A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

Observations of cosmic rays arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Veron-Cetty Veron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt-L, 2pt+ and 3pt methods, each giving a different measure of self-clustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structure as ordinary galaxies in the local Universe and if UHECRs are deflected no more than a few degrees, a study of mock maps suggests that these three method can efficiently respond to the resulting anisotropy with a P-value = 1.0% or smaller with data sets as few as 100 events. using data taken from January 1, 2004 to July 31, 2010 we examined the 20, 30, ... , 110 highest energy events with a corresponding minimum energy threshold of about 49.3 EeV. The minimum P-values found were 13.5% using the 2pt-L method, 1.0% using the 2pt+ method and 1.1% using the 3pt method for the highest 100 energy events. In view of the multiple (correlated) scans performed on the data set, these catalog-independent methods do not yield strong evidence of anisotropy in the highest energy cosmic rays.

Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargue and averaged monthly models, the utility of the GDAS data is shown. (C) 2012 Elsevier B.V. All rights reserved.

Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna sensor. As the ultra-wideband reception of pulses is not widely discussed in antenna literature, we review the relevant antenna characteristics and enhance theoretical considerations towards the impulse response of antennas including polarization effects and multiple signal reflections. On the basis of the vector effective length we study the transient response characteristics of three candidate antennas in the time domain. Observing the variation of the continuous galactic background intensity we rank the antennas with respect to the noise level added to the galactic signal.

The rapid atmospheric monitoring system of the Pierre Auger Observatory

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10(17) eV. During clear nights with a low illuminated moon fraction, the UV fluorescence light produced by air showers is recorded by optical telescopes at the Observatory. To correct the observations for variations in atmospheric conditions, atmospheric monitoring is performed at regular intervals ranging from several minutes (for cloud identification) to several hours (for aerosol conditions) to several days (for vertical profiles of temperature, pressure, and humidity). In 2009, the monitoring program was upgraded to allow for additional targeted measurements of atmospheric conditions shortly after the detection of air showers of special interest, e. g., showers produced by very high-energy cosmic rays or showers with atypical longitudinal profiles. The former events are of particular importance for the determination of the energy scale of the Observatory, and the latter are characteristic of unusual air shower physics or exotic primary particle types. The purpose of targeted (or "rapid") monitoring is to improve the resolution of the atmospheric measurements for such events. In this paper, we report on the implementation of the rapid monitoring program and its current status. The rapid monitoring data have been analyzed and applied to the reconstruction of air showers of high interest, and indicate that the air fluorescence measurements affected by clouds and aerosols are effectively corrected using measurements from the regular atmospheric monitoring program. We find that the rapid monitoring program has potential for supporting dedicated physics analyses beyond the standard event reconstruction.

SEARCH FOR POINT-LIKE SOURCES OF ULTRA-HIGH ENERGY NEUTRINOS AT THE PIERRE AUGER OBSERVATORY AND IMPROVED LIMIT ON THE DIFFUSE FLUX OF TAU NEUTRINOS

The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy E-nu between 10(17) eV and 10(20) eV from point-like sources across the sky south of +55 degrees and north of -65 degrees declinations. A search has been performed for highly inclined extensive air showers produced by the interaction of neutrinos of all flavors in the atmosphere (downward-going neutrinos), and by the decay of tau leptons originating from tau neutrino interactions in Earth's crust (Earth-skimming neutrinos). No candidate neutrinos have been found in data up to 2010 May 31. This corresponds to an equivalent exposure of similar to 3.5 years of a full surface detector array for the Earth-skimming channel and similar to 2 years for the downward-going channel. An improved upper limit on the diffuse flux of tau neutrinos has been derived. Upper limits on the neutrino flux from point-like sources have been derived as a function of the source declination. Assuming a differential neutrino flux k(PS) . E-nu(-2). from a point-like source, 90% confidence level upper limits for k(PS) at the level of approximate to 5x10(-7) and 2.5x10(-6) GeV cm(-2) s(-1) have been obtained over a broad range of declinations from the searches for Earth-skimming and downward-going neutrinos, respectively.

LARGE-SCALE DISTRIBUTION OF ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE 10(18) eV AT THE PIERRE AUGER OBSERVATORY

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 10(18) eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 10(18) eV from stationary Galactic sources densely distributed in the Galactic disk and predominantly emitting light particles in all directions.

Measurement of the proton-air cross section at root s=57 TeV with the Pierre Auger Observatory

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505 +/- 22(stat)(-36)(+28)(syst)] mb is found.

