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upper limits on the one-flavor neutrino flux normalization of this search are shown in Figure 5 for different source extensions. Export citation and abstract National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, Wisconsin Alumni Research Foundation, Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison, Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy–National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland, Institute for Cyber-Enabled Research at Michigan State University, and Astroparticle physics computational facility at Marquette University; Belgium—Funds for Scientific Research (FRS-FNRS and FWO), FWO Odysseus and Big Science programmes, and Belgian Federal Science Policy Office (Belspo); Germany—Bundesministerium für Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Initiative and Networking Fund of the Helmholtz Association, Deutsches Elektronen Synchrotron (DESY), and High Performance Computing Cluster of the RWTH Aachen; Sweden—Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation; Australia—Australian Research Council; Canada—Natural Sciences and Engineering Research Council of Canada, Calcul Québec, Compute Ontario, Canada Foundation for Innovation, WestGrid, and Compute Canada; Denmark—Villum Fonden, Danish National Research Foundation (DNRF), Carlsberg Foundation; New Zealand—Marsden Fund; Japan—Japan Society for Promotion of Science (JSPS) and Institute for Global Prominent Research (IGPR) of Chiba University; Korea—National Research Foundation of Korea (NRF); Switzerland—Swiss National Science Foundation (SNSF); United Kingdom—Department of Physics, University of Oxford. scalar relativistic basis sets for the elements Rb–Xe. This makes it possible to properly calculate the median of the background Q-distribution. Only Southern Sky events (numbers of events reported in the last column) have been selected for the present analysis. of Physics, University of Alberta, Edmonton, Alberta, T6G 2E1, Canada, 87 Reported are the source extension {\sigma }_{{\rm{s}}}, the best-fit parameters (number of signal events, {\hat{n}}_{{\rm{s}}}, spectral index, \hat{\gamma }, decl., \hat{\delta }, R.A., \hat{\alpha }), and the pretrial and posttrial p-values. Dipartimento di Fisica dell'Università, Via Dodecaneso 33, I-16146 Genova, Italy, 27 Five types of searches for point-like and extended sources are performed in this analysis. Table 5. Formation of Mono Oxo Molybdenum(IV) PNP Pincer Complexes: Interplay between Water and Molecular Oxygen. University Mohammed V in Rabat, Faculty of Sciences, 4 av. Synthesis, characterization, and spectroscopy of model molybdopterin complexes. Dr. Remeis-Sternwarte and ECAP, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France, 10 Pascal Köpke wurde am 03.09.1995 in Hanau geboren. Table 1. Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany, 67 Revised 2020 February 26 SiCN: a route to a cyanide-bridged multimer to a monomer. A. Martínez-Mora6, R. Mele45,46, K. Melis14,16, P. Migliozzi45, M. Moser5, A. Moussa13, R. Muller14, L. Nauta14, S. Navas41, E. Nezri9, C. Nielsen8, A. Nuñez-Castiñeyra7,9, B. O'Fearraigh14, M. Organokov1, G. E. Păvălaş15, C. Pellegrino21,29, M. Perrin-Terrin7, P. Piattelli11, C. Poirè6, V. Popa15, T. Pradier1, L. Quinn7, N. Randazzo40, G. Riccobene11, A. Sánchez-Losa22, A. Salah-Eddine20, D. F. E. Samtleben14,34, M. Sanguineti4,26, P. Sapienza11, F. Schüssler42, M. Spurio21,29, Th. A total of 5160 digital optical modules (DOMs), each consisting of a pressure-resistant sphere that houses electronics, calibration LEDs, and a 10'' PMT facing downward, are attached to 86 vertical strings, with a mean distance between strings of ~125 m. The construction of the IceCube detector began in 2005 and was finished six years later. The most significant clustering with respect to the expected background is searched for at any position in a predefined region of the sky. }/{{\rm{\Phi }}}_{0}. Kim Scheele wurde von Alexandra Finder gespielt. A density functional theory study. 