Strazzeri, A. Stutz, F. Suarez, T. Suomijarvi, A. D. Supanitsky, M. S. Sutherland, J. Swain, Z. Szadkowski, A. Tamashiro, A. Tamburro, T. Tarutina, O. Tascau, R. Tcaciuc, D. Tcherniakhovski, N. T. Thao, D. Thomas, R. Ticona, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, B. Tome, A. Tonachini, I. Torres, P. Trapani, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, V. Tuci, M. Tueros, E. Tusi, R. Ulrich, M. Unger, M. Urban, J. F. Valdes Galicia, I. Valino, L. Valore, A. M. van den Berg, J. R. Vazquez, R. A. Vazquez, D. Veberic, A. Velarde, T. Venters, V. Verzi, M. Videla, L. Villasenor, G. Vitali, S. Vorobiov, L. Voyvodic, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Warner, S. Westerhoff, B. J. Whelan, N. Wild, C. Wiebusch, G. Wieczorek, L. Wiencke, B. Wilczynska, H. Wilczynski, C. Wileman, M. G. Winnick, G. Worner, H. Wuac, B. Wundheiler, T. Yamamoto, P. Younk, G. Yuan, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, M. Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, Guarino, Fausto, Valore, Laura, D'Urso, Domenico, Yushkov, Alexey, Aramo, Carla, The Pierre Auger, Collaboration, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, J., Abraham, P., Abreu, M., Aglietta, C., Aguirre, E. J., Ahn, D., Allard, I., Allekotte, J., Allen, P., Allison, J., Alvarez Muniz, M., Ambrosio, L., Anchordoqui, S., Andringa, A., Anzalone, C., Aramo, E., Arganda, S., Argir, K., Arisaka, F., Arneodo, F., Arquero, T., Asch, H., Asorey, P., Assi, J., Aublin, M., Ave, G., Avila, A., Bacher, T., Backer, D., Badagnani, K. B., Barber, A. F., Barbosa, H. J. M., Barbosa, N., Barenthien, S. L. C., Barroso, B., Baughman, P., Bauleo, J. J., Beatty, T., Beau, B. R., Becker, K. H., Becker, A., Belletoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, O., Blanch Biga, F., Blanco, C., Bleve, H., Blumer, M., Bohacova, E., Bollmann, H., Bolz, C., Bonifazi, R., Bonino, N., Borodai, F., Bracci, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, N. G., Busca, K. S., Caballero Mora, D., Camin, L., Caramete, R., Caruso, W., Carvalho, A., Castellina, J., Castro, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, J., Chye, P. D. J., Clark, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, B., Connolly, F., Contrera, J., Coppen, A., Cordero, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J. W., Cronin, J., Cuautle, A., Curutiu, S., Dagoret Campagne, R., Dallier, F., Daudo, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, G., Decerprit, L., del Peral, O., Deligny, A., Della Selva, C., Delle Fratte, H., Dembinski, C., Di Giulio, J. C., Diaz, P. N., Diep, C., Dobrigkeit, J. C., D’Olivo, P. N., Dong, D., Dornic, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, I., Dutan, M. A., Du Vernoi, R., Engel, M., Erdmann, C. O., Escobar, A., Etchegoyen, P., Facal San Lui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, F., Ferrer, A., Ferrero, B., Fick, A., Filevich, A., Filipcic, I., Fleck, S., Fliescher, R., Fonte, C. E., Fracchiolla, E. D., Fraenkel, W., Fulgione, R. F., Gama rra, S., Gambetta, B., Garcıa, D., Garcıa Gamez, D., Garcia Pinto, X., Garrido, H., Geenen, G., Gelmini, H., Gemmekeai, P. L., Ghia, U., Giaccari, K., Gibb, M., Giller, J., Gitto, H., Gla, L. M., Goggin, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gomez Berisso, P. F., Gomez Vitale, P., Goncalve, M., Goncalves do Amaral, D., Gonzalez, J. G., Gonzalez, D., Gora, A., Gorgi, P., Gouffon, E., Grashorn, V., Grassi, S., Grebe, M., Grigat, A. F., Grillo, J., Grygar, Y., Guardincerri, N., Guardone, C., Guerard, F., Guarino, R., Gumbsheimer, G. P., Guede, J., Gutierrez, J. D., Hague, V., Halenka, P., Hansen, D., Harari, S., Harmsma, S., Hartmann, J. L., Harton, A., Haung, M. D., Healy, T., Hebbeker, G., Hebrero, D., Heck, C., Hojvat, V. C., Holme, P., Homola, G., Hofman, J. R., Horandel, A., Horneffer, M., Horvat, M., Hrabovsky, H., Hucker, T., Huege, M., Hussain, M., Iarlori, A., Insolia, F., Ionita, A., Italiano, S., Jiraskova, M., Kaducak, K. H., Kampert, T., Karova, P., Kasper, B., Ke, B., Keilhauer, E., Kempq, H., Kern, R. M., Kieckhafer, H. O., Klage, Kleifges, M., J., Kleinfeller, R., Knapik, J., Knapp, D. H., Koang, A., Kopmann, A., Krieger, O., Kromer, D., Kruppke Hansen, D., Kuempel, N., Kunka, A., Kusenko, G., La Rosa, C., Lachaud, B. L., Lago, P., Lautridou, M. S. A. B., Leao, D., Lebrun, P., Lebrun, J., Lee, M. A., Leiguide Oliveira, A., Lemiere, A., Letessier Selvon, M., Leuthold, I., Lhenry Yvon, R., Lopez, A., Lopez Aguera, K., Louedec, J., Lozano Bahilo, A., Lucero, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, M., Malek, D., Mandat, P., Mantsch, F., Marchetto, A. G., Mariazzi, I. C., Mari, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, O., Martineau, O., Martınez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, M., Mcewen, R. R., Mcneil, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, R., Meyhandan, M. I., Micheletti, G., Miele, W., Miller, L., Miramonti, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, J. C., Moreno, C., Morri, M., Mostafa, C. A., Moura, M., Mucchi, S., Mueller, M. . A., Muller, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, F., Nerling, C., Newman Holme, D., Newton, P. T., Nhung, D., Nicotra, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nozka, M., Nyklicek, J., Oehlschlager, A., Olinto, P., Oliva, V. M., Olmos Gilbaja, M., Ortiz, F., Ortolani, B., Oßwald, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, G., Parente, E., Parizot, S., Parlati, S., Pastor, M., Patel, T., Paul, V., Pavlidou, K., Payet, M., Pech, J., Pekala, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, A., Pichel, R., Piegaia, T., Pierog, M., Pimenta, T., Pinto, V., Pirronello, O., Pisanti, M., Platino, J., Pochon, V. H., Ponce, M., Pontz, J., Pouryamout, L. Prado J., R., P., Privitera, M., Prouza, E. J., Quel, G., Raia, J., Rautenberg, O., Ravel, D., Ravignani, A., Redondo, H. C., Rei, S., Reucroft, B., Revenu, F. A. S., Rezendem, J., Ridky, S., Riggi, M., Risse, C., Riviere, V., Rizi, C., Robledo, M. D., Robert, G., Rodriguez, J., Ro driguez Martino, J., Rodriguez Rojo, I., Rodriguez Cabo, M. D., Rodrıguez Fria, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouille d’Orfeuil, E., Roulet, A. C., Rovero, F., Salamida, H., Salazar, G., Salina, F., Sanchez, M., Santander, C. E., Santo, E. M., Santo, F., Sarazin, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, G., Schleif, A., Schmidt, F., Schmidt, T., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovanek, F., Schroeder, S., Schulte, F., Schussler, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, D., Semikoz, G., Sequiero, M., Settimo, R. C., Shellard, I., Sidelnik, B. B., Siffert, A., Smiakowski, R., Smıda, A. G. K., Smith, B. E., Smith, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijarvi, A. D., Supanitsky, M. S., Sutherland, J., Swain, Z., Szadkowski, A., Tamashiro, A., Tamburro, T., Tarutina, O., Tascau, R., Tcaciuc, D., Tcherniakhovski, N. T., Thao, D., Thoma, R., Ticona, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, B., Tome, A., Tonachini, I., Torre, P., Trapani, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, V., Tuci, M., Tuero, E., Tusi, R., Ulrich, M., Unger, M., Urban, J. F., Valdes Galicia, I., Valino, L., Valore, A. M., van den Berg, J. R., Vazquez, R. A., Vazquez, D., Veberic, A., Velarde, T., Venter, V., Verzi, M., Videla, L., Villasenor, G., Vitali, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, S., Westerhoff, B. J., Whelan, N., Wild, C., Wiebusch, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., Wileman, M. G., Winnick, G., Worner, H., Wuac, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, M., Ziolkowski, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Pierre et Marie Curie - Paris 6 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Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Abreu, P., Aglietta, M., Ahn, E., Albuquerque, I., Allard, D., Allekotte, I., Allen, J., Allison, P., Alvarez Castillo, J., Alvarez-Muñiz, J., Ambrosio, M., Aminaei, A., Anchordoqui, L., Andringa, S., Antičić, T., Anzalone, A., Aramo, C., Arganda, E., Arqueros, F., Asorey, H., Assis, P., Aublin, J., Ave, M., Avenier, M., Avila, G., Bäcker, T., Balzer, M., Barber, K., Barbosa, A., Bardenet, R., Barroso, S., Baughman, B., Bäuml, J., Beatty, J., Becker, B., Becker, K., Bellétoile, A., Bellido, J., Benzvi, S., Berat, C., Bertou, X., Biermann, P., Billoir, P., Blanco, F., Blanco, M., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brogueira, P., Brown, W., Bruijn, R., Buchholz, P., Bueno, A., Burton, R., Caballero-Mora, K., Caramete, L., Caruso, R., Castellina, A., Catalano, O., Cataldi, G., Cazon, L., Cester, R., Chauvin, J., Cheng, S., Chiavassa, A., Chinellato, J., Chou, A., Chudoba, J., Clay, R., Coluccia, M., Conceição, R., Contreras, F., Cook, H., Cooper, M., Coppens, J., Cordier, A., Coutu, S., Covault, C., Creusot, A., Criss, A., Cronin, J., Curutiu, A., Dagoret-Campagne, S., Dallier, R., Dasso, S., Daumiller, K., Dawson, B., De Almeida, R., De Domenico, M., De Donato, C., De Jong, S., De La Vega, G., De Mello Junior, W., De Mello Neto, J., De Mitri, I., De Souza, V., De Vries, K., Decerprit, G., Del Peral, L., Del Río, M., Deligny, O., Dembinski, H., Dhital, N., Di Giulio, C., Diaz, J., Díaz Castro, M., Diep, P., Dobrigkeit, C., Docters, W., D'Olivo, J., Dong, P., Dorofeev, A., Dos Anjos, J., Dova, M., D'Urso, D., Dutan, I., Ebr, J., Engel, R., Erdmann, M., Escobar, C., Espadanal, J., Etchegoyen, A., Facal San Luis, P., Fajardo Tapia, I., Falcke, H., Farrar, G., Fauth, A., Fazzini, N., Ferguson, A., Ferrero, A., Fick, B., Filevich, A., Filipčič, A., Fliescher, S., Fracchiolla, C., Fraenkel, E., Fröhlich, U., Fuchs, B., Gaior, R., Gamarra, R., Gambetta, S., García, B., García Gámez, D., Garcia-Pinto, D., Gascon, A., Gemmeke, H., Gesterling, K., Ghia, P., Giaccari, U., Giller, M., Glass, H., Gold, M., Golup, G., Gomez Albarracin, F., Gómez Berisso, M., Gonçalves, P., Gonzalez, D., Gonzalez, J., Gookin, B., Góra, D., Gorgi, A., Gouffon, P., Gozzini, S., Grashorn, E., Grebe, S., Griffith, N., Grigat, M., Grillo, A., Guardincerri, Y., Guarino, F., Guedes, G., Guzman, A., Hague, J., Hansen, P., Harari, D., Harmsma, S., Harrison, T., Harton, J., Haungs, A., Hebbeker, T., Heck, D., Herve, A., Hojvat, C., Hollon, N., Holmes, V., Homola, P., Hörandel, J., Horneffer, A., Horvath, P., Hrabovský, M., Huege, T., Insolia, A., Ionita, F., Italiano, A., Jarne, C., Jiraskova, S., Josebachuili, M., Kadija, K., Kampert, K., Karhan, P., Kasper, P., Kégl, B., Keilhauer, B., Keivani, A., Kelley, J., Kemp, E., Kieckhafer, R., Klages, H., Kleinfeller, J., Knapp, J., Koang, D., Kotera, K., Krohm, N., Krömer, O., Kruppke-Hansen, D., Kuehn, F., Kuempel, D., Kulbartz, J., Kunka, N., Rosa, G., Lachaud, C., Lautridou, P., Leão, M., Lebrun, D., Lebrun, P., Leigui De Oliveira, M., Lemiere, A., Letessier-Selvon, A., Lhenry-Yvon, I., Link, K., López, R., Lopez Agüera, A., Louedec, K., Lozano Bahilo, J., Lu, L., Lucero, A., Ludwig, M., Lyberis, H., Maccarone, M., Macolino, C., Maldera, S., Mandat, D., Mantsch, P., Mariazzi, A., Marin, J., Marin, V., Maris, I., Marquez Falcon, H., Marsella, G., Martello, D., Martin, L., Martinez, H., Martínez Bravo, O., Mathes, H., Matthews, J., Matthiae, G., Maurizio, D., Mazur, P., Medina-Tanco, G., Melissas, M., Melo, D., Menichetti, E., Menshikov, A., Mertsch, P., Meurer, C., Mićanović, S., Micheletti, M., Miller, W., Miramonti, L., Molina-Bueno, L., Mollerach, S., Monasor, M., Monnier Ragaigne, D., Montanet, F., Morales, B., Morello, C., Moreno, E., Moreno, J., Morris, C., Mostafá, M., Moura, C., Mueller, S., Muller, M., Müller, G., Münchmeyer, M., Mussa, R., Navarra, G., Navarro, J., Navas, S., Necesal, P., Nellen, L., Nelles, A., Neuser, J., Newton, D., Nhung, P., Niemietz, L., Nierstenhoefer, N., Nitz, D., Nosek, D., Noka, L., Nyklicek, M., Oehlschläger, J., Olinto, A., Oliva, P., Olmos-Gilbaja, V., Ortiz, M., Pacheco, N., Pakk Selmi-Dei, D., Palatka, M., Pallotta, J., Palmieri, N., Parente, G., Parizot, E., Parra, A., Parsons, R., Pastor, S., Paul, T., Pech, M., Pekala, J., Pelayo, R., Pepe, I., Perrone, L., Pesce, R., Petermann, E., Petrera, S., Petrinca, P., Petrolini, A., Petrov, Y., Petrovic, J., Pfendner, C., Phan, N., Piegaia, R., Pierog, T., Pieroni, P., Pimenta, M., Pirronello, V., Platino, M., Ponce, V., Pontz, M., Privitera, P., Prouza, M., Quel, E., Querchfeld, S., Rautenberg, J., Ravel, O., Ravignani, D., Revenu, B., Ridky, J., Riggi, S., Risse, M., Ristori, P., Rivera, H., Rizi, V., Roberts, J., Robledo, C., Rodrigues De Carvalho, W., Rodriguez, G., Rodriguez Martino, J., Rodriguez Rojo, J., Rodriguez-Cabo, I., Rodríguez-Frías, M., Ros, G., Rosado, J., Rossler, T., Roth, M., Rouillé-D'Orfeuil, B., Roulet, E., Rovero, A., Rühle, C., Salamida, F., Salazar, H., Salesa Greus, F., Salina, G., Sánchez, F., Santo, C., Santos, E., Sarazin, F., Sarkar, B., Sarkar, S., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Schmidt, F., Scholten, O., Schoorlemmer, H., Schovancova, J., Schovánek, P., Schröder, F., Schulte, S., Schuster, D., Sciutto, S., Scuderi, M., Segreto, A., Settimo, M., Shadkam, A., Shellard, R., Sidelnik, I., Sigl, G., Silva Lopez, H., Amiałkowski, A., Amída, R., Snow, G., Sommers, P., Sorokin, J., Spinka, H., Squartini, R., Stanic, S., Stapleton, J., Stasielak, J., Stephan, M., Strazzeri, E., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A., Aua, T., Sutherland, M., Swain, J., Szadkowski, Z., Szuba, M., Tamashiro, A., Tapia, A., Tartare, M., Taşcau, O., Tavera Ruiz, C., Tcaciuc, R., Tegolo, D., Thao, N., Thomas, D., Tiffenberg, J., Timmermans, C., Tiwari, D., Tkaczyk, W., Todero Peixoto, C., Tomé, B., Tonachini, A., Travnicek, P., Tridapalli, D., Tristram, G., Trovato, E., Tueros, M., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J., Valiño, I., Valore, L., Van Den Berg, A., Varela, E., Vargas Cárdenas, B., Vázquez, J., Vázquez, R., Veberič, D., Verzi, V., Vicha, J., Videla, M., Villaseñor, L., Wahlberg, H., Wahrlich, P., Wainberg, O., Walz, D., Warner, D., Watson, A., Weber, M., Weidenhaupt, K., Weindl, A., Westerhoff, S., Whelan, B., Wieczorek, G., Wiencke, L., Wilczyńska, B., Wilczyński, H., Will, M., Williams, C., Winchen, T., Winnick, M., Wommer, M., Wundheiler, B., Yamamoto, T., Yapici, T., Younk, P., Yuan, G., Yushkov, A., Zamorano, B., Zas, E., Zavrtanik, D., Zavrtanik, M., Zaw, I., Zepeda, A., Zimbres Silva, M., Ziolkowski, M., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), KVI - Center for Advanced Radiation Technology, and Research unit Astroparticle Physics
- Subjects
Physics::Instrumentation and Detectors ,Solar neutrino ,Astrophysics ,UPPER LIMIT ,PHOTON FRACTION ,01 natural sciences ,7. Clean energy ,neutrino ,Observatory ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,ORIGIN ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,pion ,Astrophysics::Instrumentation and Methods for Astrophysics ,Pierre Auger Observatory ,COSMIC-RAYS ,cosmic ray detectors ,and other elementary particle detectors ,Cosmic neutrino background ,NEUTRINOS ,Física nuclear ,Neutrino ,Astrophysics - High Energy Astrophysical Phenomena ,FLUX ,FERMI-LAT ,Nuclear and High Energy Physics ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,TELESCOPE ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Cosmic ray ,EXTENSIVE AIR-SHOWERS ,SURFACE DETECTOR ,Cosmic Ray ,Pion ,muon ,0103 physical sciences ,010306 general physics ,Cosmic rays ,Muon ,010308 nuclear & particles physics ,Física ,and other elementary particles ,Ultra-high energy cosmic rays ,PERFORMANCE ,neutrino flavor ,air showers ,surface detector ,observatory ,atmosphere ,Auger ,cosmic radiation ,energy spectrum ,13. Climate action ,High Energy Physics::Experiment - Abstract
Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902], The Surface Detector of the Pierre Auger Observatory is sensitive to neutrinos of all flavours above 0.1 EeV. These interact through charged and neutral currents in the atmosphere giving rise to extensive air showers. When interacting deeply in the atmosphere at nearly horizontal incidence, neutrinos can be distinguished from regular hadronic cosmic rays by the broad time structure of their shower signals in the water-Cherenkov detectors. In this paper we present for the first time an analysis based on down-going neutrinos. We describe the search procedure, the possible sources of background, the method to compute the exposure and the associated systematic uncertainties. No candidate neutrinos have been found in data collected from 1 January 2004 to 31 May 2010. Assuming an E^-2 differential energy spectrum the limit on the single flavour neutrino is (E^2 * dN/dE) < 1.74x10^-7 GeV cm^-2 s^-1 sr^-1 at 90% C.L. in the energy range 1x10^17 eV < E < 1x10^20 eV., We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundaçao de Amparo à Pesquisa do Estado de Rio de Janeiro(FAPERJ), Fundaçao de Amparo à Pesquisa do Estado de Sao Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB100100904, MSMT-CRLA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l’Univers (SDU-INSU/CNRS), France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Württemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden- Württemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. 1 P03 D 014 30, N202 090 31/0623, and PAP/218/2006, Poland; Fundaçao para a Ciencia e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejería de Educación de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovación and Consolider-Ingenio 2010 (CPAN), Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract Nos. DEAC02-07CH11359, DE-FR02-04ER41300, National Science Foundation, Grant No. 0450696, The Grainger Foundation USA; ALFA-EC / HELEN, European Union 6th Framework Program, Grant No. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO.
- Published
- 2011
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18. Anisotropy and chemical compositionof ultra-high energy cosmic rays usingarrival directions measured by thePierre Auger Observatory
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, E. J. Ahn, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, E. Arganda, S. Argir, K. Arisaka, F. Arneodo, F. Arqueros, T. Asch, H. Asorey, P. Assis, J. Aublin, M. Ave, G. Avila, A. Bacher, T. Backer, D. Badagnani, K. B. Barber, A. F. Barbosa, H. J. M. Barbosa, N. Barenthien, S. L. C. Barroso, B. Baughman, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, A. Belletoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, C. Bleve, H. Blumer, M. Bohacova, E. Bollmann, H. Bolz, C. Bonifazi, R. Bonino, N. Borodai, F. Bracci, J. Brack, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, D. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, J. Castro, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chudoba, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordero, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. W. Cronin, J. Cuautle, A. Curutiu, S. Dagoret Campagne, R. Dallier, F. Daudo, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, G. Decerprit, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, P. N. Diep, C. Dobrigkeit, J. C. D’Olivo, P. N. Dong, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. Du Vernois, R. Engel, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, A. Ferrero, B. Fick, A. Filevich, A. Filipcic, I. Fleck, S. Fliescher, R. Fonte, C. E. Fracchiolla, E. D. Fraenkel, W. Fulgione, R. F. Gama rra, S. Gambetta, B. Garcıa, D. Garcıa Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmekeai, P. L. Ghia, U. Giaccari, K. Gibbs, M. Giller, J. Gitto, H. Glass, L. M. Goggin, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, P. F. Gomez Vitale, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, E. Grashorn, V. Grassi, S. Grebe, M. Grigat, A. F. Grillo, J. Grygar, Y. Guardincerri, N. Guardone, C. Guerard, F. Guarino, R. Gumbsheimer, G. P. Guedes, J. Gutierrez, J. D. Hague, V. Halenka, P. Hansen, D. Harari, S. Harmsma, S. Hartmann, J. L. Harton, A. Haungs, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, G. Hofman, J. R. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, H. Hucker, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, S. Jiraskova, M. Kaducak, K. H. Kampert, T. Karova, P. Kasper, B. Ke, B. Keilhauer, E. Kempq, H. Kern, R. M. Kieckhafer, H. O. Klages, M. . Kleifges, J. Kleinfeller, R. Knapik, J. Knapp, D. H. Koang, A. Kopmann, A. Krieger, O. Kromer, D. Kruppke Hansen, D. Kuempel, N. Kunka, A. Kusenko, G. La Rosa, C. Lachaud, B. L. Lago, P. Lautridou, M. S. A. B. Leao, D. Lebrun, P. Lebrun, J. Lee, M. A. Leiguide Oliveira, A. Lemiere, A. Letessier Selvon, M. Leuthold, I. Lhenry Yvon, R. Lopez, A. Lopez Aguera, K. Louedec, J. Lozano Bahilo, A. Lucero, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, M. Malek, D. Mandat, P. Mantsch, F. Marchetto, A. G. Mariazzi, I. C. Maris, H. R. Marquez Falcon, O. Martineau, O. Martınez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurizio, P. O. Mazur, M. McEwen, R. R. McNeil, G. Medina Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, R. Meyhandan, M. I. Micheletti, G. Miele, W. Miller, L. Miramonti, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, J. C. Moreno, C. Morris, M. Mostafa, C. A. Moura, M. Mucchi, S. Mueller, M. . A. Muller, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, F. Nerling, C. Newman Holmes, D. Newton, P. T. Nhung, D. Nicotra, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nozka, M. Nyklicek, J. Oehlschlager, A. Olinto, P. Oliva, V. M. Olmos Gilbaja, M. Ortiz, F. Ortolani, B. Oßwald, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, G. Parente, E. Parizot, S. Parlati, S. Pastor, M. Patel, T. Paul, V. Pavlidou, K. Payet, M. Pech, J. Pekala, I. M. Pepe, R. Pesce, E. Petermann, S. Petrera, P. Petrinca, A. Petrolini, Y. Petrov, J. Petrovic, C. Pfendner, A. Pichel, R. Piegaia, T. Pierog, M. Pimenta, T. Pinto, V. Pirronello, O. Pisanti, M. Platino, J. Pochon, V. H. Ponce, M. Pontz, J. Pouryamout, L. Prado J.r., P. Privitera, M. Prouza, E. J. Quel, G. Raia, J. Rautenberg, O. Ravel, D. Ravignani, A. Redondo, H. C. Reis, S. Reucroft, B. Revenu, F. A. S. Rezendem, J. Ridky, S. Riggi, M. Risse, C. Riviere, V. Rizi, C. Robledo, M. D. Roberts, G. Rodriguez, J. Ro driguez Martino, J. Rodriguez Rojo, I. Rodriguez Cabo, M. D. Rodrıguez Frias, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouille d’Orfeuil, E. Roulet, A. C. Rovero, F. Salamida, H. Salazar, G. Salina, F. Sanchez, M. Santander, C. E. Santo, E. M. Santos, F. Sarazin, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, G. Schleif, A. Schmidt, F. Schmidt, T. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovanek, F. Schroeder, S. Schulte, F. Schussler, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, D. Semikoz, G. Sequieros, M. Settimo, R. C. Shellard, I. Sidelnik, B. B. Siffert, A. Smiakowski, R. Smıda, A. G. K. Smith, B. E. Smith, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, E. Strazzeri, A. Stutz, F. Suarez, T. Suomijarvi, A. D. Supanitsky, M. S. Sutherland, J. Swain, Z. Szadkowski, A. Tamashiro, A. Tamburro, T. Tarutina, O. Tascau, R. Tcaciuc, D. Tcherniakhovski, N. T. Thao, D. Thomas, R. Ticona, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, B. Tome, A. Tonachini, I. Torres, P. Trapani, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, V. Tuci, M. Tueros, E. Tusi, R. Ulrich, M. Unger, M. Urban, J. F. Valdes Galicia, I. Valino, L. Valore, A. M. van den Berg, J. R. Vazquez, R. A. Vazquez, D. Veberic, A. Velarde, T. Venters, V. Verzi, M. Videla, L. Villasenor, G. Vitali, S. Vorobiov, L. Voyvodic, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Warner, S. Westerhoff, B. J. Whelan, N. Wild, C. Wiebusch, G. Wieczorek, L. Wiencke, B. Wilczynska, H. Wilczynski, C. Wileman, M. G. Winnick, G. Worner, H. Wuac, B. Wundheiler, T. Yamamoto, P. Younk, G. Yuan, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, M. Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, J., Abraham, P., Abreu, M., Aglietta, C., Aguirre, E. J., Ahn, D., Allard, I., Allekotte, J., Allen, P., Allison, J., Alvarez Muniz, M., Ambrosio, L., Anchordoqui, S., Andringa, A., Anzalone, C., Aramo, E., Arganda, S., Argir, K., Arisaka, F., Arneodo, F., Arquero, T., Asch, H., Asorey, P., Assi, J., Aublin, M., Ave, G., Avila, A., Bacher, T., Backer, D., Badagnani, K. B., Barber, A. F., Barbosa, H. J. M., Barbosa, N., Barenthien, S. L. C., Barroso, B., Baughman, P., Bauleo, J. J., Beatty, T., Beau, B. R., Becker, K. H., Becker, A., Belletoile, J. A., Bellido, S., Benzvi, C., Berat, X., Bertou, P. L., Biermann, P., Billoir, O., Blanch Biga, F., Blanco, C., Bleve, H., Blumer, M., Bohacova, E., Bollmann, H., Bolz, C., Bonifazi, R., Bonino, N., Borodai, F., Bracci, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, N. G., Busca, K. S., Caballero Mora, D., Camin, L., Caramete, R., Caruso, W., Carvalho, A., Castellina, J., Castro, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, J., Chye, P. D. J., Clark, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, B., Connolly, F., Contrera, J., Coppen, A., Cordero, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J. W., Cronin, J., Cuautle, A., Curutiu, S., Dagoret Campagne, R., Dallier, F., Daudo, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, G., Decerprit, L., del Peral, O., Deligny, A., Della Selva, C., Delle Fratte, H., Dembinski, C., Di Giulio, J. C., Diaz, P. N., Diep, C., Dobrigkeit, J. C., D’Olivo, P. N., Dong, D., Dornic, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, I., Dutan, M. A., Du Vernoi, R., Engel, M., Erdmann, C. O., Escobar, A., Etchegoyen, P., Facal San Lui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, F., Ferrer, A., Ferrero, B., Fick, A., Filevich, A., Filipcic, I., Fleck, S., Fliescher, R., Fonte, C. E., Fracchiolla, E. D., Fraenkel, W., Fulgione, R. F., Gama rra, S., Gambetta, B., Garcıa, D., Garcıa Gamez, D., Garcia Pinto, X., Garrido, H., Geenen, G., Gelmini, H., Gemmekeai, P. L., Ghia, U., Giaccari, K., Gibb, M., Giller, J., Gitto, H., Gla, L. M., Goggin, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gomez Berisso, P. F., Gomez Vitale, P., Goncalve, M., Goncalves do Amaral, D., Gonzalez, J. G., Gonzalez, D., Gora, A., Gorgi, P., Gouffon, E., Grashorn, V., Grassi, S., Grebe, M., Grigat, A. F., Grillo, J., Grygar, Y., Guardincerri, N., Guardone, C., Guerard, F., Guarino, R., Gumbsheimer, G. P., Guede, J., Gutierrez, J. D., Hague, V., Halenka, P., Hansen, D., Harari, S., Harmsma, S., Hartmann, J. L., Harton, A., Haung, M. D., Healy, T., Hebbeker, G., Hebrero, D., Heck, C., Hojvat, V. C., Holme, P., Homola, G., Hofman, J. R., Horandel, A., Horneffer, M., Horvat, M., Hrabovsky, H., Hucker, T., Huege, M., Hussain, M., Iarlori, A., Insolia, F., Ionita, A., Italiano, S., Jiraskova, M., Kaducak, K. H., Kampert, T., Karova, P., Kasper, B., Ke, B., Keilhauer, E., Kempq, H., Kern, R. M., Kieckhafer, H. O., Klage, Kleifges, M., J., Kleinfeller, R., Knapik, J., Knapp, D. H., Koang, A., Kopmann, A., Krieger, O., Kromer, D., Kruppke Hansen, D., Kuempel, N., Kunka, A., Kusenko, G., La Rosa, C., Lachaud, B. L., Lago, P., Lautridou, M. S. A. B., Leao, D., Lebrun, P., Lebrun, J., Lee, M. A., Leiguide Oliveira, A., Lemiere, A., Letessier Selvon, M., Leuthold, I., Lhenry Yvon, R., Lopez, A., Lopez Aguera, K., Louedec, J., Lozano Bahilo, A., Lucero, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, M., Malek, D., Mandat, P., Mantsch, F., Marchetto, A. G., Mariazzi, I. C., Mari, H. R., Marquez Falcon, Marsella, Giovanni, Martello, Daniele, O., Martineau, O., Martınez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, M., Mcewen, R. R., Mcneil, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, R., Meyhandan, M. I., Micheletti, G., Miele, W., Miller, L., Miramonti, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, J. C., Moreno, C., Morri, M., Mostafa, C. A., Moura, M., Mucchi, S., Mueller, M. . A., Muller, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, F., Nerling, C., Newman Holme, D., Newton, P. T., Nhung, D., Nicotra, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nozka, M., Nyklicek, J., Oehlschlager, A., Olinto, P., Oliva, V. M., Olmos Gilbaja, M., Ortiz, F., Ortolani, B., Oßwald, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, G., Parente, E., Parizot, S., Parlati, S., Pastor, M., Patel, T., Paul, V., Pavlidou, K., Payet, M., Pech, J., Pekala, I. M., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, A., Pichel, R., Piegaia, T., Pierog, M., Pimenta, T., Pinto, V., Pirronello, O., Pisanti, M., Platino, J., Pochon, V. H., Ponce, M., Pontz, J., Pouryamout, L. Prado J., R., P., Privitera, M., Prouza, E. J., Quel, G., Raia, J., Rautenberg, O., Ravel, D., Ravignani, A., Redondo, H. C., Rei, S., Reucroft, B., Revenu, F. A. S., Rezendem, J., Ridky, S., Riggi, M., Risse, C., Riviere, V., Rizi, C., Robledo, M. D., Robert, G., Rodriguez, J., Ro driguez Martino, J., Rodriguez Rojo, I., Rodriguez Cabo, M. D., Rodrıguez Fria, G., Ro, J., Rosado, T., Rossler, M., Roth, B., Rouille d’Orfeuil, E., Roulet, A. C., Rovero, F., Salamida, H., Salazar, G., Salina, F., Sanchez, M., Santander, C. E., Santo, E. M., Santo, F., Sarazin, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, G., Schleif, A., Schmidt, F., Schmidt, T., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovanek, F., Schroeder, S., Schulte, F., Schussler, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, D., Semikoz, G., Sequiero, M., Settimo, R. C., Shellard, I., Sidelnik, B. B., Siffert, A., Smiakowski, R., Smıda, A. G. K., Smith, B. E., Smith, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijarvi, A. D., Supanitsky, M. S., Sutherland, J., Swain, Z., Szadkowski, A., Tamashiro, A., Tamburro, T., Tarutina, O., Tascau, R., Tcaciuc, D., Tcherniakhovski, N. T., Thao, D., Thoma, R., Ticona, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, B., Tome, A., Tonachini, I., Torre, P., Trapani, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, V., Tuci, M., Tuero, E., Tusi, R., Ulrich, M., Unger, M., Urban, J. F., Valdes Galicia, I., Valino, L., Valore, A. M., van den Berg, J. R., Vazquez, R. A., Vazquez, D., Veberic, A., Velarde, T., Venter, V., Verzi, M., Videla, L., Villasenor, G., Vitali, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, S., Westerhoff, B. J., Whelan, N., Wild, C., Wiebusch, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., Wileman, M. G., Winnick, G., Worner, H., Wuac, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, and M., Ziolkowski
- Subjects
cosmic ray experiments ,ultra high energy cosmic ray - Abstract
The Pierre Auger Collaboration has reported evidence for anisotropy in the dis- tribution of arrival directions of the cosmic rays with energies E > Eth = 5.5×10^19 eV. These show a correlation with the distribution of nearby extragalactic objects, including an appar- ent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > Eth are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above Eth/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above Eth are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.
