I Lamenti d''Orfeo

Am 4. April, dem Karfreitag des Jahres 1749, an dem am Dresdner Hof keine Opernaufführung stattfinden konnte, kam I Lamenti d’Orfeo, Festa di Camera consagrata alle Glorie Auguste di Ermelinda Talea. Patrocinio, e Decoro d’Arcadia, Poesia del Sig.re Ab:te Giov. Claudio Pasquini d:to Trigenio Migonitidio Pastore Arcade. Musica di Giov. Alberto Ristori 1749 zur Aufführung. Mitwirkende waren Calliope, eine Muse: Rosa Ravona, Orfeo, ihr Sohn: Regina Mingotti. Vermutlich hat Ristori die Hofkapelle vom Cembalo aus geleitet

I Lamenti d’Orfeo: Festa di camera für 2 Soprane, 2 Hörner, 2 Flöten, 2 Oboen, 2 Fagotte, 2 Violinen, Viola und Basso continuo: Partitur

Am 4. April, dem Karfreitag des Jahres 1749, an dem am Dresdner Hof keine Opernaufführung stattfinden konnte, kam I Lamenti d’Orfeo, Festa di Camera consagrata alle Glorie Auguste di Ermelinda Talea. Patrocinio, e Decoro d’Arcadia, Poesia del Sig.re Ab:te Giov. Claudio Pasquini d:to Trigenio Migonitidio Pastore Arcade. Musica di Giov. Alberto Ristori 1749 zur Aufführung. Mitwirkende waren Calliope, eine Muse: Rosa Ravona, Orfeo, ihr Sohn: Regina Mingotti. Vermutlich hat Ristori die Hofkapelle vom Cembalo aus geleitet

Fünf Oboenkonzerte: in Dresdner Überlieferung: Partitur

Der vorliegende Band vereint fünf Oboenkonzerte, die in der Sächsischen Landesbibliothek – Staats- und Universitätsbibliothek Dresden überliefert sind. Sie werden hier, nahezu drei Jahrhunderte nach ihrer Entstehung, der musikalischen Öffentlichkeit in neuen quellenkritischen Ausgaben vorgelegt. Bei den Quellen handelt es sich hauptsächlich um Abschriften Dresdner Hofnotisten. Sie wurden im sogenannten „Schranck No: II.“ in der Katholischen Hofkirche aufbewahrt, die sie als Repertoire der Dresdner Hofkapelle der ersten Hälfte des 18. Jahrhunderts ausweisen. Dieser Band 19 der Editionsreihe Denkmäler der Tonkunst in Dresden ergänzt in sinnvoller Weise den von Hans-Günter Ottenberg herausgegebenen Band 1, Fünf Fagottkonzerte in Dresdner Überlieferung (2011). Er enthält lediglich fünf der zahlreichen Dresdner Konzerte für Oboe solo mit Orchesterbegleitung

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file

Optimasi Portofolio Resiko Menggunakan Model Markowitz MVO Dikaitkan dengan Keterbatasan Manusia dalam Memprediksi Masa Depan dalam Perspektif Al-Qur`an

Risk portfolio on modern finance has become increasingly technical, requiring the use of sophisticated mathematical tools in both research and practice. Since companies cannot insure themselves completely against risk, as human incompetence in predicting the future precisely that written in Al-Quran surah Luqman verse 34, they have to manage it to yield an optimal portfolio. The objective here is to minimize the variance among all portfolios, or alternatively, to maximize expected return among all portfolios that has at least a certain expected return. Furthermore, this study focuses on optimizing risk portfolio so called Markowitz MVO (Mean-Variance Optimization). Some theoretical frameworks for analysis are arithmetic mean, geometric mean, variance, covariance, linear programming, and quadratic programming. Moreover, finding a minimum variance portfolio produces a convex quadratic programming, that is minimizing the objective function ðð¥with constraintsð ð 𥠥 ðandð´ð¥ = ð. The outcome of this research is the solution of optimal risk portofolio in some investments that could be finished smoothly using MATLAB R2007b software together with its graphic analysis

Search for supersymmetry in events with one lepton and multiple jets in proton-proton collisions at root s=13 TeV

Peer reviewe