2014; Fang & Murase 2018). Find more information about Crossref citation counts. Here, we present an untargeted search, to allow for the greatest range of possibilities. … This professional brewing journal in English is aimed at providing a forum to exchange experience and knowledge in all areas of brewing and malting, not just by publishing technical articles by research institutes, but also through reports from suppliers and above all by contributions from actual factory situations. 2,-40\buildrel{\circ}\over{.} Point-source 5σ discovery fluxes for an unbroken {E}_{\nu }^{-\gamma } neutrino spectrum, with γ = 2.0 (left) and γ = 2.5 (right). Dipartimento di Fisica dell'Università Federico II di Napoli, Via Cintia I-80126, Napoli, Italy, 47 Institute of Space Science, RO-077125 Bucharest, Măgurele, Romania, 16 Die Lieder und Texte sind alle von Kurt selbst geschrieben auf dieser Seite werden alle Lieder von Dark Circle mit Liedtexten zusammengestellt - in Aufbau- I'm Insane . A three-dimensional array of photomultiplier tubes (PMTs) inside a transparent medium—water or ice, respectively—collects the Cerenkov photons induced by the passage of relativistic charged particles. Laboratoire de Physique Corpusculaire, Clermont Université, Université Blaise Pascal, CNRS/IN2P3, BP 10448, F-63000 Clermont-Ferrand, France, 31 of Physics, University of Texas at Arlington, 502 Yates St., Science Hall Rm 108, Box 19059, Arlington, TX 76019, USA, 92 Molybdenum and Tungsten Oxidoreductase Models. Characterization of a reduced molybdenum-oxo compound derived from an oxo-transfer process under stoichiometric conditions. Published 2020 April 1. 0) at equatorial coordinates (\hat{\alpha },\hat{\delta })=(274\buildrel{\circ}\over{.} Table 2. Rep. Prog. Dept. For each ANTARES event i, \mathrm{PSF}({\rm{\Delta }}{{\rm{\Psi }}}_{i}) provides the PDF of reconstructing the event at an angular distance ΔΨi from the source. Abschließend geht es um Schwachstellen, die womöglich noch behoben werden sollten und darüber was wir uns von der Saison erhoffen. Bis(dithiolene) Molybdenum Complex that Promotes Combined Coupled Electron–Proton Transfer and Oxygen Atom Transfer Reactions: A Water-Active Model of the Arsenite Oxidase Molybdenum Center. Two main event topologies can be identified in the ANTARES and IceCube telescopes: tracks and showers. Dept. Finally, the location of the SNR RXJ 1713.7-3946 was investigated assuming two proposed neutrino emission models and a source extension of 06. INFN—Sezione di Roma, P.le Aldo Moro 2, I-00185 Roma, Italy, 18 Neutrinos are expected to be produced through the decay of charged mesons, a result of hadronic interactions of accelerated protons with matter or radiation in the surroundings of the acceleration sites. Géoazur, UCA, CNRS, IRD, Observatoire de la Côte d'Azur, Sophia Antipolis, France, 26 Chemistry of oxidomolybdenum(IV) and -(VI) complexes with ONS donor ligands: Synthesis, computational evaluation and oxo-transfer reactions. Mechanistic Insight into the Reactivity of Oxotransferases by Novel Asymmetric Dioxomolybdenum(VI) Model Complexes. ), Lecture Notes in Computer Science, Vol. © 2020. Dept. upper limits on the one-flavor neutrino flux normalization of the Galactic Center region search, assuming an {E}_{\nu }^{-2.0} spectrum for different source extensions σs. Institut für Physik, Humboldt-Universität zu Berlin, D-12489 Berlin, Germany, 82 A quantum chemical study. The values of the best-fit {\hat{n}}_{{\rm{s}}} and \hat{\gamma } are 20.3 and 3.0, respectively. A. Diggle A. Irvine A. Moore A. Kubert A. Lanning A. Johnston A. Schlagman A. Syaf A. Gaines A. Katsnelson A. Maleev A. Simons A. D. Coulter A. Davi A. Cooper A. Vitti A. Conley A. 1, D-91058 Erlangen, Germany, 6 The likelihood describes the data in terms of signal and background probability density functions (PDFs) and is defined as: where ns and γ are respectively the unknown total number of signal events and signal spectral index, α and δ are the unknown equatorial coordinates of the source, and Sji and Bji are the values of the signal and background PDFs for the event i in the sample j. Nj is the total number of data events in sample