- Published
- 2011
19. The Lateral Trigger Probability function for UHE Cosmic Rays Showers detected by the Pierre Auger Observatory
- Author
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, E. J. Ahn, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, E. Arganda, S. Argir, K. Arisaka, F. Arneodo, F. Arqueros, T. Asch, H. Asorey, P. Assis, J. Aublin, M. Ave, G. Avila, A. Bacher, T. Backer, D. Badagnani, K. B. Barber, A. F. Barbosa, H. J. M. Barbosa, N. Barenthien, S. L. C. Barroso, B. Baughman, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, A. Belletoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, C. Bleve, H. Blumer, M. Bohacova, E. Bollmann, H. Bolz, C. Bonifazi, R. Bonino, N. Borodai, F. Bracci, J. Brack, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, D. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, J. Castro, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chudoba, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordero, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. W. Cronin, J. Cuautle, A. Curutiu, S. Dagoret Campagne, R. Dallier, F. Daudo, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, K. D. de Vries, G. Decerprit, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, P. N. Diep, C. Dobrigkeit, J. C. D’Olivo, P. N. Dong, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. Du Vernois, R. Engel, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, A. Ferrero, B. Fick, A. Filevich, A. Filipcic, I. Fleck, S. Fliescher, R. Fonte, C. E. Fracchiolla, E. D. Fraenkel, W. Fulgione, R. F. Gama rra, S. Gambetta, B. Garcıa, D. Garcıa Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmekeai, P. L. Ghia, U. Giaccari, K. Gibbs, M. Giller, J. Gitto, H. Glass, L. M. Goggin, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, P. F. Gomez Vitale, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, E. Grashorn, V. Grassi, S. Grebe, M. Grigat, A. F. Grillo, J. Grygar, Y. Guardincerri, N. Guardone, C. Guerard, F. Guarino, R. Gumbsheimer, G. P. Guedes, J. Gutierrez, J. D. Hague, V. Halenka, P. Hansen, D. Harari, S. Harmsma, S. Hartmann, J. L. Harton, A. Haungs, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, G. Hofman, J. R. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, H. Hucker, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, S. Jiraskova, M. Kaducak, K. H. Kampert, T. Karova, P. Kasper, B. Ke, B. Keilhauer, E. Kempq, H. Kern, R. M. 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Timmermans, W. Tkaczyk, C. J. Todero Peixoto, B. Tome, A. Tonachini, I. Torres, P. Trapani, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, V. Tuci, M. Tueros, E. Tusi, R. Ulrich, M. Unger, M. Urban, J. F. Valdes Galicia, I. Valino, L. Valore, A. M. van den Berg, J. R. Vazquez, R. A. Vazquez, D. Veberic, A. Velarde, T. Venters, V. Verzi, M. Videla, L. Villasenor, G. Vitali, S. Vorobiov, L. Voyvodic, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Warner, S. Westerhoff, B. J. Whelan, N. Wild, C. Wiebusch, G. Wieczorek, L. Wiencke, B. Wilczynska, H. Wilczynski, C. Wileman, M. G. Winnick, G. Worner, H. Wuac, B. Wundheiler, T. Yamamoto, P. Younk, G. Yuan, A. Yushkov, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, M. Ziolkowski, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, J., Abraham, P., Abreu, M., Aglietta, C., Aguirre, E. 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S., Caballero Mora, D., Camin, L., Caramete, R., Caruso, W., Carvalho, A., Castellina, J., Castro, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, J., Chye, P. D. J., Clark, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, B., Connolly, F., Contrera, J., Coppen, A., Cordero, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J. W., Cronin, J., Cuautle, A., Curutiu, S., Dagoret Campagne, R., Dallier, F., Daudo, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, K. D., de Vrie, G., Decerprit, L., del Peral, O., Deligny, A., Della Selva, C., Delle Fratte, H., Dembinski, C., Di Giulio, J. C., Diaz, P. N., Diep, C., Dobrigkeit, J. C., D’Olivo, P. N., Dong, D., Dornic, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, I., Dutan, M. 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B., Tridapalli, G., Tristram, E., Trovato, V., Tuci, M., Tuero, E., Tusi, R., Ulrich, M., Unger, M., Urban, J. F., Valdes Galicia, I., Valino, L., Valore, A. M., van den Berg, J. R., Vazquez, R. A., Vazquez, D., Veberic, A., Velarde, T., Venter, V., Verzi, M., Videla, L., Villasenor, G., Vitali, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, S., Westerhoff, B. J., Whelan, N., Wild, C., Wiebusch, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., Wileman, M. G., Winnick, G., Worner, H., Wuac, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, and M., Ziolkowski
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Hybrid detector ,Surface detector ,Extensive Air Shower ,Trigger performance ,Ultra-High Energy Cosmic Ray - Abstract
In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an Extensive Air Shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consisting of a 1.5 km spaced grid of about 1600 water Cherenkov stations. Using Monte Carlo simulations of ultra-high energy showers the LTP functions are derived for energies in the range between 10^17 and 10^19 eV and zenith angles up to 65 degree. A parametrization combining a step function with an exponential is found to reproduce them very well in the considered range of energies and zenith angles. The LTP functions can also be obtained from data using events simultaneously observed by the fluorescence and the surface detector of the Pierre Auger Observatory (hybrid events). We validate the Monte Carlo results showing how LTP functions from data are in good agreement with simulations.
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- 2011
20. A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory
- Author
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J. ABRAHAM, P. ABREU, M. AGLIETTA, E. J. AHN, D. ALLARD, I. ALLEKOTTE, J. ALLEN, J. ALVAREZ MUNIZ, M. AMBROSIO, L. ANCHORDOQUI, S. ANDRINGA, T. ANTICIC, A. ANZALONE, C. ARAMO, E. ARGANDA, K. ARISAKA, F. ARQUEROS, H. ASOREY, P. ASSIS, J. AUBLIN, M. AVE, G. AVILA, T. BACKER, D. BADAGNANI, M. BALZER, K. B. BARBER, A. F. BARBOSA, S. L. C. BARROSO, B. BAUGHMAN, P. BAULEO, J. BEATTY, B. R. BECKER, K. H. BECKER, A. BELLETOILE, J. A. BELLIDO, S. BENZVI, C. BERAT, T. BERGMANN, X. BERTOU, P. L. BIERMANN, P. BILLOIR, O. BLANCH BIGAS, F. BLANCO, M. BLANCO, H. BLUMER, M. BOHACOVA, D. BONCIOLI, C. BONIFAZI, R. BONINO, N. BORODAI, J. BRACK, P. BROGUEIRA, W. C. BROWN, R. BRUIJN, P. BUCHHOLZ, A. BUENO, R. E. BURTON, N. BUSCA, K. S. CABALLERO MORA, L. CARAMETE, R. CARUSO, A. CASTELLINA, O. CATALANO, G. CATALDI, L. CAZON, R. CESTER, J. CHAUVIN, A. CHIAVASSA, J. A. CHINELLATO, A. CHOU, J. CHUDOBA, R. W. CLAY, E. COLOMBO, R. CONCEICAO, F. CONTRERAS, H. COOK, M. COOPER, J. COPPENS, A. CORDIER, U. COTTI, S. COUTU, C. E. COVAULT, A. CREUSOT, A. CRISS, J. CRONIN, A. CURUTIU, S. DAGORET CAMPAGNE, R. DALLIER, K. DAUMILLER, B. R. DAWSON, R. M. DE, ALMEIDA, M. DEDOMENICO, C. DEDONATO, S. J. DEJONG, G. DELAVEGA, W. J. M. DEMELLOJUNIOR, J. DEMELLONETO, V. DESOUZAM, K. D. DEVRIES, G. DECERPRIT, L. DELPERAL, O. DELIGNY, A. DELLASELVA, C. DELLEFRATTE, H. DEMBINSKI, C. DIGIULIO, J. C. DIAZ, M. CASTRO, P. N. DIEP, C. DOBRIGKEIT, J. C. DOLIVO, P. N. DONG, A. DOROFEEV, J. C. DOSANJOS, M. DOVA, D. DURSO, I. DUTAN, M. A. DUVERNOIS, J. EBR, R. ENGEL, M. ERDMANN, C. O, A. ETCHEGOYEN, P. FACALSANLUIS, H. FALCKE, G. FARRAR, A. C. FAUTH, N. FAZZINI, A. FERRERO, B. FICK, A. FILEVICH, A. FILIPCIC, I. FLECK, S. FLIESCHER, C. E. FRACCHIOLLA, E. D. FRAENKEL, U. FROHLICH, W. FULGIONE, R. F. GAMARRA, S. GAMBETTA, B. GARCIA, D. GAMEZ, D. GARCIA PINTO, X. GARRIDO, G. GELMINI, H. GEMMEKEAG, P. L. GHIA, U. GIACCARI, M. GILLER, H. GLASS, L. GOGGIN, M. S. GOLD, G. GOLUP, F. GOMEZALBARRACIN, M. BERISSO, P. GONC ALVES, D. GONZALEZ, J. G. GONZALEZ, D. GORA, A. GORGI, P. GOUFFON, S. R. GOZZINI, E. GRASHORN, S. GREBE, M. GRIGAT, A. F. GRILLO, Y. GUARDINCERRI, F. GUARINO, G. P. GUEDES, J. D. HAGUE, V. HALENKA, P. HANSEN, D. HARARI, S. HARMSMA, J. L. HARTON, A. HAUNGS, T. HEBBEKER, D. HECK, A. E. HERVE, C. HOJVAT, V. C. HOLMES, P. HOMOLA, J. R. HORANDEL, A. HORNEFFER, M. HRABOVSKY, T. HUEGE, M. HUSSAIN, M. IARLORI, A. INSOLIA, F. IONITA, A. ITALIANO, S. JIRASKOVA, K. KADIJA, M. KADUCAK, K. H. KAMPERT, T. KAROVA, P. KASPER, B. KEGL, B. KEILHAUER, A. KEIVANI, J. KELLEY, E. KEMPO, R. M. KIECKHAFER, H. O. KLAGES, M. KLEIFGES, J. KLEINFELLER, R. KNAPIK, J. KNAPP, D. H. KOANG, A. KRIEGER, O. KROMER, D. KRUPPKE HANSEN, F. KUEHN, D. KUEMPEL, K. KULBARTZ, N. KUNKA, A. KUSENKO, G. LAROSA, C. LACHAUD, B. LAGO, P. LAUTRIDOU, M. S. A. B. LEAO, D. LEBRUN, P. LEBRUN, J. LEE, M. A. LEIGUIDEOLIVEIRA, A. LEMIERE, A. LETESSIER SELVON, I. LHENRY YVON, R. LOPEZ, A. LOPEZAGUERA, K. LOUEDEC, J. LOZANOBAHILO, A. LUCERO, M. LUDWIG, H. LYBERIS, M. C. MACCARONE, C. MACOLINO, S. MALDERA, D. MANDAT, P. MANTSCH, A. G. MARIAZZI, V. MARIN, I. C. MARIS, H. FALCON, O. BRAVO, H. J. MATHES, J. MATTHEWS, G. MATTHIAE, D. MAURIZIO, P. O. MAZUR, M. MCEWENBP, G. MEDINA TANCO, M. MELISSAS, D. MELO, E. MENICHETTI, A. MENSHIKOV, C. MEURER, S. MICANOVIC, M. I. MICHELETTI, W. MILLER, L. MIRAMONTI, S. MOLLERACH, M. MONASOR, D. MONNIERRAGAIGNE, F. MONTANET, B. MORALES, C. MORELLO, E. BA, J. C. MORENO, C. MORRIS, M. MOSTAFA, S. MUELLER, M. MULLER, R. MUSSA, G. NAVARRA, J. L. NAVARRO, S. NAVAS, P. NECESAL, L. NELLEN, P. NHUNG, N. NIERSTENHOEFER, D. NITZ, D. NOSEK, L. NOZKA, M. NYKLICEK, J. OEHLSCHLAGER, A. OLINTO, P. OLIVA, V. BR, M. ORTIZ, N. PACHECO, D. PAKKSELMI DEI, M. PALATKA, J. PALLOTTA, N. PALMIERI, G. PARENTE, E. PARIZOT, S. PARLATI, A. PARRA, J. PARRISIUS, R. PARSONS, S. PASTOR, T. PAUL, V. PAVLIDOU, K. PAYET, M. PECH, J. PEKALA, R. PELAYO, I. PEPE, R. PESCE, E. PETERMANN, S. PETRERA, P. PETRINCA, A. PETROLINI, Y. PETROV, J. PETROVIC, C. PFENDNER, R. PIEGAIA, T. PIEROG, M. PIMENTA, V. PIRRONELLO, M. PLATINO, V. H. PONCE, M. PONTZ, P. PRIVITERA, M. PROUZA, E. J. QUEL, J. RAUTENBERG, O. RAVEL, D. RAVIGNANI, A. REDONDO, B. REVENU, F. A. S. REZENDE, J. RIDKY, S. RIGGI, M. RISSE, P. RISTORI, C. RIVIERE, V. RIZI, C. ROBLEDO, G. RODRIGUEZ, J. RODRIGUEZMARTINO, J. RODRIGUEZROJO, I. RODRIGUEZ CABO, M. D. RODRIGUEZ FRIAS, G. ROS, J. ROSADO, T. ROSSLER, M. ROTH, B. ROUILLE DORFEUIL, E. ROULET, A. C. ROVERO, F. SALAMIDA, H. SALAZAR, G. SALINA, F. SANCHEZ, M. SANTANDER, C. E. SANTO, E. SANTO, E. M. SANTOS, F. SARAZIN, S. SARKAR, R. SATO, N. SCHARF, V. SCHERINI, H. SCHIELER, P. SCHIFFER, A. SCHMIDT, F. SCHMIDT, T. SCHMIDT, O. SCHOLTEN, H. SCHOORLEMMER, J. SCHOVANCOVA, P. SCHOVANEK, F. SCHROEDER, S. SCHULTE, F. SCHUSSLER, D. SCHUSTER, S. J. SCIUTTO, M. SCUDERI, A. SEGRETO, D. SEMIKOZ, R. SHELLARD, I. SIDELNIK, B. B. SIFFERT, G. SIGL, A. SMIAKOWSKI, R. SMIDA, G. R. SNOW, P. SOMMERS, J. SOROKIN, H. SPINKA, R. SQUARTINI, J. STASIELAK, M. STEPHAN, E. STRAZZERI, A. STUTZ, F. SUAREZ, T. SUOMIJARVI, A. D. SUPANITSKY, T. SUSA, M. S. SUTHERLAND, J. SWAIN, Z. SZADKOWSKI, A. TAMASHIRO, A. TAMBURRO, A. TAPIA, T. TARUTINA, O. TAS CAU, R. TCACIUC, D. TCHERNIAKHOVSKI, D. TEGOLO, N. T. THAO, D. THOMAS, J. TIFFENBERG, C. TIMMERMANS, W. TKACZYK, C. J. TODEROPEIXOTO, B. TOME, A. TONACHINI, P. TRAVNICEK, D. B. TRIDAPALLI, G. TRISTRAM, E. TROVATO, M. TUEROS, R. ULRICH, M. UNGER, M. URBAN, J. GALICIA, I. VALINO, L. VALORE, A. M. VANDENBERG, J. R. VAZQUEZ, R. A. VAZQUEZ, D. VEBERIC, T. VENTERS, V. VERZI, M. VIDELA, L. VILLASENOR, S. VOROBIOV, L. VOYVODIC, H. WAHLBERG, P. WAHRLICH, O. WAINBERG, D. WARNER, A. A. WATSON, S. WESTERHOFF, B. J. WHELAN, G. WIECZOREK, L. WIENCKE, B. WILCZYNSKA, H. WILCZYNSKI, C. WILLIAMS, T. WINCHEN, M. G. WINNICK, B. WUNDHEILER, T. YAMAMOTO, P. YOUNK, G. YUAN, A. YUSHKOV, E. ZAS, D. ZAVRTANIK, M. ZAVRTANIK, I. ZAW, A. ZEPEDA, M. ZIOLKOWSKI, BLEVE, Carla, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, SETTIMO, MARIANGELA, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), PIERRE