# ZEU-ICE

Latest additions:
 2019-03-1411:25 [PUBDB-2019-01536] Journal Article et al Measurement of atmospheric tau neutrino appearance with IceCube DeepCore Physical review / D 99(3), 032007 (2019) [10.1103/PhysRevD.99.032007]   We present a measurement of atmospheric tau neutrino appearance from oscillations with three years of data from the DeepCore subarray of the IceCube Neutrino Observatory. This analysis uses atmospheric neutrinos from the full sky with reconstructed energies between 5.6 and 56 GeV to search for a statistical excess of cascadelike neutrino events which are the signature of $ν_τ$ interactions [...] OpenAccess: PDF PDF (PDFA); 2019-03-1410:57 [PUBDB-2019-01534] Journal Article et al The First Tidal Disruption Flare in ZTF: From Photometric Selection to Multi-wavelength Characterization The astrophysical journal 872(2), 198 (2019) [10.3847/1538-4357/aafe0c]   We present Zwicky Transient Facility (ZTF) observations of the tidal disruption flare AT2018zr/PS18kh reported by Holoien et al. and detected during ZTF commissioning. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1416:36 [PUBDB-2019-00459] Poster IceCube Collaboration New measurement of the flavor composition of high-energy neutrino events with contained vertices in IceCube XXVIII International Conference on Neutrino Physics and Astrophysics, NEUTRINO 2018, HeidelbergHeidelberg, Germany, 4 Jun 2018 - 9 Jun 2018   OpenAccess: PDF PDF (PDFA); 2019-01-1416:25 [PUBDB-2019-00458] Report/Contribution to a conference proceedings ARIANNA Collaboration ARIANNA: Current developments and understanding the ice for neutrino detection [arXiv:1811.10660] 8th International Conference on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2018, CataniaCatania, Italy, 12 Jun 2018 - 15 Jun 2018Contributions / Info 6 pp. (2018) [10.3204/PUBDB-2019-00458]   The ARIANNA experiment aims to detect the radio signals of cosmogenic neutrinos. It is running in its pilot phase on the Ross Ice-shelf, and one station has been installed at South Pole. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1416:11 [PUBDB-2019-00457] Preprint/Report et al Supernova PTF12glz: a possible shock breakout driven through an aspherical wind [arXiv:1808.04232 ]   We present visible-light and ultraviolet (UV) observations of the supernova PTF12glz. The SN was discovered and monitored in near-UV and R bands as part of a joint GALEX and Palomar Transient Factory campaign. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1416:05 [PUBDB-2019-00456] Preprint/Report Franckowiak, A. Eddington Bias for Cosmic Neutrino Sources [arXiv:1809.06865; DESY-18-164]   We describe a consequence of the Eddington bias which occurs when a single astrophysical neutrino event is used to infer the neutrino flux of the source. A trial factor is introduced by the potentially large number of similar sources that remain undetected and if not accounting for this factor the luminosity of the observed source can be overestimated by several orders of magnitude. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1415:46 [PUBDB-2019-00453] Preprint/Report et al High-Energy Emission from Interacting Supernovae: New Constraints on Cosmic-Ray Acceleration in Dense Circumstellar Environments [arXiv:1807.01460]   Supernovae (SNe) with strong interactions with circumstellar material (CSM) are promising candidate sources of high-energy neutrinos and gamma rays, and have been suggested as an important contributor to Galactic cosmic rays beyond 1 PeV. Taking into account the shock dissipation by a fast velocity component of SN ejecta, we present comprehensive calculations of the non-thermal emission from SNe powered by shock interactions with a dense wind or CSM. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1415:34 [PUBDB-2019-00451] Preprint/Report et al Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate [arXiv:1806.03849]   As part of an on-going effort to identify, understand and correct for astrophysics biases in the standardization of Type Ia supernovae (SN Ia) for cosmology, we have statistically classified a large sample of nearby SNe Ia into those located in predominantly younger or older environments. This classification is based on the specific star formation rate measured within a projected distance of 1 kpc from each SN location, (LsSFR). [...] OpenAccess: PDF PDF (PDFA); 2019-01-1415:20 [PUBDB-2019-00448] Journal Article et al SNEMO: Improved Empirical Models for Type Ia Supernovae The astrophysical journal 869(2), 167 (2018) [10.3847/1538-4357/aaec7e]   SN Ia cosmology depends on the ability to fit and standardize observations of supernova magnitudes with an empirical model. We present here a series of new models of SN Ia spectral time series that capture a greater amount of supernova diversity than is possible with the models that are currently customary. [...] OpenAccess: PDF PDF (PDFA); 2019-01-1414:42 [PUBDB-2019-00441] Preprint/Report et al Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments [arXiv:1803.05390]   The current and upcoming generation of Very Large Volume Neutrino Telescopes - collecting unprecedented quantities of neutrino events - can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. [...] OpenAccess: PDF PDF (PDFA);