j, while {n}_{{\rm{s}}}^{j} is the unknown number of signal events in sample j, related to ns through the relative contribution of the given sample, {n}_{{\rm{s}}}^{j}={n}_{{\rm{s}}}\cdot \ {C}^{j}(\delta ,{\rm{\Phi }}). Click here to close this overlay, or press the "Escape" key on your keyboard. Table 6. As no significant evidence of cosmic neutrinos was observed, upper limits were derived. Please note, The Astrophysical Journal Letters (ApJL) and Research Notes of the AAS (RNAAS) Cross sections, in both the electron and muon decay modes of the W Sagittarius A* was tested as a point-like source and as an extended source. The position of the most significant cluster is also indicated. of Physics and Astronomy, UCLA, Los Angeles, CA 90095, USA. This work supersedes a previous combined analysis using a smaller data sample of five and three years of ANTARES and IceCube data, respectively (Adrian-Martinez et al. Photoinduced electron transfer from the oxo–Mo The dashed line depicts the boundary of the search area. Das entspricht 40.000 Euro pro Monat. The longer lever arm of the track topology allows for a better reconstruction of the particle direction and therefore for a better median angular resolution, while a better reconstruction of the particle energy is achieved for showers, as the topology allows for a calorimetric measurement. 103 Also at National Research Nuclear University, Moscow Engineering Physics Institute (MEPhI), Moscow 115409, Russia. Dots (...) in the fitted number of source events, spectral index, and p-value indicate cases of null observations ({\hat{n}}_{{\rm{s}}}=0.001). Request new password . {Project} KuN_Gemüse: Kosten und Nutzen optimierter betrieblicher und überbetrieblicher Nährstoffmanagementstrategien im ökologischen Gemüsebau. Dept. During the likelihood maximization, the number of signal events ns and the signal spectral index γ are free parameters. The fraction of background-like pseudoexperiments with a value of Q larger than the observed Q-value gives the significance (p-value) of the observation. -enedithiolate complexes – a look at both ends of the catalytic transformation. of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand, 49 Dept. Proceedings, José Neuman de Souza, Petre Dini, Pascal Lorenz (Eds. © 2020. Searches for pair-produced scalar leptoquarks are performed using 20 fb of proton–proton collision data provided by the LHC and recorded by the ATLAS detector at TeV. For the softer spectrum {E}_{\nu }^{-2.5}, the contribution of high-energy neutrinos is lower, and therefore the relative contribution of the ANTARES sample increases. By continuing to use this site you agree to our use of cookies. of Physics, University of Wuppertal, D-42119 Wuppertal, Germany, 66 Sport/Fußball: NEU - Roy Beerens, Änis Ben-Hatira, Javairo Dilrosun, Ondrej Duda, Jens Hegeler, Pascal Köpke, Peter Pekarik, Maximilian Philipp, Valentin Stocker, Jordan Torunarigha, Johannes Van den Bergh, Mitchell Weiser ERGÄNZUNG - Alexander Baumjohann, Julian Schieber UPDATE 2019-06-30 SW-Cast: ERGÄNZUNG - Katee Sackhoff The first molybdenum dioxo compounds with η Here, Tj is the livetime of the sample j reported in Table 1, Ω is the solid angle, Eν is the neutrino energy, {A}_{\mathrm{eff}}^{j,{\nu }_{f}+{\bar{\nu }}_{f}} is the detector effective area, and {{\rm{\Phi }}}_{{\nu }_{f}+{\bar{\nu }}_{f}} is the expected flux from the source. 2014) and seven years (Aartsen et al. Köpke und seine Kim - FCN-Stürmer liebt Promi-Tochter. In the first two searches, a scan of the full Southern Sky and of a restricted region around the Galactic Center (GC) are carried out. A median angular resolution better than 04 is achieved for the selected tracks for energies above 100 TeV, and ~3° for the selected showers for energies between 1 TeV and 0.5 PeV. 1,-40\buildrel{\circ}\over{.