AUGER, KVI - Center for Advanced Radiation Technology, Research unit Astroparticle Physics, Guarino, Fausto, D'Urso, Domenico, Valore, Laura, M., Ambrosio, Aramo, Carla, DELLA SELVA, Angelo, C., Moura, Yushkov, Alexey, The Pierre Auger, Collaboration, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, Abraham, J., Abreu, P., Aglietta, M., Aguirre, C., Ahn, E., Allard, D., Allekotte, I., Allen, J., Alvarez-Muñiz, J., Ambrosio, M., Anchordoqui, L., Andringa, S., Anzalone, A., Aramo, C., Arganda, E., Arisaka, K., Arqueros, F., Asch, T., Asorey, H., Assis, P., Aublin, J., Ave, M., Avila, G., Bäcker, T., Badagnani, D., Barber, K., Barbosa, A., Barroso, S., Baughman, B., Bauleo, P., Beatty, J., Beau, T., Becker, B., Becker, K., Bellétoile, A., Bellido, J., Benzvi, S., Berat, C., Bertou, X., Biermann, P., Billoir, P., Blanch-Bigas, O., Blanco, F., Bleve, C., Blümer, H., Boháčová, M., Boncioli, D., Bonifazi, C., Bonino, R., Borodai, N., Brack, J., Brogueira, P., Brown, W., Bruijn, R., Buchholz, P., Bueno, A., Burton, R., Busca, N., Caballero-Mora, K., Caramete, L., Caruso, R., Castellina, A., Catalano, O., Cazon, L., Cester, R., Chauvin, J., Chiavassa, A., Chinellato, J., Chou, A., Chudoba, J., Chye, J., Clay, R., Colombo, E., Conceição, R., Contreras, F., Cook, H., Coppens, J., Cordier, A., Cotti, U., Coutu, S., Covault, C., Creusot, A., Criss, A., Cronin, J., Curutiu, A., Dagoret-Campagne, S., Dallier, R., Daumiller, K., Dawson, B., de Almeida, R., De Domenico, M., De Donato, C., de Jong, S., De La Vega, G., de Mello Junior, W., de Mello Neto, J., De Mitri, I., de Souza, V., de Vries, K., Decerprit, G., del Peral, L., Deligny, O., Della Selva, A., Delle Fratte, C., Dembinski, H., Di Giulio, C., Diaz, J., Diep, P., Dobrigkeit, C., D'Olivo, J., Dong, P., Dorofeev, A., dos Anjos, J., Dova, M., D'Urso, D., Dutan, I., Duvernois, M., Ebr, J., Engel, R., Erdmann, M., Escobar, C., Etchegoyen, A., Facal San Luis, P., Falcke, H., Farrar, G., Fauth, A., Fazzini, N., Ferrer, F., Ferrero, A., Fick, B., Filevich, A., Filipčič, A., Fleck, I., Fliescher, S., Fracchiolla, C., Fraenkel, E., Fulgione, W., Gamarra, R., Gambetta, S., García, B., García Gámez, D., Garcia-Pinto, D., Garrido, X., Gelmini, G., Gemmeke, H., Ghia, P., Giaccari, U., Giller, M., Glass, H., Goggin, L., Gold, M., Golup, G., Gomez Albarracin, F., Gómez Berisso, M., Gonçalves, P., Gonzalez, D., Gonzalez, J., Góra, D., Gorgi, A., Gouffon, P., Gozzini, S., Grashorn, E., Grebe, S., Grigat, M., Grillo, A., Guardincerri, Y., Guarino, F., Guedes, G., Gutiérrez, J., Hague, J., Halenka, V., Hansen, P., Harari, D., Harmsma, S., Harton, J., Haungs, A., Healy, M., Hebbeker, T., Hebrero, G., Heck, D., Hojvat, C., Holmes, V., Homola, P., Hörandel, J., Horneffer, A., Hrabovský, M., Huege, T., Hussain, M., Iarlori, M., Insolia, A., Ionita, F., Italiano, A., Jiraskova, S., Kaducak, M., Kampert, K., Karova, T., Kasper, P., Kégl, B., Keilhauer, B., Kelley, J., Kemp, E., Kieckhafer, R., Klages, H., Kleifges, M., Kleinfeller, J., Knapik, R., Knapp, J., Koang, D., Krieger, A., Krömer, O., Kruppke-Hansen, D., Kuehn, F., Kuempel, D., Kulbartz, K., Kunka, N., Kusenko, A., La Rosa, G., Lachaud, C., Lago, B., Lautridou, P., Leão, M., Lebrun, D., Lebrun, P., Lee, J., Leigui de Oliveira, M., Lemiere, A., Letessier-Selvon, A., Lhenry-Yvon, I., López, R., Lopez Agüera, A., Louedec, K., Lozano Bahilo, J., Lucero, A., Ludwig, M., Lyberis, H., Maccarone, M., Macolino, C., Maldera, S., Mandat, D., Mantsch, P., Mariazzi, A., Maris, I., Marquez Falcon, H., Marsella, G., Martello, D., Martínez Bravo, O., Mathes, H., Matthews, J., Matthiae, G., Maurizio, D., Mazur, P., Mcewen, M., Mcneil, R., Medina-Tanco, G., Melissas, M., Melo, D., Menichetti, E., Menshikov, A., Meurer, C., Micheletti, M., Miller, W., Miramonti, L., Mollerach, S., Monasor, M., Monnier Ragaigne, D., Montanet, F., Morales, B., Morello, C., Moreno, J., Morris, C., Mostafá, M., Moura, C., Mueller, S., Muller, M., Mussa, R., Navarra, G., Navarro, J., Navas, S., Necesal, P., Nellen, L., Newman-Holmes, C., Nhung, P., Nierstenhoefer, N., Nitz, D., Nosek, D., Nožka, L., Nyklicek, M., Oehlschläger, J., Olinto, A., Oliva, P., Olmos-Gilbaja, V., Ortiz, M., Pacheco, N., Pakk Selmi-Dei, D., Palatka, M., Pallotta, J., Palmieri, N., Parente, G., Parizot, E., Parlati, S., Parsons, R., Pastor, S., Paul, T., Pavlidou, V., Payet, K., Pech, M., Pȩkala, J., Pepe, I., Perrone, L., Pesce, R., Petermann, E., Petrera, S., Petrinca, P., Petrolini, A., Petrov, Y., Petrovic, J., Pfendner, C., Piegaia, R., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Ponce, V., Pontz, M., Privitera, P., Prouza, M., Quel, E., Rautenberg, J., Ravel, O., Ravignani, D., Redondo, A., Revenu, B., Rezende, F., Ridky, J., Riggi, S., Risse, M., Rivière, C., Rizi, V., Robledo, C., Rodriguez, G., Rodriguez Martino, J., Rodriguez Rojo, J., Rodriguez-Cabo, I., Rodríguez-Frías, M., Ros, G., Rosado, J., Rossler, T., Roth, M., Rouillé-d'Orfeuil, B., Roulet, E., Rovero, A., Salamida, F., Salazar, H., Salina, G., Sánchez, F., Santander, M., Santo, C., Santos, E., Sarazin, F., Sarkar, S., Sato, R., Scharf, N., Scherini, V., Schieler, H., Schiffer, P., Schmidt, A., Schmidt, F., Schmidt, T., Scholten, O., Schoorlemmer, H., Schovancova, J., Schovánek, P., Schroeder, F., Schulte, S., Schüssler, F., Schuster, D., Sciutto, S., Scuderi, M., Segreto, A., Semikoz, D., Settimo, M., Shellard, R., Sidelnik, I., Siffert, B., Sigl, G., Śmiałkowski, A., Šmída, R., Snow, G., Sommers, P., Sorokin, J., Spinka, H., Squartini, R., Strazzeri, E., Stutz, A., Suarez, F., Suomijärvi, T., Supanitsky, A., Sutherland, M., Swain, J., Szadkowski, Z., Tamashiro, A., Tamburro, A., Tarutina, T., Taşcǎu, O., Tcaciuc, R., Tcherniakhovski, D., Tegolo, D., Thao, N., Thomas, D., Ticona, R., Tiffenberg, J., Timmermans, C., Tkaczyk, W., Todero Peixoto, C., Tomé, B., Tonachini, A., Torres, I., Travnicek, P., Tridapalli, D., Tristram, G., Trovato, E., Tueros, M., Ulrich, R., Unger, M., Urban, M., Valdés Galicia, J., Valiño, I., Valore, L., van den Berg, A., Vázquez, J., Vázquez, R., Veberič, D., Velarde, A., Venters, T., Verzi, V., Videla, M., Villaseñor, L., Vorobiov, S., Voyvodic, L., Wahlberg, H., Wahrlich, P., Wainberg, O., Warner, D., Watson, A., Westerhoff, S., Whelan, B., Wieczorek, G., Wiencke, L., Wilczyńska, B., Wilczyński, H., Winchen, T., Winnick, M., Wu, H., Wundheiler, B., Yamamoto, T., Younk, P., Yuan, G., Yushkov, A., Zas, E., Zavrtanik, D., Zavrtanik, M., Zaw, I., Zepeda, A., Ziolkowski, M., J., Abraham, P., Abreu, M., Aglietta, E. J., Ahn, D., Allard, I., Allekotte, J., Allen, J., ALVAREZ MUNIZ, L., Anchordoqui, S., Andringa, T., Anticic, A., Anzalone, C., Aramo, E., Arganda, K., Arisaka, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, G., Avila, T., Backer, D., Badagnani, M., Balzer, K. B., Barber, A. F., Barbosa, S. L. C., Barroso, B., Baughman, P., Bauleo, J., Beatty, B. R., Becker, K. H., Becker, A., Belletoile, J. A., Bellido, S., Benzvi, C., Berat, T., Bergmann, X., Bertou, P. L., Biermann, P., Billoir, O., BLANCH BIGAS, F., Blanco, M., Blanco, Bleve, Carla, H., Blumer, M., Bohacova, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, N., Busca, K. S., CABALLERO MORA, L., Caramete, R., Caruso, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, F., Contrera, H., Cook, M., Cooper, J., Coppen, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., DAGORET CAMPAGNE, R., Dallier, K., Daumiller, B. R., Dawson, R. M., De, Almeida, M., Dedomenico, C., Dedonato, S. J., Dejong, G., Delavega, W. J. M., Demellojunior, J., Demelloneto, DE MITRI, Ivan, V., Desouzam, K. D., Devrie, G., Decerprit, L., Delperal, O., Deligny, A., Dellaselva, C., Dellefratte, H., Dembinski, C., Digiulio, J. C., Diaz, M., Castro, P. N., Diep, C., Dobrigkeit, J. C., Dolivo, P. N., Dong, A., Dorofeev, J. C., Dosanjo, M., Dova, D., Durso, I., Dutan, M. A., Duvernoi, J., Ebr, R., Engel, M., Erdmann, C., O, A., Etchegoyen, P., Facalsanlui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, A., Ferrero, B., Fick, A., Filevich, A., Filipcic, I., Fleck, S., Fliescher, C. E., Fracchiolla, E. D., Fraenkel, U., Frohlich, W., Fulgione, R. 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T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Toderopeixoto, B., Tome, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J., Galicia, I., Valino, L., Valore, A. M., Vandenberg, J. R., Vazquez, R. A., Vazquez, D., Veberic, T., Venter, V., Verzi, M., Videla, L., Villasenor, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, A. A., Watson, S., Westerhoff, B. J., Whelan, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., William, T., Winchen, M. G., Winnick, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, and M., Ziolkowski
- Subjects
Angstrom exponent ,Astronomy ,Astrophysics ,01 natural sciences ,Auger ,CROSS-SECTIONS ,COSMIC-RAY SHOWERS ,Observatory ,DEPENDENCE ,High-Energy Cosmic Ray ,010303 astronomy & astrophysics ,Physics ,High Energy Astrophysical Phenomena (astro-ph.HE) ,Lidar ,[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,ANGSTROM EXPONENT ,Pierre Auger Observatory ,Bi-static lidar ,ELECTRONS ,ComputingMethodologies_DOCUMENTANDTEXTPROCESSING ,MULTIPLE-SCATTERING ,Light emission ,Física nuclear ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,LIGHT-EMISSION ,Astrophysics - Cosmology and Nongalactic Astrophysics ,[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE] ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Extensive air shower ,FOS: Physical sciences ,Cosmic ray ,SURFACE DETECTOR ,Air fluorescence method ,0103 physical sciences ,Extensive air showers ,RECONSTRUCTION ,Aerosol ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Cosmic rays ,Aerosols ,Calorimeter (particle physics) ,Atmospheric effect ,010308 nuclear & particles physics ,Atmosphere ,Física ,Astronomy and Astrophysics ,NITROGEN ,Air shower ,Fluorescence Telescopes ,13. Climate action ,Experimental High Energy Physics ,AEROSSOL - Abstract
The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements oil air shower reconstructions. Between 10(18) and 10(20) eV, the systematic Uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g cm(-2) to 8 g cm(-2) in measurements of the shower maximum., The successful installation and commissioning of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Comisión Nacional de Energía Atómica, Fundación Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargüe, NDM Holdings and Valle Las Leñas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundaçao de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundaçao de Amparo à Pesquisa do Estado de Sao Paulo (FAPESP), Ministério de Ciência e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB300100801 and KJB100100904, MSMT-CR LA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Régional Ile-de-France, Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS), Département Sciences de l’Univers (SDU-INSU/CNRS), France; Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden- Württemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium für Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium für Wissenschaft, Forschung und Kunst, Baden-W¨urttemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell’Istruzione,dell’Università e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. 1 P03 D 014 30, N202 090 31/0623, and PAP/218/2006, Poland; Fundaçao para a Ciência e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejería de Educación de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovación, Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract No. DE-AC02-07CH11359, National Science Foundation, Grant No. 0450696, The Grainger Foundation USA; ALFA-EC / HELEN, European Union 6th Framework Program, Grant No. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO.
