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. Alle Informationen zu den Sportstars, Vereinen und Nationalteams wurden nach bestem Wissen und Gewissen zusammengetragen - sollten Sie aber trotzdem einen Fehler bemerkt haben, dann können Sie sich gern per E-Mail (info@trikotshop.net) mit uns in Verbindung setzen und wir werden den Fehler umgehend korrigieren. Dept. 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. lena hatebur. If the senior members of the given member did not play international football, the family will be listed according to nationality (e.g., the Trézéguets). Differently from high-energy photons, neutrinos are effectively not absorbed while traveling through cosmological distances and can escape from dense astrophysical environments. ), Lecture Notes in Computer Science, Vol. Gran Sasso Science Institute, Viale Francesco Crispi 7, I-00167 L'Aquila, Italy, 20 Institut Universitaire de France, F-75005 Paris, France, 36 The IceCube telescope (Achterberg et al. The dashed curves indicate the sensitivities for the IceCube (blue) and ANTARES (red) individual analyses. iv
Publikations-Datenbank der Fraunhofer Wissenschaftler und Institute: Aufsätze, Studien, Forschungsberichte, Konferenzbeiträge, Tagungsbände, Patente und Gebrauchsmuster The decl.-dependent 90% C.L. filmgeschÄftsfÜhrung / accountants. 2,-40\buildrel{\circ}\over{.} Results of the Search at the Location of RXJ 1713.7-3946. ben laser. 0). These qualities make them ideal cosmic messengers as they point back to their production sites. Note. Blue and red curves show the results for the individual IceCube and ANTARES analyses, respectively. 3
Pascal Köpke wurde am 03.09.1995 in Hanau geboren. for the unbroken {E}_{\nu }^{-\gamma } spectrum for two values of the spectral index, γ = 2.0 and γ = 2.5. Results of the Search at the Location of Sagittarius A*. SOMM17/6104/UGR), Generalitat Valenciana: Grisolía (ref. 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. Reviewers, Librarians Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany, 58 Mechanism of Nitrate Reduction byDesulfovibrio desulfuricans Nitrate Reductase—A Theoretical Investigation. 2019) and based on the methods described by Vissani et al. Bioinorganic chemistry of molybdenum and tungsten enzymes: A structural–functional modeling approach. Chem. –bis(dithiolene) complex and its interconversion to a discrete oxo or desoxo DMSOR model. where {\hat{n}}_{{\rm{s}}}, \hat{\gamma }, \hat{\alpha }, and \hat{\delta } are the best-fit values that maximize the likelihood. of Physics, University of Alberta, Edmonton, Alberta, T6G 2E1, Canada, 87 7, D-96049 Bamberg, Germany, 37 You will need to select a minimum of one corridor. A detailed description of these cuts can be found in Adrian-Martinez et al. Mononuclear bis(dithiolene) Mo(
For the ANTARES samples, a spline parameterization of the point-spread function (PSF) is used as the spatial signal PDF. 2, p. 245. Results of the Search in the Galactic Center Region. Dr. Remeis-Sternwarte and ECAP, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. of Physics, TU Dortmund University, D-44221 Dortmund, Germany, 89 PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucía (ref. Indeed, the origin of most of the observed neutrino flux remains unknown. Institute of Space Science, RO-077125 Bucharest, Măgurele, Romania, 16 Find more information about Crossref citation counts. JBIC Journal of Biological Inorganic Chemistry. 