} However, if the hypothesis used to guide such searches is incorrect, sensitivity to neutrino sources will be reduced. Description. Figure 4 depicts the pretrial p-values for all the investigated directions for a point-like source hypothesis. Institut Universitaire de France, F-75005 Paris, France, 36 Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA, 71 An Asymmetrically Substituted Aliphatic Bis-Dithiolene Mono-Oxido Molybdenum(IV) Complex With Ester and Alcohol Functions as Structural and Functional Active Site Model of Molybdoenzymes. The detector comprises a three-dimensional array of 885 optical modules (OMs), each one housing a 10'' PMT, facing 45° downward in order to optimize the detection of Cerenkov photons from upgoing charged particles. The shell-type SNR RXJ 1713.7-3946, at equatorial coordinates (α, δ) = (25825, −3975), is the brightest object of this kind in the TeV γ-ray sky and represents a particularly interesting target to the search for cosmic neutrinos (Vissani 2006; Kappes et al. iv To find the largest deviation from background expectation, the scanned region is divided into a grid with boxes of 1° × 1° in R.A. and decl. 2 Sie bestehen meist nur aus einer Strophe und dem Refrain. A. Albert1,2, M. André3, M. Anghinolfi4, G. Anton5, M. Ardid6, J.-J. Dept. B. Baret https://orcid.org/0000-0001-6064-3858, G. Illuminati https://orcid.org/0000-0002-4138-8027, O. Kalekin https://orcid.org/0000-0001-6206-1288, U. Katz https://orcid.org/0000-0002-7063-4418, R. Le Breton https://orcid.org/0000-0001-8522-4983, E. Leonora https://orcid.org/0000-0002-0536-3551, J. Wilms https://orcid.org/0000-0003-2065-5410, A. Franckowiak https://orcid.org/0000-0002-5605-2219, J. Gallagher https://orcid.org/0000-0001-8608-0408, S. Garrappa https://orcid.org/0000-0003-2403-4582, M. Santander https://orcid.org/0000-0001-7297-8217, N. L. Strotjohann https://orcid.org/0000-0002-4667-6730, Received 2019 December 25 iv Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen, Germany, 56 2016; Kopper 2017, and Aartsen et al. Dept. Juli 1998zu sehen. Juni 1998 bis Folge 1512 am 08. It works to advance physics research, application and education; and engages with policy makers and the public to develop awareness and understanding of physics. Its publishing company, IOP Publishing, is a world leader in professional scientific communications. Polymer-Supported Dioxido-MoVI Complexes as Truly Functional Molybdenum Oxotransferase Model Systems. A new series of molybdenum-(iv), -(v), and -(vi) dithiolate compounds as active site models of molybdoenzymes: preparation, crystal structures, spectroscopic/electrochemical properties and reactivity in oxygen atom transfer. Dioxomolybdenum(vi) and dioxotungsten(vi) complexes supported by an amido ligand. For each ANTARES sample j ∈ [1, 2] given in Table 1, the expected mean number of signal events, Nj, is obtained as (Aartsen et al. The most significant result of the search restricted to the Galactic Center region is observed for an extended source hypothesis ({\sigma }_{{\rm{s}}}=2\buildrel{\circ}\over{.} 2018a) (\gamma =2.5 (Aartsen et al. Notes. The neutrino flux of TXS 0506+056 can only account for less than 1% of the total observed astrophysical flux (Aartsen et al. Université de Haute Alsace, F-68200 Mulhouse, France, 3 Equipartition at Earth of the three neutrino flavors is assumed. do not currently use the corridors. LPHEA, Faculty of Science—Semlali, Cadi Ayyad University, P.O.B. When limiting the search to the GC region, the most significant cluster was found at equatorial coordinates (\hat{\alpha },\hat{\delta })=(274\buildrel{\circ}\over{.} To this purpose, the pretrial p-value is compared to the distribution of the smallest p-values found when performing the same analysis on many background-only PEs. 0. The observation of neutrinos from these sources would be an unambiguous indication of hadronic acceleration. 