Autologous hematopoietic stem cell transplantation vs intravenous pulse cyclophosphamide in diffuse cutaneous systemic sclerosis: a randomized clinical trial

IMPORTANCE High-dose immunosuppressive therapy and autologous hematopoietic stem cell transplantation (HSCT) have shown efficacy in systemic sclerosis in phase 1 and small phase 2 trials. OBJECTIVE To compare efficacy and safety of HSCT vs 12 successive monthly intravenous pulses of cyclophosphamide. DESIGN, SETTING, AND PARTICIPANTS The Autologous Stem Cell Transplantation International Scleroderma (ASTIS) trial, a phase 3, multicenter, randomized (1:1), open-label, parallel-group, clinical trial conducted in 10 countries at 29 centers with access to a European Group for Blood and Marrow Transplantation-registered transplant facility. From March 2001 to October 2009, 156 patients with early diffuse cutaneous systemic sclerosis were recruited and followed up until October 31, 2013. INTERVENTIONS HSCT vs intravenous pulse cyclophosphamide. MAIN OUTCOMES AND MEASURES The primary end point was event-free survival, defined as time from randomization until the occurrence of death or persistent major organ failure. RESULTS A total of 156 patients were randomly assigned to receive HSCT (n = 79) or cyclophosphamide (n = 77). During a median follow-up of 5.8 years, 53 events occurred: 22 in the HSCT group (19 deaths and 3 irreversible organ failures) and 31 in the control group (23 deaths and 8 irreversible organ failures). During the first year, there were more events in the HSCT group (13 events [16.5%], including 8 treatment-related deaths) than in the control group (8 events [10.4%], with no treatment-related deaths). At 2 years, 14 events (17.7%) had occurred cumulatively in the HSCT group vs 14 events (18.2%) in the control group; at 4 years, 15 events (19%) had occurred cumulatively in the HSCT group vs 20 events (26%) in the control group. Time-varying hazard ratios (modeled with treatment × time interaction) for event-free survival were 0.35 (95% CI, 0.16-0.74) at 2 years and 0.34 (95% CI, 0.16-0.74) at 4 years. CONCLUSIONS AND RELEVANCE Among patients with early diffuse cutaneous systemic sclerosis, HSCT was associated with increased treatment-related mortality in the first year after treatment. However, HCST conferred a significant long-term event-free survival benefit. TRIAL REGISTRATION isrctn.org Identifier: ISRCTN54371254.

Na 1 Nachlass Max Horkheimer, 42 - Korrespondenzen u.a. mit Kurt Pinthus (p. I 21, 1-130)

1 Brief von Max Horkheimer an Pierre van Paassen, 31.01.1944; 1 Brief von Max Horkheimer an Frederick M. Padelford, 25.03.1941; 1 Exposé und Beilage von Karl O. Paetel sowie sowie Briefwechsel mit Karl A. Wittfogel; 2 Briefe zwischen Karl A. Wittfogel und Margot von Mendelssohn, 01.06.1941, 04.06.1941; 2 Briefe von Max Horkheimer an D. D. Paige, August 1944; 2 Briefe zwischen Maria Pape und Max Horkheimer, 23.07.1949, 29.07.1949; 1 Brief von Fritz Pappenheim an Max Horkheimer, 11.03.1939; 2 Briefe zwischen Claire Patek-Hohenadl und Max Horkheimer, 18.02.1945, 02.03.1945; 4 Briefe zwischen Wilhelm Pauck und Max Horkheimer, 1938; 2 Briefe von Max Horkheimer an Thomas Peardon, September 1941; 2 Briefe zwischen Christine Peck und Max Horkheimer, 01.02.1944, 16.02.1944; 2 Briefe zwischen Alexander H. Pekelis und Max Horkheimer, 20.10.1941, 29.10.1941; 4 Briefe zwischen Pendle Hill Wallingford und Max Horkheimer, 21.05.1940, 1940; 1 Einladung von The People Lobby an Max Horkheimer, April 1937; 1 Brief von Franz L. Neumann an Selig Perlman, 08.10.1941; 2 Briefe zwischen Florence Pfleger und Max Horkheimer, 30.10.1944, 06.11.1944; 2 Briefe zwischen The Philharmonic-Symphony Society of New York und Max Horkheimer, 11.06.1936, 22.06.1936; 2 Briefe zwischen Philosophical Library New York und Max Horkheimer, 09.09.1941; 2 Briefe von Max Horkheimer an Donald A. Piatt, Oktober 1940; 1 Brief von Max Horkheimer an Alfred Pinkus, 27.08.1942; 20 Briefe und Beilage zwischen Kurt Pinthus und Max Horkheimer, 1940-1942; 1 Brief von Friedrich Pollock an das American Consul General Berlin, 20.05.1941; 1 Brief von Friedrich Pollock an den National Refugee Service New York, 30.04.1941; 4 Briefe zwischen The Emergency Committee in Aid of Displaced Foreign Scholars, New York und Friedrich Pollock, 27.09.1940-1941; 1 Brief von Max Horkheimer an John Simon Guggeheim von der Memorial Foundation, 08.11.1940; 3 Brief zwischen Robert Plank und Max Horkheimer, 12.07.1944, 1944; 4 Briefe und 1 Beilage zwischen Richard S. Plant und Max Horkheimer, Januar 1939; 2 Briefe zwischen Caroline S. Platt und Max Horkheimer, 06.05.1942, 08.05.1942; 1 Brief und 2 Beilagen vom Pledge for Peace Committee New York an Max Horkheimer, 10.04.1944; 1 Brief vom Popular Publications, Inc. New York an Mein, 23.10.1939; 2 Briefe von Else Heim an die Popular Publikations, Inc. New York, 1939; 1 Brief und 1 Beilage von Frederick Pollock an Leonard Powers, 03.06.1941; 2 Briefe zwischen S. Pressburger udn Max Horkheimer, 18.06.1939, 05.07.1939; 2 Briefe zwsichen dem Preston Hotel, Swampscott und Max Horkheimer, 28.04.1937, 08.05.1937; 1 Brief von Lucio José F. Weil an das Preston Hotel, Swampscott, 25.06.1936; 5 Briefe zwischen F. V. Preve und Max Horkheimer, 1937; 4 Briefe zwischen Rena Proulx und Max Horkheimer, 1934, 1937; 2 Briefe zwischen dem Psychatry Journal of the Biology and the Pathology of Interpersonal Relations Washington und Max Horkheimer, 21.08.1939, 11.09.1939;