2018a, 2018b). Dept. For an {E}_{\nu }^{-2.0} spectrum, a considerable gain in the sensitivity to point-like sources is achieved in all the Southern Sky and in a larger scale in the region close to the Galactic Center. Proceedings, José Neuman de Souza, Petre Dini, Pascal Lorenz (Eds. Dept. Top: upper limits at 90% C.L. By continuing to use this site you agree to our use of cookies. The dashed line depicts the boundary of the search area. Dioxidomolybdenum(VI) complexes chelated with N4-(3-methoxyphenyl)thiosemicarbazone as molybdenum(IV) precursors in oxygen atom transfer process and oxidation of styrene. For each search and source-extension hypothesis, the best-fit values of the parameters and the p-value of the most significant cluster are reported. for the spectral indices γ = 2.0 (left) and γ = 2.5 (right). The mission of the AAS is to enhance and share humanity's scientific understanding of the universe. of Physics, Mercer University, Macon, GA 31207-0001, USA, 98 Baran, Dominika M. 2018. The complementarity of the two detectors is mostly effective for a harder spectral index, as all the samples provide a significant contribution. SNOLAB, 1039 Regional Road 24, Creighton Mine 9, Lively, ON, P3Y 1N2, Canada, 77 Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany, 67 Its membership of about 7,000 individuals also includes physicists, mathematicians, geologists, engineers, and others whose research and educational interests lie within the broad spectrum of subjects comprising contemporary astronomy. ) complexes (chalcogenide E = O, S, Se): Probing MoE and ene-1,2-dithiolate substituent effects on geometric and electronic structure. Figure 7. Enzyme Mimetic Active Intermediates for Nitrate Reduction in Neutral Aqueous Media. Results of the Candidate List Search. Dept. Reported are the source's name, equatorial coordinates, best-fit values of the free parameters, pretrial p-value and 90% C.L. By G. Aad, T. Abajyan, B. Abbott, J. Abdallah, S. Abdel Khalek, A.A. Abdelalim, O. Abdinov, R. Aben, B. Abi, M. Abolins, O.S. Charged current (CC) interactions of muon neutrinos and antineutrinos produce a relativistic muon that can travel large distances through the medium, leaving a track-like signature in the detector. of Physics, University of Wisconsin, River Falls, WI 54022, USA, 96 Values of the best-fit parameters (number of signal events, {\hat{n}}_{{\rm{s}}}, and spectral index, \hat{\gamma }) and p-value for the search at the location of Sagittarius A* for different hypotheses of source extension σs. The 90% C.L. The high density of candidate objects and the presence of molecular clouds around the Galactic Center makes the detection of an extended source more likely than the detection of a point-like source. Spectropotentiometric and Structural Analysis of the Periplasmic Nitrate Reductase from Escherichia coli. This procedure selects only very high-energy events (Eν 100 TeV) with a median angular resolution better than 04 for energies above 1 PeV. Fusion was only possible when the anthracene carried electron-donating alkoxy substituents. In Section 3, the samples employed in the searches are described. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The analysis method and the expected performances are discussed in Section 4, while the performed searches and corresponding results are presented in Section 5. Dipartimento di Fisica dell'Università La Sapienza, P.le Aldo Moro 2, I-00185 Roma, Italy, 19 You need an eReader or compatible software to experience the benefits of the ePub3 file format. 31, D-97074 Würzburg, Germany, 29 In this analysis, two different models are considered for the neutrino emission: that proposed by Kappes et al. Carbon dioxide would be an ideal carbon source for these production systems, but efficient production of long carbon chains from CO2 is difficult to achieve in a single organism. sensitivity and upper limit, both expressed as a ratio with the theoretical source flux. de Física Teórica y del Cosmos & C.A.F.P.E., University of Granada, E-18071 Granada, Spain, 42 The vertical dashed line marks the decl. Chem., Sect. mirja gerle. Five types of searches for point-like and extended sources are performed in this analysis. The largest excess over the background was observed at an angular extension of 00 with a significance of 6%. In this study, the location of 57 astrophysical objects is investigated to look for point-like emission of high-energy neutrinos. of