New German Telecommunications Act, The

In the wake of the debate in Germany on how to weather the storms against the marketplace Germany (Unternehmensstandort Deutschland) the new German Telecommunications Act ( TA ) has been earmarked as a milestone. Its supporters hail the TA to spur competition in Germany\u27s telecommunications market, which they expect to have a turnover of over DM 100 billion (app. US $66 billion) by the year 2000.... This article seeks to summarize the salient features of the TA and to outline the perspectives for potential foreign investors in the German telecommunications market as to the regulatory environment such investor will face. For this purpose, it will briefly describe the process which led to the TA (2.), the applicability of the TA (3.), the Regulator to be established under the TA (4.), the licenses available under the TA (5.), the duties of the licensee (6.) and finally the rights of the licensee (7.). This article is not intended to and cannot provide a comprehensive summary of the TA. Instead it seeks to inform about and draw attention to only those issues which may be of primary interest to a potential investor and which are essential for understanding the regulatory framework for the telecommunications industry in Germany

Explanation as a Social Practice: Toward a Conceptual Framework for the Social Design of AI Systems

none20siThe recent surge of interest in explainability in artificial intelligence (XAI) is propelled by not only technological advancements in machine learning, but also by regulatory initiatives to foster transparency in algorithmic decision making. In this article, we revise the current concept of explainability and identify three limitations: passive explainee, narrow view on the social process, and undifferentiated assessment of understanding. In order to overcome these limitations, we present explanation as a social practice in which explainer and explainee co-construct understanding on the microlevel. We view the co-construction on a microlevel as embedded into a macrolevel, yielding expectations concerning, e.g., social roles or partner models: Typically, the role of the explainer is to provide an explanation and to adapt it to the current level of understanding of the explainee; the explainee, in turn, is expected to provide cues that guide the explainer. Building on explanations being a social practice, we present a conceptual framework that aims to guide future research in XAI. The framework relies on the key concepts of monitoring and scaffolding to capture the development of interaction. We relate our conceptual framework and our new perspective on explaining to transparency and autonomy as objectives considered for XAInoneKatharina J. Rohlfing; Philipp Cimiano; Ingrid Scharlau; Tobias Matzner; Heike M. Buhl; Hendrik Buschmeier; Elena Esposito; Angela Grimminger; Barbara Hammer; Reinhold Häb-Umbach; Ilona Horwath; Eyke Hüllermeier; Friederike Kern; Stefan Kopp; Kirsten Thommes; Axel-Cyrille Ngonga Ngomo; Carsten Schulte; Henning Wachsmuth; Petra Wagner; Britta WredeKatharina J. Rohlfing; Philipp Cimiano; Ingrid Scharlau; Tobias Matzner; Heike M. Buhl; Hendrik Buschmeier; Elena Esposito; Angela Grimminger; Barbara Hammer; Reinhold Häb-Umbach; Ilona Horwath; Eyke Hüllermeier; Friederike Kern; Stefan Kopp; Kirsten Thommes; Axel-Cyrille Ngonga Ngomo; Carsten Schulte; Henning Wachsmuth; Petra Wagner; Britta Wred

Galactic Core-Collapse Supernovae at IceCube: “Fire Drill” Data Challenges and follow-up

The next Galactic core-collapse supernova (CCSN) presents a once-in-a-lifetime opportunity to make astrophysical measurements using neutrinos, gravitational waves, and electromagnetic radiation. CCSNe local to the Milky Way are extremely rare, so it is paramount that detectors are prepared to observe the signal when it arrives. The IceCube Neutrino Observatory, a gigaton water Cherenkov detector below the South Pole, is sensitive to the burst of neutrinos released by a Galactic CCSN at a level >10σ. This burst of neutrinos precedes optical emission by hours to days, enabling neutrinos to serve as an early warning for follow-up observation. IceCube\u27s detection capabilities make it a cornerstone of the global network of neutrino detectors monitoring for Galactic CCSNe, the SuperNova Early Warning System (SNEWS 2.0). In this contribution, we describe IceCube\u27s sensitivity to Galactic CCSNe and strategies for operational readiness, including "fire drill" data challenges. We also discuss coordination with SNEWS 2.0

All-Energy Search for Solar Atmospheric Neutrinos with IceCube

The interaction of cosmic rays with the solar atmosphere generates a secondary flux of mesons that decay into photons and neutrinos – the so-called solar atmospheric flux. Although the gamma-ray component of this flux has been observed in Fermi-LAT and HAWC Observatory data, the neutrino component remains undetected. The energy distribution of those neutrinos follows a soft spectrum that extends from the GeV to the multi-TeV range, making large Cherenkov neutrino telescopes a suitable for probing this flux. In this contribution, we will discuss current progress of a search for the solar neutrino flux by the IceCube Neutrino Observatory using all available data since 2011. Compared to the previous analysis which considered only high-energy muon neutrino tracks, we will additionally consider events produced by all flavors of neutrinos down to GeV-scale energies. These new events should improve our analysis sensitivity since the flux falls quickly with energy. Determining the magnitude of the neutrino flux is essential, since it is an irreducible background to indirect solar dark matter searches

TXS 0506+056 with Updated IceCube Data

Past results from the IceCube Collaboration have suggested that the blazar TXS 0506+056 is a potential source of astrophysical neutrinos. However, in the years since there have been numerous updates to event processing and reconstruction, as well as improvements to the statistical methods used to search for astrophysical neutrino sources. These improvements in combination with additional years of data have resulted in the identification of NGC 1068 as a second neutrino source candidate. This talk will re-examine time-dependent neutrino emission from TXS 0506+056 using the most recent northern-sky data sample that was used in the analysis of NGC 1068. The results of using this updated data sample to obtain a significance and flux fit for the 2014 TXS 0506+056 "untriggered" neutrino flare are reported

Recent neutrino oscillation results with the IceCube experiment

The IceCube South Pole Neutrino Observatory is a Cherenkov detector instrumented in a cubic kilometer of ice at the South Pole. IceCube’s primary scientific goal is the detection of TeV neutrino emissions from astrophysical sources. At the lower center of the IceCube array, there is a subdetector called DeepCore, which has a denser configuration that makes it possible to lower the energy threshold of IceCube and observe GeV-scale neutrinos, opening the window to atmospheric neutrino oscillations studies. Advances in physics sensitivity have recently been achieved by employing Convolutional Neural Networks to reconstruct neutrino interactions in the DeepCore detector. In this contribution, the recent IceCube result from the atmospheric muon neutrino disappearance analysis using the CNN-reconstructed neutrino sample are presented and compared to the existing worldwide measurements