- Published
- 2010
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21. The Northen Site of the Pierre Auger Observatory
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J. ABRAHAM, P. ABREU, M. AGLIETTA, E. J. AHN, D. ALLARD, I. ALLEKOTTE, J. ALLEN, J. ALVAREZ MUNIZ, M. AMBROSIO, L. ANCHORDOQUI, S. ANDRINGA, T. ANTICIC, A. ANZALONE, C. ARAMO, E. ARGANDA, K. ARISAKA, F. ARQUEROS, H. ASOREY, P. ASSIS, J. AUBLIN, M. AVE, G. AVILA, T. BACKER, D. BADAGNANI, M. BALZER, K. B. BARBER, A. F. BARBOSA, S. L. C. BARROSO, B. BAUGHMAN, P. BAULEO, J. BEATTY, B. R. BECKER, K. H. BECKER, A. BELLETOILE, J. A. BELLIDO, S. BENZVI, C. BERAT, T. BERGMANN, X. BERTOU, P. L. BIERMANN, P. BILLOIR, O. BLANCH BIGAS, F. BLANCO, M. BLANCO, H. BLUMER, M. BOHACOVA, D. BONCIOLI, C. BONIFAZI, R. BONINO, N. BORODAI, J. BRACK, P. BROGUEIRA, W. C. BROWN, R. BRUIJN, P. BUCHHOLZ, A. BUENO, R. E. BURTON, N. BUSCA, K. S. CABALLERO MORA, L. CARAMETE, R. CARUSO, A. CASTELLINA, O. CATALANO, G. CATALDI, L. CAZON, R. CESTER, J. CHAUVIN, A. CHIAVASSA, J. A. CHINELLATO, A. CHOU, J. CHUDOBA, R. W. CLAY, E. COLOMBO, R. CONCEICAO, F. CONTRERAS, H. COOK, M. COOPER, J. COPPENS, A. CORDIER, U. COTTI, S. 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SQUARTINI, J. STASIELAK, M. STEPHAN, E. STRAZZERI, A. STUTZ, F. SUAREZ, T. SUOMIJARVI, A. D. SUPANITSKY, T. SUSA, M. S. SUTHERLAND, J. SWAIN, Z. SZADKOWSKI, A. TAMASHIRO, A. TAMBURRO, A. TAPIA, T. TARUTINA, O. TAS CAU, R. TCACIUC, D. TCHERNIAKHOVSKI, D. TEGOLO, N. T. THAO, D. THOMAS, J. TIFFENBERG, C. TIMMERMANS, W. TKACZYK, C. J. TODEROPEIXOTO, B. TOME, A. TONACHINI, P. TRAVNICEK, D. B. TRIDAPALLI, G. TRISTRAM, E. TROVATO, M. TUEROS, R. ULRICH, M. UNGER, M. URBAN, J. GALICIA, I. VALINO, L. VALORE, A. M. VANDENBERG, J. R. VAZQUEZ, R. A. VAZQUEZ, D. VEBERIC, T. VENTERS, V. VERZI, M. VIDELA, L. VILLASENOR, S. VOROBIOV, L. VOYVODIC, H. WAHLBERG, P. WAHRLICH, O. WAINBERG, D. WARNER, A. A. WATSON, S. WESTERHOFF, B. J. WHELAN, G. WIECZOREK, L. WIENCKE, B. WILCZYNSKA, H. WILCZYNSKI, C. WILLIAMS, T. WINCHEN, M. G. WINNICK, B. WUNDHEILER, T. YAMAMOTO, P. YOUNK, G. YUAN, A. YUSHKOV, E. ZAS, D. ZAVRTANIK, M. ZAVRTANIK, I. ZAW, A. ZEPEDA, M. ZIOLKOWSKI, BLEVE, Carla, COLUCCIA, MARIA RITA, DE MITRI, Ivan, MARSELLA, GIOVANNI, MARTELLO, Daniele, PERRONE, Lorenzo, SETTIMO, MARIANGELA, J., Abraham, P., Abreu, M., Aglietta, E. J., Ahn, D., Allard, I., Allekotte, J., Allen, J., ALVAREZ MUNIZ, M., Ambrosio, L., Anchordoqui, S., Andringa, T., Anticic, A., Anzalone, C., Aramo, E., Arganda, K., Arisaka, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, G., Avila, T., Backer, D., Badagnani, M., Balzer, K. B., Barber, A. F., Barbosa, S. L. C., Barroso, B., Baughman, P., Bauleo, J., Beatty, B. R., Becker, K. H., Becker, A., Belletoile, J. A., Bellido, S., Benzvi, C., Berat, T., Bergmann, X., Bertou, P. L., Biermann, P., Billoir, O., BLANCH BIGAS, F., Blanco, M., Blanco, Bleve, Carla, H., Blumer, M., Bohacova, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, P., Brogueira, W. C., Brown, R., Bruijn, P., Buchholz, A., Bueno, R. E., Burton, N., Busca, K. S., CABALLERO MORA, L., Caramete, R., Caruso, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chudoba, R. W., Clay, E., Colombo, Coluccia, MARIA RITA, R., Conceicao, F., Contrera, H., Cook, M., Cooper, J., Coppen, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., DAGORET CAMPAGNE, R., Dallier, K., Daumiller, B. R., Dawson, R. M., De, Almeida, M., Dedomenico, C., Dedonato, S. J., Dejong, G., Delavega, W. J. M., Demellojunior, J., Demelloneto, DE MITRI, Ivan, V., Desouzam, K. D., Devrie, G., Decerprit, L., Delperal, O., Deligny, A., Dellaselva, C., Dellefratte, H., Dembinski, C., Digiulio, J. C., Diaz, M., Castro, P. N., Diep, C., Dobrigkeit, J. C., Dolivo, P. N., Dong, A., Dorofeev, J. C., Dosanjo, M., Dova, D., Durso, I., Dutan, M. A., Duvernoi, J., Ebr, R., Engel, M., Erdmann, C., O, A., Etchegoyen, P., Facalsanlui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, A., Ferrero, B., Fick, A., Filevich, A., Filipcic, I., Fleck, S., Fliescher, C. E., Fracchiolla, E. D., Fraenkel, U., Frohlich, W., Fulgione, R. F., Gamarra, S., Gambetta, B., Garcia, D., Gamez, D., GARCIA PINTO, X., Garrido, G., Gelmini, H., Gemmekeag, P. L., Ghia, U., Giaccari, M., Giller, H., Gla, L., Goggin, M. S., Gold, G., Golup, F., Gomezalbarracin, M., Berisso, P., GONC ALVES, D., Gonzalez, J. G., Gonzalez, D., Gora, A., Gorgi, P., Gouffon, S. R., Gozzini, E., Grashorn, S., Grebe, M., Grigat, A. F., Grillo, Y., Guardincerri, F., Guarino, G. P., Guede, J. D., Hague, V., Halenka, P., Hansen, D., Harari, S., Harmsma, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, A. E., Herve, C., Hojvat, V. C., Holme, P., Homola, J. R., Horandel, A., Horneffer, M., Hrabovsky, T., Huege, M., Hussain, M., Iarlori, A., Insolia, F., Ionita, A., Italiano, S., Jiraskova, K., Kadija, M., Kaducak, K. H., Kampert, T., Karova, P., Kasper, B., Kegl, B., Keilhauer, A., Keivani, J., Kelley, E., Kempo, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, R., Knapik, J., Knapp, D. H., Koang, A., Krieger, O., Kromer, D., KRUPPKE HANSEN, F., Kuehn, D., Kuempel, K., Kulbartz, N., Kunka, A., Kusenko, G., Larosa, C., Lachaud, B., Lago, P., Lautridou, M. S. A. B., Leao, D., Lebrun, P., Lebrun, J., Lee, M. A., Leiguideoliveira, A., Lemiere, A., LETESSIER SELVON, I., LHENRY YVON, R., Lopez, A., Lopezaguera, K., Louedec, J., Lozanobahilo, A., Lucero, M., Ludwig, H., Lyberi, M. C., Maccarone, C., Macolino, S., Maldera, D., Mandat, P., Mantsch, A. G., Mariazzi, V., Marin, I. C., Mari, H., Falcon, Marsella, Giovanni, Martello, Daniele, O., Bravo, H. J., Mathe, J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, M., Mcewenbp, G., MEDINA TANCO, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, C., Meurer, S., Micanovic, M. I., Micheletti, W., Miller, L., Miramonti, S., Mollerach, M., Monasor, D., Monnierragaigne, F., Montanet, B., Morale, C., Morello, E., Ba, J. C., Moreno, C., Morri, M., Mostafa, S., Mueller, M., Muller, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, P., Nhung, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nozka, M., Nyklicek, J., Oehlschlager, A., Olinto, P., Oliva, V., Br, M., Ortiz, N., Pacheco, D., PAKKSELMI DEI, M., Palatka, J., Pallotta, N., Palmieri, G., Parente, E., Parizot, S., Parlati, A., Parra, J., Parrisiu, R., Parson, S., Pastor, T., Paul, V., Pavlidou, K., Payet, M., Pech, J., Pekala, R., Pelayo, I., Pepe, Perrone, Lorenzo, R., Pesce, E., Petermann, S., Petrera, P., Petrinca, A., Petrolini, Y., Petrov, J., Petrovic, C., Pfendner, R., Piegaia, T., Pierog, M., Pimenta, V., Pirronello, M., Platino, V. H., Ponce, M., Pontz, P., Privitera, M., Prouza, E. J., Quel, J., Rautenberg, O., Ravel, D., Ravignani, A., Redondo, B., Revenu, F. A. S., Rezende, J., Ridky, S., Riggi, M., Risse, P., Ristori, C., Riviere, V., Rizi, C., Robledo, G., Rodriguez, J., Rodriguezmartino, J., Rodriguezrojo, I., RODRIGUEZ CABO, M. D., RODRIGUEZ FRIAS, G., Ro, J., Rosado, T., Rossler, M., Roth, B., ROUILLE DORFEUIL, E., Roulet, A. C., Rovero, F., Salamida, H., Salazar, G., Salina, F., Sanchez, M., Santander, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, S., Sarkar, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, A., Schmidt, F., Schmidt, T., Schmidt, O., Scholten, H., Schoorlemmer, J., Schovancova, P., Schovanek, F., Schroeder, S., Schulte, F., Schussler, D., Schuster, S. J., Sciutto, M., Scuderi, A., Segreto, D., Semikoz, Settimo, Mariangela, R., Shellard, I., Sidelnik, B. B., Siffert, G., Sigl, A., Smiakowski, R., Smida, G. R., Snow, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, J., Stasielak, M., Stephan, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijarvi, A. D., Supanitsky, T., Susa, M. S., Sutherland, J., Swain, Z., Szadkowski, A., Tamashiro, A., Tamburro, A., Tapia, T., Tarutina, O., TAS CAU, R., Tcaciuc, D., Tcherniakhovski, D., Tegolo, N. T., Thao, D., Thoma, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Toderopeixoto, B., Tome, A., Tonachini, P., Travnicek, D. B., Tridapalli, G., Tristram, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, J., Galicia, I., Valino, L., Valore, A. M., Vandenberg, J. R., Vazquez, R. A., Vazquez, D., Veberic, T., Venter, V., Verzi, M., Videla, L., Villasenor, S., Vorobiov, L., Voyvodic, H., Wahlberg, P., Wahrlich, O., Wainberg, D., Warner, A. A., Watson, S., Westerhoff, B. J., Whelan, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., William, T., Winchen, M. G., Winnick, B., Wundheiler, T., Yamamoto, P., Younk, G., Yuan, A., Yushkov, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, M., Ziolkowski, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), PIERRE AUGER, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Guarino, Fausto, D'Urso, Domenico, Valore, Laura, Aramo, Carla, DELLA SELVA, Angelo, Yushkov, Alexey, and The Pierre Auger, Collaboration
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Pierre Auger Observatory ,Physics ,high energy ,Particle composition ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Instrumentation and Methods for Astrophysics ,General Physics and Astronomy ,Astronomy ,Cosmic ray ,Cosmic Ray ,01 natural sciences ,Auger ,North-Site of the Pierre Auger Observatory ,Auger Observatory ,Observatory ,0103 physical sciences ,Energy spectrum ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Neutrino ,High-Energy Cosmic Ray ,010306 general physics - Abstract
Part of Focus on High Energy Cosmic Rays - see paper for full liste of authors; The Pierre Auger Observatory is an international facility dedicated to the full-sky study of the highest-energy cosmic rays. The southern site of the Auger Observatory was completed in June 2008. Data collected since January 2004 have yielded important information on the energy spectrum, the primary particle composition, the fluxes of photons and neutrinos and on the anisotropic distribution of the arrival directions of the most energetic particles. On this basis, the scientific motivation for the northern Auger Observatory site in Colorado, USA, is discussed. The overall layout, the key components and the expected performance of this 20 000 km2 hybrid observatory comprised of an array of 4400 surface detectors and 39 fluorescence telescopes are described.