Physics, University of Maryland, College Park, MD 20742, USA, 69 Abschließend geht es um Schwachstellen, die womöglich noch behoben werden sollten und darüber was wir uns von der Saison erhoffen. Base game and two expansions in one big box. This overview shows the selected player's opponents and his performance record against them. The information provided by the number of detected Cerenkov photons and their arrival times is used to infer the neutrino interaction topology, direction and energy. It works to advance physics research, application and education; and engages with policy makers and the public to develop awareness and understanding of physics. Oxo-carboxylato-molybdenum(vi) complexes possessing dithiolene ligands related to the active site of type II DMSOR family molybdoenzymes. Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels, Belgium, 50 Bottom: ratio between the best individual sensitivity and the combined sensitivity as a function of the source decl. 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. Notes. {Project} KuN_Gemüse: Kosten und Nutzen optimierter betrieblicher und überbetrieblicher Nährstoffmanagementstrategien im ökologischen Gemüsebau. Photoinduced electron transfer from the oxo–Mo
All rights reserved. For an {E}_{\nu }^{-2.0} spectrum, the largest improvement is achieved in a region of the sky that is centered approximately at the decl. Figure 4 depicts the pretrial p-values for all the investigated directions for a point-like source hypothesis. IV
List of the most significant clusters found when performing the search in the Galactic Center region for different source-extension hypotheses. Number 2 Figure 1. Synthesis, Structure and a DFT/TDDFT Study of a Diimido-Bridged Asymmetric Dimolybdenum Complex. 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. Results of the Southern Sky Search. This site uses cookies. 2017c): where the contribution of each neutrino flavor f to the track and shower channels is considered. This is a list of association football families. 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{.} produktionsassistenz / production assistant. The corresponding posttrial significance is 18% (0.9σ in the one-sided sigma convention). maja goethel. Dept. Dept. BibTeX of Physics, Stockholm University, SE-10691 Stockholm, Sweden, 52 In the first search, the scanned region is defined by the whole Southern Sky. Overview of the seven data samples of ANTARES and IceCube employed in the analysis. The oxygen-atom transfer reactions of Mo-diselenolene biomimetic complexes: A computational investigation. Das entspricht 40.000 Euro pro Monat. Der FCN hat jede Menge nominelle Mittelstürmer und hat trotzdem noch zwei weitere hinzugefügt. philipp schindler. of Physics, Southern University, Baton Rouge, LA 70813, USA, 84 There’s hustle and bustle at Istanbul’s grand bazaar as merchants and their assistants rush through the narrow alleys in their attempt to be more successful than their competitors. A summary of the data sets in terms of livetime and number of selected events in each sample and for each detector is given in Table 1. INFN—Sezione di Genova, Via Dodecaneso 33, I-16146 Genova, Italy, 5 The first molybdenum dioxo compounds with η
Technical University of Catalonia, Laboratory of Applied Bioacoustics, Rambla Exposició, E-08800 Vilanova i la Geltrú, Barcelona, Spain, 4 of Physics, Marquette University, Milwaukee, WI 53201, USA, 54 A Crystallographic and Mo K-Edge XAS Study of Molybdenum Oxo Bis-, Mono-, and Non-Dithiolene Complexes - First-Sphere Coordination Geometry and Noninnocence of Ligands. 1), with a posttrial significance of 3%, for a source extension of 20. The candidates are sources of high-energy γ-rays and belong to different object classes. Collaboration (Abdalla et al. A combined search for neutrino sources in the Southern Sky using data from the ANTARES and IceCube telescopes was presented. In the case of the shower events, a cut was also applied on the interaction vertex, required to be located within a fiducial volume slightly larger than the instrumented volume. Synthesis, Crystal Structure, UV-vis and EPR Studies of (NH3CH2CH2NH2)2.5 [Mo(V)0.5W(VI)0.5O2 (OC6H4O)2]. 