2014; Kopper et al. Common backgrounds in both detectors are atmospheric muons and neutrinos originating from cosmic-ray interactions in Earth's atmosphere. Volume 892, Moreover, exploiting multimessenger observations helps to refine the selection of the target neutrino source candidates, allowing to reduce the number of tested locations and therefore the trial factor (Franckowiak 2017). III. Indeed, the origin of most of the observed neutrino flux remains unknown. Collaboration (Abdalla et al. 2017c) are used in this analysis. INFN—Sezione di Bologna, Viale Berti-Pichat 6/2, I-40127 Bologna, Italy, 22 of Physics, University of Adelaide, Adelaide, 5005, Australia, 88 The red contour indicates the location of the most significant cluster. Gran Sasso Science Institute, Viale Francesco Crispi 7, I-00167 L'Aquila, Italy, 20 of Physics, Yale University, New Haven, CT 06520, USA, 97 Indeed, if the lower boundary, {n}_{{\rm{s}}}^{\min }, is set to {n}_{{\rm{s}}}^{\min }=0, a test statistic Q = 0 is obtained in more than 50% of the PEs, leading to an overestimation of the median 90% upper limit. Sein aktueller Verein ist 1.FC Nürnberg, er spielt dort im Sturm - Mittelstürmer. Sport/Fußball: NEU - Roy Beerens, Änis Ben-Hatira, Javairo Dilrosun, Ondrej Duda, Jens Hegeler, Pascal Köpke, Peter Pekarik, Maximilian Philipp, Valentin Stocker, Jordan Torunarigha, Johannes Van den Bergh, Mitchell Weiser ERGÄNZUNG - Alexander Baumjohann, Julian Schieber UPDATE 2019-06-30 SW-Cast: ERGÄNZUNG - Katee Sackhoff Accepted 2020 February 26 de Física Teórica y del Cosmos & C.A.F.P.E., University of Granada, E-18071 Granada, Spain, 42 (in units of {10}^{-6}\ {\mathrm{GeV}}^{-1}\,{\mathrm{cm}}^{-2}\,{{\rm{s}}}^{-1}). ) complexes with P,P; S,S; O,S and O,O donor ligands: a comparative reactivity study. Note. Di Palma17,18, A. Domi4,26, C. Donzaud8,27, D. Dornic7, D. Drouhin1,2, T. Eberl5, I. El Bojaddaini13, N. El Khayati12, D. Elsässer28, A. Enzenhöfer5,7, A. Ettahiri12, F. Fassi12, P. Fermani17,18, G. Ferrara11, F. Filippini21,29, L. Fusco8,29, P. Gay8,30, H. Glotin31, R. Gozzini23, R. Gracia Ruiz1, K. Graf5, C. Guidi4,26, S. Hallmann5, H. van Haren32, A. J. Heijboer14, Y. Hello25, J. J. Hernández-Rey23, J. Hößl5, J. Hofestädt5, G. Illuminati23, C. W. James33, M. de Jong14,34, P. de Jong14, M. Jongen14, M. Kadler28, O. Kalekin5, U. Katz5, N. R. Khan-Chowdhury23, A. Kouchner8,35, M. Kreter28, I. Kreykenbohm36, V. Kulikovskiy4,37, R. Lahmann5, R. Le Breton8, D. Lefèvre38,39, E. Leonora40, G. Levi21,29, M. Lincetto7, D. Lopez-Coto41, S. Loucatos8,42, G. Maggi7, J. Manczak23, M. Marcelin9, A. Margiotta21,29, A. Marinelli43,44, J. Here, only the number of signal events and the spectral index are left as free parameters in the likelihood maximization, as the direction of the selected sources is known. Indeed, using the information of the neutrino arrival times is expected to significantly increase the discovery potential, as it improves the signal-to-background discrimination (Aartsen et al. The advantageous field of view of ANTARES and the large size of IceCube are exploited to improve the sensitivity in the Southern Sky by a factor of ~2 compared to both individual analyses. In the first search, the scanned region is defined by the whole Southern Sky. The countries are listed according to the national teams of the senior family member if the other family member played for a different country. Upper limits on the neutrino flux from 57 astrophysical candidate sources were presented. Moreover, the position of the source is either kept fixed or fitted within specific limits, depending on the type of search (see Section 5). upper limits on the one-flavor neutrino flux normalization as a function of the source extension are shown in Figure 7, together with the median sensitivity and the discovery flux. The data set consists of all the track-like and shower-like events pointing in the direction of the Southern Sky included in the nine-year ANTARES point-source analysis, combined with the throughgoing track-like events used in the seven-year IceCube point-source search. Juni 1996 sowie von Folge 1497 am 19. In this Letter a search is performed at the ATLAS experiment for slow-moving charged Dipartimento di Fisica e Astronomia dell'Università, Viale Berti Pichat 6/2, I-40127 Bologna, Italy, 30 31, D-97074 Würzburg, Germany. Results of the Southern Sky Search. The spectral index γ can range between 1.0 and 4.0, as these are the limits of reasonable spectral assumptions for astrophysical particle acceleration mechanisms. -pyrazolate ligands: crystal structure and oxo transfer properties. 