A “REVOLTA” DE JEÚ E A ESTELA DE DÃ: Um Estudo Em 2 Reis 10,28-36

A pesquisa tem por objetivo trabalhar o evento da Revolta de Jeú, em conjunto com a Estela de Dã, tendo como ponto de partida para tal, a exegese da perícope de 2 Reis 10-28,36. A história Deuteronomista apresenta o ato da Revolta de Jeú como sendo um feito demasiadamente importante, na restauração do culto a Javé em Israel, a partir de um contexto onde o culto a outras divindades, em Israel Norte, estava em pleno curso. No entanto, a partir da análise conjunta da Estela de Dã, que tem como provável autor o rei Hazael de Damasco, somos desafiados a ler esta história pelas entrelinhas não contempladas pelo texto, que apontam para uma participação ativa de Hazael, nos desfechos referentes a Revolta de Jeú, como sendo o responsável direto que proporcionou a subida de Jeú ao trono em Israel, clarificando desta forma este importante período na história Bíblica. Para tal análise, observar-se-á três distintos tópicos, ligados diretamente ao tema proposto: (1) A Revolta de Jeú e a Redação Deuteronomista, a partir do estudo exegético da perícope de 2 Reis 10,28-36, onde estão descritas informações pontuais sobre período em que Jeú reinou em Israel; (2) Jeú e a Estela de Dã, a partir da apresentação e análise do conteúdo da Estela de Dã, tratando diretamente dos desdobramentos da guerra em Ramote de Gileade, de onde se dá o ponto de partida à Revolta de Jeú; e por fim (3) O Império da Síria, onde a partir da continuidade da análise do conteúdo da Estela de Dã, demonstraremos a significância deste reino, além de apontamentos diretamente ligados ao reinado de Hazael, personagem mui relevante no evento da Revolta de Jeú.

Collection complète des œuvres /

Livr. [44] without t.p. and preliminary commentaries.

Antwerpsch archievenblad uitg. op last van het gemeentebestuur.

Archivists: v. 1-20, P. Génard; v. 21- F. Jos van den Branden.

Historie van het leven en sterven van Heer Johan van Oldenbarnevelt ... Waerachtelijek beschreven door een liefhebber der waarheydt.

Contains also"Eenige opmerckingen, memorien, notitien, ende consideratien, tegens den inhouldt van de pretense, ende gansch ongesondeerde, sententie, op den 13 May, 1619, tegens den Heere Iohan van Olden-Barnevelt..."

Precis of the archives of the Cape of Good Hope

Vol. 18-20 have imprint: Cape Town : South African Library.

Jaarboek van het mijnwegen in Nederlandsch-Indië.

"Verhandlingen" for 1915-16, 1918-19, 1925,1927,1929- include section: Geologische overzichtskaart van den Nederlandsch-Indischen archipel.