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. Dept. Nikhef, Science Park, Amsterdam, The Netherlands, 15 By setting {n}_{{\rm{s}}}^{\min } slightly above 0, the test statistic Q gets negative values for underfluctuation of the signal. The observation of neutrinos from these sources would be an unambiguous indication of hadronic acceleration. upper limits on the one-flavor neutrino flux normalization for an {E}_{\nu }^{-2.0} and an {E}_{\nu }^{-2.5} spectrum. In this case, atmospheric muons represent the bulk of the detected events before selection, outnumbering the atmospheric neutrinos by a factor from 104 up to 106 depending on the direction. Several filters can be selected. Trotzdem musste der FCN am Ende eine bittere 2:3-Niederlage in Braunschweig hinnehmen. The IceCube selection of throughgoing tracks in the Southern Sky was based on multivariate selection techniques (boosted decision tree; BDT), which made use of parameters connected to the event quality, track topology, energy deposited along the track, and light-arrival time of photons at the DOMs (Aartsen et al. 0) at equatorial coordinates (\hat{\alpha },\hat{\delta })=(274\buildrel{\circ}\over{.} 2014), combined with the throughgoing track-like events—i.e., tracks induced by muons traversing the detector—included in the seven-year IceCube point-source search (Aartsen et al. List of the most significant clusters found when performing the Southern Sky search for different source-extension hypotheses. Moreover, recent searches for neutrino emission from the directions of blazars in the second Fermi-LAT AGN catalog performed by the IceCube Collaboration indicated that blazars contribute less than about 40%–80% (30%) to the total observed neutrino flux, assuming an unbroken power-law spectrum {\rm{\Phi }}({E}_{\nu })\propto {E}_{\nu }^{-\gamma } with \gamma =2.0 (Aartsen et al. 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. of Computer Architecture and Technology/CITIC, University of Granada, E-18071 Granada, Spain, 25 10000, Morocco, 13 of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA, 78 }/{{\rm{\Phi }}}_{0}, and ratio of the upper limit to the assumed source flux, {{\rm{\Phi }}}_{\mathrm{UL}}^{90 \% {\rm{C}}.{\rm{L}}. IFIC—Instituto de Física Corpuscular (CSIC—Universitat de València), c/ Catedrático José Beltrán, 2 E-46980 Paterna, Valencia, Spain; antares.spokesperson@in2p3.fr, 24 Bioinorganic modeling chemistry of carbon monoxide dehydrogenases: description of model complexes, current status and possible future scopes. The most significant source of the list is HESSJ1023-575, a TeV γ-ray source coincident with the young stellar cluster Westerlund 2 (Aharonian 2007), with a pretrial p-value of 0.79%. The charged particles are produced in neutrino interactions with the target medium, inside or near the instrumented volume. montage assistent / assistant editor. Here, we present an untargeted search, to allow for the greatest range of possibilities. 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. A. Aguilar49, M. Ahlers50, M. Ahrens51, C. Alispach52, K. Andeen53, T. Anderson54, I. Ansseau49, G. Anton55, C. Argüelles56, J. Auffenberg57, S. Axani56, P. Backes57, H. Bagherpour47, X. Bai58, A. Balagopal V.59, A. Barbano52, S. W. Barwick60, B. Bastian48, V. Baum61, S. Baur49, R. Bay62, J. J. Beatty63,64, K.