2016). For a soft spectral index, the contribution of high-energy neutrinos is suppressed and ANTARES dominates in most of the Southern Sky. The analyzed candidates correspond to all the sources in the Southern Sky considered in the candidate list search performed by the ANTARES (Adrian-Martinez et al. The green line indicates the sensitivity of the combined analysis. Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany, 74 2018). Dots (...) in the fitted number of source events, spectral index and pretrial p-value indicate sources with null observations ({\hat{n}}_{{\rm{s}}}=0.001). Several filters can be selected. The most significant source candidate is HESSJ1023-575, with a posttrial significance of 42%. The IceCube data were taken from 2008 to 2015, with the detector operating either in partial (samples IC40, IC59, IC79) or in full (samples IC86-2011, IC86-2012-2015) configuration. for the unbroken {E}_{\nu }^{-\gamma } spectrum for two values of the spectral index, γ = 2.0 and γ = 2.5. A total of 6.4 signal events and a spectral index of 3.5 are fitted for the cluster at the position of HESSJ1023-575. Zeitschrift für anorganische und allgemeine Chemie. The standard time-integrated method fits 1.03 signal events, which corresponds to a p-value of 3.4% (not considering trial corrections). Synthesis and structure of [L][MoIVO(mnt)2] {L=[(C2H5)4N]+, [C5H5NH]+, [(C2H5)3NH]+, [lysinium]2+ and (mnt2−=1,2-dicyanoethylenedithiolate)} in relevance to molybdenum cofactor of diverse class of molybdoenzymes. iv the Altmetric Attention Score and how the score is calculated. Figure 5. http://pubs.acs.org/page/copyright/permissions.html, https://doi.org/10.1021/acs.inorgchem.7b02956, https://doi.org/10.1021/acs.inorgchem.5b02395, https://doi.org/10.1016/j.poly.2019.08.006, https://doi.org/10.1016/j.ccr.2019.05.005, https://doi.org/10.1016/j.ica.2018.10.001, https://doi.org/10.1016/j.comptc.2018.07.003, https://doi.org/10.1016/j.poly.2017.12.023, https://doi.org/10.1002/9783527664160.ch13, https://doi.org/10.1002/9780470682531.pat0604, https://doi.org/10.1007/s00775-012-0961-5, https://doi.org/10.1002/9781119951438.eibc0136, https://doi.org/10.1016/j.ccr.2010.10.017, https://doi.org/10.1016/j.ccr.2010.11.027, https://doi.org/10.1016/j.ccr.2011.02.010, https://doi.org/10.1016/j.ccr.2010.01.017, https://doi.org/10.1007/s00775-009-0548-y, https://doi.org/10.1016/j.ica.2008.01.026, https://doi.org/10.1016/j.jinorgbio.2007.07.012, https://doi.org/10.1016/j.molcata.2006.07.025, https://doi.org/10.1080/00268970500179461, https://doi.org/10.1016/j.jinorgbio.2004.07.002, https://doi.org/10.1016/S0022-2860(03)00336-3, https://doi.org/10.1016/B0-08-043748-6/03033-4, https://doi.org/10.1016/B0-08-043748-6/08168-8, https://doi.org/10.1016/S0968-0004(02)02107-2, https://doi.org/10.1016/S1387-7003(02)00442-2. 2011) and IceCube (Achterberg et al. of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802, USA, 80 Results of the Search at the Location of RXJ 1713.7-3946. This overview shows the selected player's opponents and his performance record against them. Dept. Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 8 0. Motivated by the high concentration of candidate sources and gas around the GC and the recent observation of a possible Pevatron presence close to the GC by the HESS Collaboration (Abramowski et al. APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 9 Spectropotentiometric and Structural Analysis of the Periplasmic Nitrate Reductase from Escherichia coli. The decl.-dependent 90% C.L. The last four columns show the results in terms of best-fit number of signal events, {\hat{n}}_{{\rm{s}}}, p-value, ratio of the sensitivity to the assumed source flux, {{\rm{\Phi }}}_{\mathrm{sens}}^{90 \% {\rm{C}}.{\rm{L}}. 8), for a point-like source hypothesis. U., Universität Bonn . Stolarczyk42, B. Strandberg14, M. Taiuti4,26, Y. Tayalati12, T. Thakore23, S. J. Tingay33, A. Trovato11, B. Vallage8,42, V. Van Elewyck8,35, F. Versari8,21,29, S. Viola11, D. Vivolo45,46, J. Wilms36, D. Zaborov7, A. Zegarelli17,18, J. D. Zornoza23, J. Zúñiga23, (ANTARES Collaboration), M. G. Aartsen47, M. Ackermann48, J. Adams47, J.