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- 2010
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22. Carcinoma of the Stomach with Myelosclerosis: Presentation of a Case and Review of the Literature
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H, Blumer, A, Aronoff, J, Chartier, and L, Shapiro
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Case Report - Published
- 2010
23. The SLS Optics Beamline
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H. Blumer, H. Walther, A. Jaggi, Alastair A. MacDowell, K. Frank, V. Schonherr, H. A. Padmore, Rafael Abela, U. Flechsig, R. Betemps, Saša Zelenika, J. Ulrich, and C. Zumbach
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Physics ,synchrotron radiation beamline optics channel cut monochromator cryogenic cooling ,Photon ,synchrotron radiation ,beamline optics ,channel cut monochromator ,cryogenic cooling ,business.industry ,Physics::Instrumentation and Detectors ,X-ray optics ,Synchrotron radiation ,Particle accelerator ,law.invention ,Engineering ,Optics ,Beamline ,law ,Electromagnetic shielding ,Optoelectronics ,Physics::Accelerator Physics ,business ,Swiss Light Source ,Monochromator - Abstract
A multipurpose beamline for tests and developments in the ?eld of x-ray optics and synchrotron radiation instrumentation in general is under construction at the Swiss Light Source (SLS) bending magnet X05DA. The beamline uses a newly developed UHV compatible, 100 mm thick, brazed CVD diamond vacuum window. The very compact cryogenicly cooled channel cut Si(111) monochromator and bendable 1:1 toroidal focusing mirror at 7:75 m from the source point are installed inside the shielding tunnel. The beamline covers a photon energy range of about 6 to 17 keV. We expect 5x1011 photons=s within a 100 mu m spot and a re solving power of 1300. The monochromator and focusing mirror can be retracted independently for unfocused monochromatic and focused "white" light operation respectively.
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- 2007
24. A Configurable Solid State Power Management and Distribution System
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John M. Maxwell, John H. Blumer, and Blake Burden
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Power management ,Distribution system ,Computer science ,Solid-state ,Control engineering - Published
- 2002
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25. Practicality of using a Tether for electrodynamic reboost of the International Space Station
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John H. Blumer, Michal E. Bangham, and Benjamin B. Donahue
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Engineering ,business.product_category ,Rocket ,business.industry ,International Space Station ,Orbit (dynamics) ,Liquid rocket propellants ,Thrust ,Aerospace engineering ,Propulsion ,Space research ,business ,Space rendezvous - Abstract
ElectroDynamic (ED) Tethers can generate continuous low thrust in a low Earth orbit. An induced current running through the length of the tether reacts with the geomagnetic field to produce thrust. The amount of thrust scales with tether lens!th and current. The International Space Station (ISS) requires periodic reboost to maintain an approximately circular orbit t above the Earth. The baseline reboost method is a traditional bi-propellant rocket thruster and tankage system which must to be refueled via Soyuz / Progress or other launch vehicle. The estimated propellant costs associated with keeping ISS in the designated orbit over a 10-year life have been extremely high. The ED Tether would draw energy from the renewable ISS Solar Array electrical power system. Propulsion requirements for ISS vary depending on solar wind and other conditions. It is projected that a ED Tether could provide the majority of the required reboost thrust for ISS for a nominal solar year. For above nominal solar wind years the ISS would have to use the rocket reboost system, but at a greatly reduced level. Thus resulting in substantial cost savings, via the reduction in the number of Earth-to-orbit launch vehicle flights to the ISS that must bring reboost propellant. However, the purposes of this paper is to further Previous research on an ISS ED Tether and examine the operational and technical issues working against using a ED Tether on ISS. Issues such as Shuttle rendezvous and flight path concerns raise serious safety concerns and restrictions on tether use. Tether issues such as tether librations and off angle thrust raise concerns about impacts to microgravity payloads and the long-term effect on ISS orbital path and inclination. Operational issues such as peak power available to an ED Tether and allowable duty cycle may impose severe restrictions on tether design and ultimately limit the practicality of an ED Tether on ISS. Thus while at first glance the cost numbers appear to be strongly in favor of an ED Tether the limitations imposed by safety, operations and technical concerns may severely undermine the economic model. Possible Solutions to these problems have been investigated and proposed, however some items like off angle thrust are still being actively investigated for an adequate solution.
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- 2001
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26. Lessons learned using COTS electronics for the International Space Station radiation environment
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John H. Blumer
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Schedule ,Engineering ,Backplane ,business.industry ,Interface (computing) ,Embedded system ,International Space Station ,Eurocard ,Systems engineering ,Electronics ,Space research ,business ,VMEbus - Abstract
The mantra of 'Faster, Better, Cheaper' has to a large degree been interpreted as using Commercial Off-the-Shelf (COTS) components and/or circuit boards. One of the first space applications to actually use COTS in space along with radiation performance requirements was the Expedite the Processing of Experiments to Space Station (EXPRESS) Rack program, for the International Space Station (ISS). In order to meet the performance, cost and schedule targets, military grade Versa Module Eurocard (VME) was selected as the baseline design for the main computer, the Rack Interface Controller (RIC). VME was chosen as the computer backplane because of the large variety of military grade boards available, which were designed to meet the military environmental specifications (thermal, shock, vibration, etc.). These boards also have a paper pedigree in regards to components. Since these boards exceeded most ISS environmental requirements, it was reasoned using COTS mid-grade VME boards, as opposed to designing custom boards could save significant time and money. It was recognized up front the radiation environment of ISS, while benign compared to many space flight applications, would be the main challenge to using COTS. Thus in addition to selecting vendors on how well their boards met the usual performance and environmental specifications, the board's parts lists were reviewed on how well they would perform in the ISS radiation environment. However, issues with verifying that the available radiation test data was applicable to the actual part used, vendor part design changes and the fact most parts did not have valid test data soon complicated board and part selection in regards to radiation.
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- 2001
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27. 252 TUMOR NECROSIS FACTOR ALPHA CONTRIBUTES TO PAIN AND HYPERALGESIA IN A MOUSE CANCER/METASTASIS MODEL
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C.A. Sailer, H. Blumer, Cristina E. Constantin, Michaela Kress, and N Mair
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Anesthesiology and Pain Medicine ,business.industry ,Hyperalgesia ,Cancer research ,Medicine ,Cancer metastasis ,Tumor necrosis factor alpha ,medicine.symptom ,business - Published
- 2007
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28. PHYSICOCHEMICAL STUDIES ON PRECIPITATING AND NON-PRECIPITATING ANTIBODIES AFTER PRIMARY IMMUNIZATION
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F. Cua-Lim, Bram Rose, H. Blumer, and Maxwell Richter
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Antiserum ,Precipitating antibodies ,biology ,Antigen ,Chemistry ,biology.protein ,Serum protein ,Primary response ,Primary immunization ,Gamma globulin ,General Medicine ,Antibody ,Molecular biology - Abstract
Antisera were obtained from rabbits within 30 days (early antisera) and 90–120 days (late antisera) after the last of a series of intravenous injections of serum protein antigens (primary response). The antibodies present in early antisera were found capable of precipitating with the antigen and of agglutinating sensitized red blood cells, whereas those present in late antisera exhibited only the latter property. These two types of antibodies could not be differentiated on the basis of their electrophoretic, sedimentation, and salting out properties. Both behaved essentially as gamma globulins.
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- 1962
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29. Precipitating and Nonprecipitating Antibodies in the Primary and Secondary Immune Responses
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H. Blumer, M. Richter, F. Cua-Lim, and B. Rose
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Immunology ,Immunology and Allergy - Abstract
Summary The formation of antibodies to soluble protein antigens for many months after primary immunization has been confirmed. These antibodies were produced after the immunization of rabbits with bovine serum albumin, egg albumin, human γ-globulin, pig γ-globulin and bovine γ-globulin. The antibodies present in the circulation 11 to 16 days after the initial immunization could be detected by using antigen-coated red cells and, in most cases, by the precipitin technique as well. Those antibodies present in the circulation several months later could be detected only by the hemagglutination technique. The hemagglutinating antibody titer remained constant for at least 6 months after primary immunization. In some cases the nonprecipitating antibody concentration was found to rise at a time when the precipitating antibody level was declining. Hemagglutinating antibody titers of sera, following secondary immunization, rose to high levels very rapidly and then started to decline, rapidly at first and more slowly later. Only those antisera which were obtained during the early period of antibody production and which contained precipitating antibody could passively sensitize guinea pigs. Cortisone acetate inhibited the primary response to intravenously injected antigens in six out of seven rabbits. It failed, however, to inhibit the secondary antibody response.
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- 1962
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30. The Green Bank North Celestial Cap Pulsar Survey. V. Pulsar Census and Survey Sensitivity.
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A. E. McEwen, R. Spiewak, J. K. Swiggum, D. L. Kaplan, W. Fiore, G. Y. Agazie, H. Blumer, P. Chawla, M. DeCesar, V. M. Kaspi, V. I. Kondratiev, M. LaRose, L. Levin, R. S. Lynch, M. McLaughlin, M. Mingyar, H. Al Noori, S. M. Ransom, M. S. E. Roberts, and A. Schmiedekamp
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PULSAR detection ,RADIO interference ,PULSARS ,ACTINIC flux ,PARAMETERS (Statistics) ,SIGNAL-to-noise ratio - Abstract
The Green Bank North Celestial Cap (GBNCC) pulsar survey will cover the entire northern sky (δ > −40°) at 350 MHz, and is one of the most uniform and sensitive all-sky pulsar surveys to date. We have created a pipeline to reanalyze GBNCC survey data to take a 350 MHz census of all pulsars detected by the survey, regardless of their discovery survey. Of the 1413 pulsars in the survey region, we were able to recover 670. For these we present measured signal-to-noise ratios (S/N), flux densities, pulse widths, profiles, and where appropriate, refined measurements of dispersion measures (DMs) (656 out of 670) and new or improved spectral indices (339 out of 670 total, 47 new, 292 improved). We also measure the period-pulse width relation at 350 MHz to scale as . Detection scans for several hundred sources were reanalyzed in order to inspect pulsars’ single pulse behavior and 223 were found to exhibit evidence of nulling. With a detailed analysis of measured and expected S/N values and the evolving radio frequency interference environment at 350 MHz, we assess the GBNCC survey’s sensitivity as a function of spin period, DM, and sky position. We find the sky-averaged limiting flux density of the survey to be 0.74 mJy. Combining this analysis with PsrPopPy pulsar population simulations, we predict 60/5 nonrecycled/MSP discoveries in the survey’s remaining 21,000 pointings, and we begin to place constraints on population model parameters. [ABSTRACT FROM AUTHOR]
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- 2020
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31. Correlation of the highest-energy cosmic rays with nearby extragalactic objects
- Author