-H. Becker65, J. Becker Tjus66, S. BenZvi67, D. Berley68, E. Bernardini102,48, D. Z. Besson103,69, G. Binder62,70, D. Bindig65, E. Blaufuss68, S. Blot48, C. Bohm51, S. Böser61, O. Botner71, J. Böttcher57, E. Bourbeau50, J. Bourbeau72, F. Bradascio48, J. Braun72, S. Bron52, J. Brostean-Kaiser48, A. Burgman71, J. Buscher57, R. S. Busse73, T. Carver52, C. Chen74, E. Cheung68, D. Chirkin72, S. Choi75, K. Clark76, L. Classen73, A. Coleman77, G. H. Collin56, J. M. Conrad56, P. Coppin78, P. Correa78, D. F. Cowen54,79, R. Cross67, P. Dave74, C. De Clercq78, J. J. DeLaunay54, H. Dembinski77, K. Deoskar51, S. De Ridder80, P. Desiati72, K. D. de Vries78, G. de Wasseige78, M. de With81, T. DeYoung82, A. Diaz56, J. C. Díaz-Vélez72, H. Dujmovic59, M. Dunkman54, E. Dvorak58, B. Eberhardt72, T. Ehrhardt61, P. Eller54, R. Engel59, P. A. Evenson77, S. Fahey72, A. R. Fazely83, J. Felde68, K. Filimonov62, C. Finley51, D. Fox79, A. Franckowiak48, E. Friedman68, A. Fritz61, T. K. Gaisser77, J. Gallagher84, E. Ganster57, S. Garrappa48, L. Gerhardt70, K. Ghorbani72, T. Glauch85, T. Glüsenkamp55, A. Goldschmidt70, J. G. Gonzalez77, D. Grant82, T. Grégoire54, Z. Griffith72, S. Griswold67, M. Günder57, M. Gündüz66, C. Haack57, A. Hallgren71, R. Halliday82, L. Halve57, F. Halzen72, K. Hanson72, A. Haungs59, D. Hebecker81, D. Heereman49, P. Heix57, K. Helbing65, R. Hellauer68, F. Henningsen85, S. Hickford65, J. Hignight86, G. C. Hill87, K. D. Hoffman68, R. Hoffmann65, T. Hoinka88, B. Hokanson-Fasig72, K. Hoshina104,72, F. Huang54, M. Huber85, T. Huber48,59, K. Hultqvist51, M. Hünnefeld88, R. Hussain72, S. In75, N. Iovine49, A. Ishihara89, M. Jansson51, G. S. Japaridze90, M. Jeong75, K. Jero72, B. J. P. Jones91, F. Jonske57, R. Joppe57, D. Kang59, W. Kang75, A. Kappes73, D. Kappesser61, T. Karg48, M. Karl85, A. Karle72, U. Katz55, M. Kauer72, J. L. Kelley72, A. Kheirandish72, J. Kim75, T. Kintscher48, J. Kiryluk92, T. Kittler55, S. R. Klein62,70, R. Koirala77, H. Kolanoski81, L. Köpke61, C. Kopper82, S. Kopper93, D. J. Koskinen50, M. Kowalski48,81, K. Krings85, G. Krückl61, N. Kulacz86, N. Kurahashi94, A. Kyriacou87, J. L. Lanfranchi54, M. J. Larson68, F. Lauber65, J. P. Lazar72, K. Leonard72, A. Leszczyńska59, M. Leuermann57, Q. R. Liu72, E. Lohfink61, C. J. Lozano Mariscal73, L. Lu89, F. Lucarelli52, J. Lünemann78, W. Luszczak72, Y. Lyu62,70, W. Y. Ma48, J. Madsen95, G. Maggi78, K. B. M. Mahn82, Y. Makino89, P. Mallik57, K. Mallot72, S. Mancina72, I. C. Mariş49, R. Maruyama96, K. Mase89, R. Maunu68, F. McNally97, K. Meagher72, M. Medici50, A. Medina64, M. Meier88, S. Meighen-Berger85, G. Merino72, T. Meures49, J. Micallef82, D. Mockler49, G. Momenté61, T. Montaruli52, R. W. Moore86, R. Morse72, M. Moulai56, P. Muth57, R. Nagai89, U. Naumann65, G. Neer82, H. Niederhausen85, M. U. Nisa82, S. C. Nowicki82, D. R. Nygren70, A. Obertacke Pollmann65, M. Oehler59, A. Olivas68, A. O'Murchadha49, E. O'Sullivan51, T. Palczewski62,70, H. Pandya77, D. V. Pankova54, N. Park72, P. Peiffer61, C. Pérez de los Heros71, S. Philippen57, D. Pieloth88, S. Pieper65, E. Pinat49, A. Pizzuto72, M. Plum53, A. Porcelli80, P. B. Price62, G. T. Przybylski70, C. Raab49, A. Raissi47, M. Rameez50, L. Rauch48, K. Rawlins98, I. C. Rea85, R. Reimann57, B. Relethford94, M. Renschler59, G. Renzi49, E. Resconi85, W. Rhode88, M. Richman94, S. Robertson70, M. Rongen57, C. Rott75, T. Ruhe88, D. Ryckbosch80, D. Rysewyk82, I. Safa72, S. E. Sanchez Herrera82, A. Sandrock88, J. Sandroos61, M. Santander93, S. Sarkar99, S. Sarkar86, K. Satalecka48, M. Schaufel57, H. Schieler59, P. Schlunder88, T. Schmidt68, A. Schneider72, J. Schneider55, F. G. Schröder59,77, L. Schumacher57, S. Sclafani94, D. Seckel77, S. Seunarine95, S. Shefali57, M. Silva72, R. Snihur72, J. Soedingrekso88, D. Soldin77, M. Song68, G. M. Spiczak95, C. Spiering48, J. Stachurska48, M. Stamatikos64, T. Stanev77, R. Stein48, J. Stettner57, A. Steuer61, T. Stezelberger70, R. G. Stokstad70, A. Stößl89, N. L. Strotjohann48, T. Stürwald57, T. Stuttard50, G. W. Sullivan68, I. Taboada74, F. Tenholt66, S. Ter-Antonyan83, A. Terliuk48, S. Tilav77, K. Tollefson82, L. Tomankova66, C. Tönnis100, S. Toscano49, D. Tosi72, A. Trettin48, M. Tselengidou55, C. F. Tung74, A. Turcati85, R. Turcotte59, C. F. Turley54, B. Ty72, E. Unger71, M. A. Unland Elorrieta73, M. Usner48, J. Vandenbroucke72, W. Van Driessche80, D. van