# ZEU-ICE

 2019-07-2914:53 [PUBDB-2019-02863] Report/Journal Article et al Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1 [arXiv:1901.11080] Astronomy and astrophysics 626, A117 (2019) [10.1051/0004-6361/201935171]   In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. To increase the sensitivity of detecting counterparts of transient or variable sources by telescopes with a limited field of view, IceCube began releasing alerts for single high-energy (E$_ν$ >  60 TeV) neutrino detections with sky localisation regions of order 1° radius in 2016. [...] OpenAccess: PDF PDF (PDFA); Restricted: PDF PDF (PDFA); 2019-07-1515:53 [PUBDB-2019-02721] Journal Article et al The Zwicky Transient Facility: Science Objectives Publications of the Astronomical Society of the Pacific 131(1001), 078001 (2019) [10.1088/1538-3873/ab006c]   The Zwicky Transient Facility (ZTF), a public–private enterprise, is a new time-domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg2 field of view and an 8 second readout time. It is well positioned in the development of time-domain astronomy, offering operations at 10% of the scale and style of the Large Synoptic Survey Telescope (LSST) with a single 1-m class survey telescope [...] OpenAccess: PDF PDF (PDFA); 2019-05-0715:45 [PUBDB-2019-02172] Journal Article et al A GeV–TeV Measurement of the Extragalactic Background Light The astrophysical journal / 2 874(1), L7 (2019) [10.3847/2041-8213/ab0c10]   The extragalactic background light (EBL) can be probed via the absorption imprint it leaves in the spectra of gamma-ray sources ($\gamma \gamma \to {e}^{-}{e}^{+}$). We recently developed a dedicated technique to reconstruct the EBL, and its evolution with redshift, from γ-ray optical depth data using a large sample of blazars detected by the Fermi Large Area Telescope. [...] Published on 2019-03-22. Available in OpenAccess from 2020-03-22.: PDF PDF (PDFA); Restricted: PDF PDF (PDFA); 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 / 1 872(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);