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J. Abraham, P. Abreu, M. Aglietta, C. Aguirre, D. Allard, I. Allekotte, J. Allen, P. Allison, J. Alvarez Muniz, M. Ambrosio, L. Anchordoqui, S. Andringa, A. Anzalone, C. Aramo, S. Argiro', K. Arisaka, E. Armengaud, F. Arneodo, F. Arquero, T. Asch, H. Asorey, P. Assis, B. S. Atulugama, J. Aublin, M. Ave, G. Avila, T. Backer, D. Badagnani, A. F. Barbosa, D. Barnhill, S. L. C. Barroso, P. Bauleo, J. J. Beatty, T. Beau, B. R. Becker, K. H. Becker, J. A. Bellido, S. BenZvi, C. Berat, T. Bergmann, X. Bertou, P. L. Biermann, P. Billoir, O. Blanch Bigas, F. Blanco, P. Blasi, C. Bleve, H. Blumer, M. Bohacova, C. Bonifazi, R. Bonino, M. Boratav, J. Brack, P. Brogueira, W. C. Brown, P. Buchholz, A. Bueno, R. E. Burton, N. G. Busca, K. S. Caballero Mora, B. Cai, D. V. Camin, L. Caramete, R. Caruso, W. Carvalho, A. Castellina, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, A. Chiavassa, J. A. Chinellato, A. Chou, J. Chye, P. D. J. Clark, R. W. Clay, E. Colombo, R. Conceicao, B. Connolly, F. Contreras, J. Coppens, A. Cordier, U. Cotti, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. Cronin, A. Curutiu, S. Dagoret Campagne, K. Daumiller, B. R. Dawson, R. M. de Almeida, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, V. de Souza, L. del Peral, O. Deligny, A. Della Selva, C. Delle Fratte, H. Dembinski, C. Di Giulio, J. C. Diaz, C. Dobrigkeit, J. C. D’Olivo, D. Dornic, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D’Urso, I. Dutan, M. A. DuVernois, R. Engel, L. Epele, M. Erdmann, C. O. Escobar, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Ferrer, S. Ferry, B. Fick, A. Filevich, A. Filipcic, I. Fleck, R. Fonte, C. E. Fracchiolla, W. Fulgione, B. Garcia, D. Garcia Gamez, D. Garcia Pinto, X. Garrido, H. Geenen, G. Gelmini, H. Gemmeke, P. L. Ghia, M. Giller, H. Glass, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gomez Berisso, R. Gomez Herrero, P. Goncalves, M. Goncalves do Amaral, D. Gonzalez, J. G. Gonzalez, M. Gonzalez, D. Gora, A. Gorgi, P. Gouffon, V. Grassi, A. F. Grillo, C. Grunfeld, Y. Guardincerri, F. Guarino, G. P. Guedes, J. Gutierrez, J. D. Hague, J. C. Hamilton, P. Hansen, D. Harari, S. Harmsma, J. L. Harton, A. Haungs, T. Hauschildt, M. D. Healy, T. Hebbeker, G. Hebrero, D. Heck, C. Hojvat, V. C. Holmes, P. Homola, J. Horandel, A. Horneffer, M. Horvat, M. Hrabovsky, T. Huege, M. Hussain, M. Iarlori, A. Insolia, F. Ionita, A. Italiano, M. Kaducak, K. H. Kampert, T. Karova, B. Kegl, B. Keilhauer, E. Kemp, R. M. Kieckhafer, H. O. Klages, M. Kleifges, J. Kleinfeller, R. Knapik, J. Knapp, D. H. Koang, A. Krieger, O. Kromer, D. Kuempel, N. Kunka, A. Kusenko, G. La Rosa, C. Lachaud, B. L. Lago, D. Lebrun, P. Lebrun, J. Lee, M. A. Leigui de Oliveira, A. Letessier Selvon, M. Leuthold, I. Lhenry Yvon, R. Lopez, A. Lopez Aguera, J. Lozano Bahilo, R. Luna Garcia, M. C. Maccarone, C. Macolino, S. Maldera, M. E. Mancenido, D. Mandat, P. Mantsch, A. G. Mariazzi, I. C. Maris, H. R. Marquez Falcon, J. Martinez, O. Martinez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurizio, P. O. Mazur, T. McCauley, M. McEwen, R. R. McNeil, M. C. Medina, G. Medina Tanco, A. Meli, D. Melo, E. Menichetti, A. Menschikov, C.h.r. Meurer, R. Meyhandan, M. I. Micheletti, G. Miele, W. Miller, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, J. C. Moreno, C. Morris, M. Mostafa, M. A. Muller, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, C. Newman Holmes, D. Newton, N. T. Thao, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nozka, J. Oehlschlager, T. Ohnuki, A. Olinto, V. M. Olmos Gilbaja, M. Ortiz, F. Ortolani, S. Ostapchenko, L. Otero, N. Pacheco, D. Pakk Selmi Dei, M. Palatka, J. Pallotta, G. Parente, E. Parizot, S. Parlati, S. Pastor, M. Patel, T. Paul, V. Pavlidou, K. Payet, M. Pech, J. Pekala, R. Pelayo, I. M. Pepe, S. Petrera, P. Petrinca, Y. Petrov, P. N. Diep, P. N. Dong, P. T. Nhung, A. Pichel, R. Piegaia, T. Pierog, M. Pimenta, T. Pinto, V. Pirronello, O. Pisanti, M. Platino, J. Pochon, P. Privitera, M. Prouza, E. J. Quel, J. Rautenberg, A. Redondo, S. Reucroft, B. Revenu, F. A. S. Rezende, J. Ridky, S. Riggi, M. Risse, C. Riviere, V. Rizi, M. Roberts, C. Robledo, G. Rodriguez, M. D. Rodriguez Frias, J. RodriguezMartino, J. Rodriguez Rojo, I. Rodriguez Cabo, G. Ros, J. Rosado, M. Roth, C. Roucelle, B. Rouille' d’Orfeuil, E. Roulet, A. C. Rovero, F. Salamida, H. Salazar, G. Salina, F. Sanchez, M. Santander, C. E. Santo, E. M. Santos, F. Sarazin, S. Sarkar, R. Sato, V. Scherini, H. Schieler, A. Schmidt, F. Schmidt, T. Schmidt, O. Scholten, P. Schovanek, F. Schussler, S. J. Sciutto, M. Scuderi, A. Segreto, D. Semikoz, M. Settimo, R. C. Shellard, I. Sidelnik, B. B. Siffert, G. Sigl, N. Smetniansky De Grande, A. Smialkowski, R. Smida, A. G. K. Smith, B. E. Smith, G. R. Snow, P. Sokolsky, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, E. Strazzeri, A. Stutz, F. Suarez, T. Suomijarvi, A. D. Supanitsky, M. S. Sutherland, J. Swainc, Z. Szadkowski, J. Takahashi, A. Tamashiro, A. Tamburro, O. Tascau, R. Tcaciuc, D. Thomas, R. Ticon, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, B. Tome', A. Tonachini, I. Torres, D. Torresi, P. Travnicek, A. Tripathi, G. Tristram, D. Tscherniakhovski, M. Tueros, V. Tunnicliffe, R. Ulrich, M. Unger, M. Urbana, J. F. Valdes Galicia, I. Valino, L. Valore, A. M. van den Berg, V. van Elewyck, R. A. Vazquez, D. Veberic, A. Veiga, A. Velarde, T. Ventersc, V. Verzi, M. Videl, L. Villasenor, S. Vorobiov, L. Voyvodic, H. Wahlber, O. Wainber, P. Walker, D. Warner, A. A. Watson, S. Westerhoff, G. Wieczorek, L. Wiencke, B. Wilczynska, H. Wilczynski, C. Wileman, M. G. Winnick, H. Wua, B. Wundheiler, T. Yamamoto, P. Younk, E. Zasb, D. Zavrtanik, M. Zavrtanik, A. Zech, A. Zepeda, M. Ziolkowski, BERNARDINI, Paolo, DE MITRI, Ivan, MANCARELLA, Giovanni, MARTELLO, Daniele, PERRONE, Lorenzo, J., Abraham, P., Abreu, M., Aglietta, C., Aguirre, D., Allard, I., Allekotte, J., Allen, P., Allison, J., Alvarez Muniz, M., Ambrosio, L., Anchordoqui, S., Andringa, A., Anzalone, C., Aramo, S., Argiro', K., Arisaka, E., Armengaud, F., Arneodo, F., Arquero, T., Asch, H., Asorey, P., Assi, B. S., Atulugama, J., Aublin, M., Ave, G., Avila, T., Backer, D., Badagnani, A. F., Barbosa, D., Barnhill, S. L. C., Barroso, P., Bauleo, J. J., Beatty, T., Beau, B. R., Becker, K. H., Becker, J. A., Bellido, S., Benzvi, C., Berat, T., Bergmann, Bernardini, Paolo, X., Bertou, P. L., Biermann, P., Billoir, O., Blanch Biga, F., Blanco, P., Blasi, C., Bleve, H., Blumer, M., Bohacova, C., Bonifazi, R., Bonino, M., Boratav, J., Brack, P., Brogueira, W. C., Brown, P., Buchholz, A., Bueno, R. E., Burton, N. G., Busca, K. S., Caballero Mora, B., Cai, D. V., Camin, L., Caramete, R., Caruso, W., Carvalho, A., Castellina, O., Catalano, G., Cataldi, L., Cazon, R., Cester, J., Chauvin, A., Chiavassa, J. A., Chinellato, A., Chou, J., Chye, P. D. J., Clark, R. W., Clay, E., Colombo, R., Conceicao, B., Connolly, F., Contrera, J., Coppen, A., Cordier, U., Cotti, S., Coutu, C. E., Covault, A., Creusot, A., Cri, J., Cronin, A., Curutiu, S., Dagoret Campagne, K., Daumiller, B. R., Dawson, R. M., de Almeida, C., De Donato, S. J., de Jong, G., De La Vega, W. J. M., de Mello Junior, J. R. T., de Mello Neto, DE MITRI, Ivan, V., de Souza, L., del Peral, O., Deligny, A., Della Selva, C., Delle Fratte, H., Dembinski, C., Di Giulio, J. C., Diaz, C., Dobrigkeit, J. C., D’Olivo, D., Dornic, A., Dorofeev, J. C., dos Anjo, M. T., Dova, D., D’Urso, I., Dutan, M. A., Duvernoi, R., Engel, L., Epele, M., Erdmann, C. O., Escobar, A., Etchegoyen, P., Facal San Lui, H., Falcke, G., Farrar, A. C., Fauth, N., Fazzini, F., Ferrer, S., Ferry, B., Fick, A., Filevich, A., Filipcic, I., Fleck, R., Fonte, C. E., Fracchiolla, W., Fulgione, B., Garcia, D., Garcia Gamez, D., Garcia Pinto, X., Garrido, H., Geenen, G., Gelmini, H., Gemmeke, P. L., Ghia, M., Giller, H., Gla, M. S., Gold, G., Golup, F., Gomez Albarracin, M., Gomez Berisso, R., Gomez Herrero, P., Goncalve, M., Goncalves do Amaral, D., Gonzalez, J. G., Gonzalez, M., Gonzalez, D., Gora, A., Gorgi, P., Gouffon, V., Grassi, A. F., Grillo, C., Grunfeld, Y., Guardincerri, F., Guarino, G. P., Guede, J., Gutierrez, J. D., Hague, J. C., Hamilton, P., Hansen, D., Harari, S., Harmsma, J. L., Harton, A., Haung, T., Hauschildt, M. D., Healy, T., Hebbeker, G., Hebrero, D., Heck, C., Hojvat, V. C., Holme, P., Homola, J., Horandel, A., Horneffer, M., Horvat, M., Hrabovsky, T., Huege, M., Hussain, M., Iarlori, A., Insolia, F., Ionita, A., Italiano, M., Kaducak, K. H., Kampert, T., Karova, B., Kegl, B., Keilhauer, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, R., Knapik, J., Knapp, D. H., Koang, A., Krieger, O., Kromer, D., Kuempel, N., Kunka, A., Kusenko, G., La Rosa, C., Lachaud, B. L., Lago, D., Lebrun, P., Lebrun, J., Lee, M. A., Leigui de Oliveira, A., Letessier Selvon, M., Leuthold, I., Lhenry Yvon, R., Lopez, A., Lopez Aguera, J., Lozano Bahilo, R., Luna Garcia, M. C., Maccarone, C., Macolino, S., Maldera, Mancarella, Giovanni, M. E., Mancenido, D., Mandat, P., Mantsch, A. G., Mariazzi, I. C., Mari, H. R., Marquez Falcon, Martello, Daniele, J., Martinez, O., Martinez Bravo, H. J., Mathe, J., Matthew, J. A. J., Matthew, G., Matthiae, D., Maurizio, P. O., Mazur, T., Mccauley, M., Mcewen, R. R., Mcneil, M. C., Medina, G., Medina Tanco, A., Meli, D., Melo, E., Menichetti, A., Menschikov, Meurer, C. h. r., R., Meyhandan, M. I., Micheletti, G., Miele, W., Miller, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, B., Morale, C., Morello, J. C., Moreno, C., Morri, M., Mostafa, M. A., Muller, R., Mussa, G., Navarra, J. L., Navarro, S., Nava, P., Necesal, L., Nellen, C., Newman Holme, D., Newton, N. T., Thao, N., Nierstenhoefer, D., Nitz, D., Nosek, L., Nozka, J., Oehlschlager, T., Ohnuki, A., Olinto, V. M., Olmos Gilbaja, M., Ortiz, F., Ortolani, S., Ostapchenko, L., Otero, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, G., Parente, E., Parizot, S., Parlati, S., Pastor, M., Patel, T., Paul, V., Pavlidou, K., Payet, M., Pech, J., Pekala, R., Pelayo, I. M., Pepe, Perrone, Lorenzo, S., Petrera, P., Petrinca, Y., Petrov, P. N., Diep, P. N., Dong, P. T., Nhung, A., Pichel, R., Piegaia, T., Pierog, M., Pimenta, T., Pinto, V., Pirronello, O., Pisanti, M., Platino, J., Pochon, P., Privitera, M., Prouza, E. J., Quel, J., Rautenberg, A., Redondo, S., Reucroft, B., Revenu, F. A. S., Rezende, J., Ridky, S., Riggi, M., Risse, C., Riviere, V., Rizi, M., Robert, C., Robledo, G., Rodriguez, M. D., Rodriguez Fria, J., Rodriguezmartino, J., Rodriguez Rojo, I., Rodriguez Cabo, G., Ro, J., Rosado, M., Roth, C., Roucelle, B., Rouille' d’Orfeuil, E., Roulet, A. C., Rovero, F., Salamida, H., Salazar, G., Salina, F., Sanchez, M., Santander, C. E., Santo, E. M., Santo, F., Sarazin, S., Sarkar, R., Sato, V., Scherini, H., Schieler, A., Schmidt, F., Schmidt, T., Schmidt, O., Scholten, P., Schovanek, F., Schussler, S. J., Sciutto, M., Scuderi, A., Segreto, D., Semikoz, M., Settimo, R. C., Shellard, I., Sidelnik, B. B., Siffert, G., Sigl, N., Smetniansky De Grande, A., Smialkowski, R., Smida, A. G. K., Smith, B. E., Smith, G. R., Snow, P., Sokolsky, P., Sommer, J., Sorokin, H., Spinka, R., Squartini, E., Strazzeri, A., Stutz, F., Suarez, T., Suomijarvi, A. D., Supanitsky, M. S., Sutherland, J., Swainc, Z., Szadkowski, J., Takahashi, A., Tamashiro, A., Tamburro, O., Tascau, R., Tcaciuc, D., Thoma, R., Ticon, J., Tiffenberg, C., Timmerman, W., Tkaczyk, C. J., Todero Peixoto, B., Tome', A., Tonachini, I., Torre, D., Torresi, P., Travnicek, A., Tripathi, G., Tristram, D., Tscherniakhovski, M., Tuero, V., Tunnicliffe, R., Ulrich, M., Unger, M., Urbana, J. F., Valdes Galicia, I., Valino, L., Valore, A. M., van den Berg, V., van Elewyck, R. A., Vazquez, D., Veberic, A., Veiga, A., Velarde, T., Ventersc, V., Verzi, M., Videl, L., Villasenor, S., Vorobiov, L., Voyvodic, H., Wahlber, O., Wainber, P., Walker, D., Warner, A. A., Watson, S., Westerhoff, G., Wieczorek, L., Wiencke, B., Wilczynska, H., Wilczynski, C., Wileman, M. G., Winnick, H., Wua, B., Wundheiler, T., Yamamoto, P., Younk, E., Zasb, D., Zavrtanik, M., Zavrtanik, A., Zech, A., Zepeda, M., Ziolkowski, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), APC - Cosmologie, APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), Laboratory for Astroparticle Physics, University of Nova Gorica, PIERRE AUGER, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Guarino, Fausto, D'Urso, Domenico, Aramo, Carla, DELLA SELVA, Angelo, Miele, Gennaro, Pisanti, Ofelia, Valore, Laura, Auger, Collaboration, KVI - Center for Advanced Radiation Technology, and Research unit Astroparticle Physics
- Subjects
Active galactic nucleus ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astronomy ,Astrophysics::High Energy Astrophysical Phenomena ,particle source [cosmic radiation] ,Cosmic background radiation ,FOS: Physical sciences ,Flux ,Osservatorio Pierre Auger ,Cosmic ray ,anisotropy ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Raggi cosmici ,0103 physical sciences ,Ultra-high-energy cosmic ray ,010303 astronomy & astrophysics ,Background radiation ,Nuclei galattivi attivi ,Physics ,Pierre Auger Observatory ,SPECTRUM ,Multidisciplinary ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,Medicine (all) ,Settore FIS/01 - Fisica Sperimentale ,Astrophysics (astro-ph) ,angular dependence [cosmic radiation] ,Astrophysics::Instrumentation and Methods for Astrophysics ,Física ,Energia ultra alta ,Experimental High Energy Physics ,ddc:500 ,Energy (signal processing) ,experimental results - Abstract
Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources., Comment: 22 pages, 2 figures
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32. The Adventure of Science.Benjamin GinzburgThe History of Science and the New Humanism.George SartonScience and First Principles.F. S. C. NorthropThe Logic of Science.Harold R. SmartNumber, the Language of Science.Tobias DantzigStudies in the Literature of Natural Science.Julian M. Drachman
- Author
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H. Blumer
- Subjects
Sociology and Political Science ,GEORGE (programming language) ,Philosophy ,Natural science ,Social science ,Humanism ,Adventure ,History of science ,Classics - Published
- 1932
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33. L'opinion publique d’après les enquêtes par sondages
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H. Blumer
- Published
- 1981
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34. [How does one become an infant health counseling nurse?]
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H, Blumer
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Primary Prevention ,Education, Nursing, Continuing ,Infant Care ,Humans ,Infant ,Switzerland - Published
- 1985
35. Preparatory procedures for videotaped feedback to improve social skills
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Craig H. Blumer and J. Regis McNamara
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Male ,Social skills ,education ,Pedagogy ,Applied psychology ,Psychotherapy, Group ,Humans ,Videotape Recording ,Female ,Interpersonal Relations ,Psychology ,General Psychology ,Feedback - Abstract
Videotaped feedback in conjunction with group approaches which utilized didactic lectures, behavioral problem solving, or group exercises to increase cohesion were compared to ascertain their effectiveness in improving social skills for undergraduates. Self-report, partners' evaluations, and independent observers' ratings indicated that group treatment coupled with feedback nondifferentially improved social skills over time. For undergraduates undergoing brief social skills training, differences in subjects' preparation involving videotape feedback may not produce corresponding differences in subjects' behavior.