Eijk72, N. van Eijndhoven78, J. van Santen48, S. Verpoest80, M. Vraeghe80, C. Walck51, A. Wallace87, M. Wallraff57, N. Wandkowsky72, T. B. Watson91, C. Weaver86, A. Weindl59, M. J. Weiss54, J. Weldert61, C. Wendt72, J. Werthebach72, B. J. Whelan87, N. Whitehorn101, K. Wiebe61, C. H. Wiebusch57, L. Wille72, D. R. Williams93, L. Wills94, M. Wolf85, J. Wood72, T. R. Wood86, K. Woschnagg62, G. Wrede55, D. L. Xu72, X. W. Xu83, Y. Xu92, J. P. Yanez86, G. Yodh60, S. Yoshida89, T. Yuan72, M. Zöcklein57, and (IceCube Collaboration), Published 2020 April 1 • 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. Sie bestehen meist nur aus einer Strophe und dem Refrain. together with the median sensitivity. Dept. 2017a)). Synthesis and characterization of molybdenum oxo complexes of two tripodal ligands: reactivity studies of a functional model for molybdenum oxotransferases. Upper limits on the neutrino flux from 57 astrophysical candidate sources were presented. SNRs are the prime candidates for the acceleration of Galactic cosmic rays, and hence are potential sources of astrophysical neutrinos. Mediterranean Institute of Oceanography (MIO), Aix-Marseille University, F-13288, Marseille, Cedex 9, France, 39 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. of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA, 70 The ANTARES events were selected by applying cuts on the zenith angle, the angular error estimate, and parameters describing the quality of the reconstruction. … 2016). The American Astronomical Society. These observations represent a major breakthrough in the field, and thus further investigations are strongly motivated. ) complexes with P,P; S,S; O,S and O,O donor ligands: a comparative reactivity study. Revised 2020 February 26 of Physics, Drexel University, 3141 Chestnut Street, Philadelphia, PA 19104, USA, 95 In both cases, searches for emission regions assumed as point-like (σs = 00) or extended (σs = 05, 10, 20) are performed. Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany, 74 List of considered neutrino emission models for the search at the location of RXJ 1713.7-3946 and respective results. Sein geschätztes Gehalt liegt bei 480.000 Euro pro Jahr. 2016), the second search is concentrated around the GC. 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}}. 2018a). selenolato complex to oxygen. Chemical analogues relevant to molybdenum and tungsten enzyme reaction centres toward structural dynamics and reaction diversity. Figure 2. 1995; Halzen & Hooper 2002; Becker 2008; Kelner & Aharonian 2008; Murase 2015). The countries are listed according to the national teams of the senior family member if the other family member played for a different country. ANTARES and IceCube Samples Used in This Analysis. The values of the best-fit {\hat{n}}_{{\rm{s}}} and \hat{\gamma } are 20.3 and 3.0, respectively. Dept. Symphoria: the success of modeling the active site function of oxo-molybdoenzymes. Finally, we perform two dedicated searches at the locations of two promising neutrino source candidates: the supermassive black hole (SMBH) Sagittarius A*, and the shell-type supernova remnant (SNR) RXJ 1713.7-3946. INFN—Sezione di Bari, Via E. Orabona 4, I-70126 Bari, Italy, 23 The fraction of background-like PEs with a p-value smaller than the observed pretrial p-value gives the trial-corrected significance (posttrial p-value) of the observation. Journal of Molecular Catalysis A: Chemical. 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 two telescopes complement each other thanks to their different characteristics, in particular the larger instrumented volume of IceCube and the privileged view of the Southern Sky, with a reduced muon background for neutrino energies below 100 TeV of ANTARES. Runs 2007 - 2008. Dioxomolybdenum(vi) and dioxotungsten(vi) complexes supported by an amido ligand. 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.
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