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- 1985
36. [Profession and professional image. No more acting in the background]
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H, Blumer
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Adult ,Counseling ,Professional Competence ,Child, Preschool ,Child Health Services ,Humans ,Infant ,Mothers ,Female ,Child Care ,Switzerland - Published
- 1985
37. Where lies the future?
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H, Blumer
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Nursing ,United Kingdom ,Specialization - Published
- 1971
38. Viral hepatitis
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C, BLACKWELL and H, BLUMER
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Hepatitis, Viral, Human ,Humans ,Hepatitis A ,Communicable Diseases ,Hepatitis - Published
- 1955
39. Respiratory therapy for seasonal allergic rhinitis and asthma
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H, BLUMER, A, LEZNOFF, F, CUA-LIM, P, DELORME, and B, ROSE
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Adult ,Male ,Respiratory Therapy ,Humans ,Pollen ,Rhinitis, Allergic, Seasonal ,Female ,Seasons ,Original Articles ,Allergens ,Rhinitis, Allergic ,Asthma - Abstract
Repository therapy with an emulsified antigen preparation for pollen asthma and hay fever was used over the past three years. Overall results indicate that the response in the majority of patients was as good as that obtained with conventional preseasonal or perennial treatment. Reactions were noted in four of the 15 patients so treated during the first year of study, in 25 of 58 patients treated in the second year, and in 11 of 175 treated in the final year. These varied from mild to severe systemic reactions, some of which required hospitalization. With improvement and modification of the technique, such as the administration of the antigen in two injections rather than in a single injection, the incidence and severity of reactions were markedly reduced. The procedure is not without hazard; it requires great care, and initial experience is best obtained in a hospital environment.
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- 1962
40. Precipitating and non precipitating antibodies in the primary and secondary immune responses. Rate of decline, anaphysensitizing capacity, and the effect of cortisone
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H, BLUMER, M, RICHTER, F, CUA-LIM, and B, ROSE
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Cortisone ,Immunologic Memory ,Antibodies - Published
- 1962
41. Physicochemical studies on precipitat ing and non-precipitating antibodies after primary immunization
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M, RICHTER, H, BLUMER, F, CUA-LIM, and B, ROSE
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Immune Sera ,Vaccination ,Immunization ,Antibodies - Published
- 1962
42. [Influence of monoiodoacetic acid, sodium azide and sodium iodate on the resting potential and electroretinogram of the frog eye]
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W, MULLER-LIMMROTH and H, BLUMER
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Azides ,Electroretinography ,Iodates ,Animals ,Iodoacetates ,Anura ,Iodides ,Eye ,Sodium Azide ,Iodine ,Iodoacetic Acid ,Membrane Potentials - Published
- 1957
43. The NANOGrav 12.5 yr Data Set: The Frequency Dependence of Pulse Jitter in Precision Millisecond Pulsars.
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M. T. Lam, M. A. McLaughlin, Z. Arzoumanian, H. Blumer, P. R. Brook, H. T. Cromartie, P. B. Demorest, M. E. DeCesar, T. Dolch, J. A. Ellis, R. D. Ferdman, E. C. Ferrara, E. Fonseca, N. Garver-Daniels, P. A. Gentile, M. L. Jones, D. R. Lorimer, R. S. Lynch, C. Ng, and D. J. Nice
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PULSARS ,GRAVITATIONAL wave astronomy ,SIGNAL-to-noise ratio ,SCINTILLATION of stars ,SCATTERING (Physics) - Abstract
Low-frequency gravitational-wave experiments require the highest timing precision from an array of the most stable millisecond pulsars. Several known sources of noise on short timescales in single radio pulsar observations are well described by a simple model of three components: template fitting from a finite signal-to-noise ratio, pulse phase/amplitude jitter from single-pulse stochasticity, and scintillation errors from short-timescale interstellar scattering variations. Currently template-fitting errors dominate, but as radio telescopes push toward higher signal-to-noise ratios, jitter becomes the next dominant term for most millisecond pulsars. Understanding the statistics of jitter becomes crucial for properly characterizing arrival time uncertainties. We characterize the radio frequency dependence of jitter using data on 48 pulsars in the North American Nanohertz Observatory for Gravitational Waves timing program. We detect significant jitter in 43 of the pulsars and test several functional forms for its frequency dependence; we find significant frequency dependence for 30 pulsars. We find moderate correlations of rms jitter with pulse width (R = 0.62) and number of profile components (R = 0.40); the single-pulse rms jitter is typically ≈1% of pulse phase. The average frequency dependence for all pulsars using a power-law model has index −0.42. We investigate the jitter variations for the interpulse of PSR B1937+21 and find no significant deviations from the main pulse rms jitter. We also test the time variation of jitter in two pulsars and find that systematics likely bias the results for high-precision pulsars. Pulsar timing array analyses must properly model jitter as a significant component of the noise within the detector. [ABSTRACT FROM AUTHOR]
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- 2019
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44. A History of Science.William Cecil Dampier-Whetham
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H. Blumer
- Subjects
Sociology and Political Science ,media_common.quotation_subject ,Art ,History of science ,Classics ,media_common - Published
- 1930
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45. General Psychology for Professional Students.A. R. Gilliland , John J. B. Morgan, S. N. Stevens
- Author
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H. Blumer
- Subjects
Psychoanalysis ,Sociology and Political Science ,General psychology ,Psychology - Published
- 1932
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46. An Introduction to Human Problems.Harold Benjamin
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H. Blumer
- Subjects
Sociology and Political Science - Published
- 1932
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47. A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747.
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M. T. Lam, J. A. Ellis, G. Grillo, M. L. Jones, J. S. Hazboun, P. R. Brook, J. E. Turner, S. Chatterjee, J. M. Cordes, T. J. W. Lazio, M. E. DeCesar, Z. Arzoumanian, H. Blumer, H. T. Cromartie, P. B. Demorest, T. Dolch, R. D. Ferdman, E. C. Ferrara, E. Fonseca, and N. Garver-Daniels
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INTERSTELLAR medium ,ASTROPHYSICS ,DISPERSION (Chemistry) ,SOLAR radio emission ,RADIO pulse time modulation - Abstract
The frequency dependence of radio pulse arrival times provides a probe of structures in the intervening media. Demorest et al. was the first to show a short-term (∼100–200 days) reduction in the electron content along the line of sight to PSR J1713+0747 in data from 2008 (approximately MJD 54750) based on an apparent dip in the dispersion measure of the pulsar. We report on a similar event in 2016 (approximately MJD 57510), with average residual pulse-arrival times ≈−3.0, −1.3, and −0.7 μs at 820, 1400, and 2300 MHz, respectively. Timing analyses indicate possible departures from the standard ν
−2 dispersive-delay dependence. We discuss and rule out a wide variety of potential interpretations. We find the likeliest scenario to be lensing of the radio emission by some structure in the interstellar medium, which causes multiple frequency-dependent pulse arrival-time delays. [ABSTRACT FROM AUTHOR]- Published
- 2018
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48. Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
- Author
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P. Abreu, M. Aglietta, M. Ahlers, E. J. Ahn, I. F. M. Albuquerque, D. Allard, I. Allekotte, J. Allen, P. Allison, A. Almela, J. Alvarez Castillo, J. Alvarez-Muñiz, R. Alves Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, T. Antičić, C. Aramo, E. Arganda, F. Arqueros, H. Asorey, P. Assis, J. Aublin, M. Ave, M. Avenier, G. Avila, T. Bäcker, A. M. Badescu, M. Balzer, K. B. Barber, A. F. Barbosa, R. Bardenet, S. L. C. Barroso, B. Baughman, J. Bäuml, J. J. Beatty, B. R. Becker, K. H. Becker, A. Bellétoile, J. A. Bellido, S. BenZvi, C. Berat, X. Bertou, P. L. Biermann, P. Billoir, F. Blanco, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancus, P. Brogueira, W. C. Brown, R. Bruijn, P. Buchholz, A. Bueno, R. E. Burton, K. S. Caballero-Mora, B. Caccianiga, L. Caramete, R. Caruso, A. Castellina, O. Catalano, G. Cataldi, L. Cazon, R. Cester, J. Chauvin, S. H. Cheng, A. Chiavassa, J. A. Chinellato, J. Chirinos Diaz, J. Chudoba, M. Cilmo, R. W. Clay, M. R. Coluccia, R. Conceição, F. Contreras, H. Cook, M. J. Cooper, J. Coppens, A. Cordier, S. Coutu, C. E. Covault, A. Creusot, A. Criss, J. Cronin, A. Curutiu, S. Dagoret-Campagne, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de Almeida, M. De Domenico, C. De Donato, S. J. de Jong, G. De La Vega, W. J. M. de Mello Junior, J. R. T. de Mello Neto, I. De Mitri, V. de Souza, K. D. de Vries, L. del Peral, M. del Río, O. Deligny, H. Dembinski, N. Dhital, C. Di Giulio, M. L. Díaz Castro, P. N. Diep, F. Diogo, C. Dobrigkeit, W. Docters, J. C. D'Olivo, P. N. Dong, A. Dorofeev, J. C. dos Anjos, M. T. Dova, D. D'Urso, I. Dutan, J. Ebr, R. Engel, M. Erdmann, C. O. Escobar, J. Espadanal, A. Etchegoyen, P. Facal San Luis, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, A. P. Ferguson, B. Fick, A. Filevich, A. Filipčič, S. Fliescher, C. E. Fracchiolla, E. D. Fraenkel, O. Fratu, U. Fröhlich, B. Fuchs, R. Gaior, R. F. Gamarra, S. Gambetta, B. García, S. T. Garcia Roca, D. Garcia-Gamez, D. Garcia-Pinto, A. Gascon Bravo, H. Gemmeke, P. L. Ghia, M. Giller, J. Gitto, H. Glass, M. S. Gold, G. Golup, F. Gomez Albarracin, M. Gómez Berisso, P. F. Gómez Vitale, P. Gonçalves, J. G. Gonzalez, B. Gookin, A. Gorgi, P. Gouffon, E. Grashorn, S. Grebe, N. Griffith, M. Grigat, A. F. Grillo, Y. Guardincerri, F. Guarino, G. P. Guedes, P. Hansen, D. Harari, T. A. Harrison, J. L. Harton, A. Haungs, T. Hebbeker, D. Heck, A. E. Herve, C. Hojvat, N. Hollon, V. C. Holmes, P. Homola, J. R. Hörandel, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, F. Ionita, A. Italiano, C. Jarne, S. Jiraskova, M. Josebachuili, K. Kadija, K. H. Kampert, P. Karhan, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, J. L. Kelley, E. Kemp, R. M. Kieckhafer, H. O. Klages, M. Kleifges, J. Kleinfeller, J. Knapp, D.-H. Koang, K. Kotera, N. Krohm, O. Krömer, D. Kruppke-Hansen, F. Kuehn, D. Kuempel, J. K. Kulbartz, N. Kunka, G. La Rosa, C. Lachaud, D. LaHurd, L. Latronico, R. Lauer, P. Lautridou, S. Le Coz, M. S. A. B. Leão, D. Lebrun, P. Lebrun, M. A. Leigui de Oliveira, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. Lopez Agüera, K. Louedec, J. Lozano Bahilo, L. Lu, A. Lucero, M. Ludwig, H. Lyberis, M. C. Maccarone, C. Macolino, S. Maldera, D. Mandat, P. Mantsch, A. G. Mariazzi, J. Marin, V. Marin, I. C. Maris, H. R. Marquez Falcon, G. Marsella, D. Martello, L. Martin, H. Martinez, O. Martínez Bravo, H. J. Mathes, J. Matthews, J. A. J. Matthews, G. Matthiae, D. Maurel, D. Maurizio, P. O. Mazur, G. Medina-Tanco, M. Melissas, D. Melo, E. Menichetti, A. Menshikov, P. Mertsch, C. Meurer, S. Mićanović, M. I. Micheletti, I. A. Minaya, L. Miramonti, L. Molina-Bueno, S. Mollerach, M. Monasor, D. Monnier Ragaigne, F. Montanet, B. Morales, C. Morello, E. Moreno, J. C. Moreno, M. Mostafá, C. A. Moura, M. A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra, J. L. Navarro, S. Navas, P. Necesal, L. Nellen, A. Nelles, J. Neuser, P. T. Nhung, M. Niechciol, L. Niemietz, N. Nierstenhoefer, D. Nitz, D. Nosek, L. Nožka, J. Oehlschläger, A. Olinto, M. Ortiz, N. Pacheco, D. Pakk Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, G. Parente, E. Parizot, A. Parra, S. Pastor, T. Paul, M. Pech, J. Pękala, R. Pelayo, I. M. Pepe, L. Perrone, R. Pesce, E. Petermann, S. Petrera, A. Petrolini, Y. Petrov, C. Pfendner, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, V. H. Ponce, M. Pontz, A. Porcelli, P. Privitera, M. Prouza, E. J. Quel, S. Querchfeld, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, H. Rivera, V. Rizi, J. Roberts, W. Rodrigues de Carvalho, G. Rodriguez, I. Rodriguez Cabo, J. Rodriguez Martino, J. Rodriguez Rojo, M. D. Rodríguez-Frías, G. Ros, J. Rosado, T. Rossler, M. Roth, B. Rouillé-d'Orfeuil, E. Roulet, A. C. Rovero, C. Rühle, A. Saftoiu, F. Salamida, H. Salazar, F. Salesa Greus, G. Salina, F. Sánchez, C. E. Santo, E. Santos, E. M. Santos, F. Sarazin, B. Sarkar, S. Sarkar, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, A. Schmidt, O. Scholten, H. Schoorlemmer, J. Schovancova, P. Schovánek, F. Schröder, S. Schulte, D. Schuster, S. J. Sciutto, M. Scuderi, A. Segreto, M. Settimo, A. Shadkam, R. C. Shellard, I. Sidelnik, G. Sigl, O. Sima, A. Śmiałkowski, R. Šmída, G. R. Snow, P. Sommers, J. Sorokin, H. Spinka, R. Squartini, Y. N. Srivastava, S. Stanic, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A. D. Supanitsky, T. Šuša, M. S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, A. Tapia, M. Tartare, O. Taşcău, R. Tcaciuc, N. T. Thao, D. Thomas, J. Tiffenberg, C. Timmermans, W. Tkaczyk, C. J. Todero Peixoto, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, P. Travnicek, D. B. Tridapalli, G. Tristram, E. Trovato, M. Tueros, R. Ulrich, M. Unger, M. Urban, J. F. Valdés Galicia, I. Valiño, L. Valore, A. M. van den Berg, E. Varela, B. Vargas Cárdenas, J. R. Vázquez, R. A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, H. Wahlberg, P. Wahrlich, O. Wainberg, D. Walz, A. A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, S. Westerhoff, B. J. Whelan, A. Widom, G. Wieczorek, L. Wiencke, B. Wilczyñska, H. Wilczyñski, M. Will, C. Williams, T. Winchen, M. Wommer, B. Wundheiler, T. Yamamoto, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano Garcia, E. Zas, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, Y. Zhu, M. Zimbres Silva, and M. Ziolkowski
- Subjects
Physics ,QC1-999 - Abstract
The observation of ultrahigh energy neutrinos (UHEνs) has become a priority in experimental astroparticle physics. UHEνs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going ν) or in the Earth crust (Earth-skimming ν), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and criteria established to search for UHEνs in the data collected with the ground array of the Pierre Auger Observatory. This includes Earth-skimming as well as downward-going neutrinos. No neutrino candidates have been found, which allows us to place competitive limits to the diffuse flux of UHEνs in the EeV range and above.
- Published
- 2013
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49. Censorship of the Theater and Moving Pictures.Lamar T. Beman
- Author
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H. Blumer
- Subjects
Sociology and Political Science ,media_common.quotation_subject ,Censorship ,Media studies ,Advertising ,Art ,media_common - Published
- 1932
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50. A History of Psychology in Autobiography.Carl Murchison
- Author
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H. Blumer
- Subjects
Murchison meteorite ,Sociology and Political Science ,History of psychology ,Art history ,Biography ,Psychology - Published
- 1932
- Full Text
- View/download PDF
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