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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. ), Lecture Notes in Computer Science, Vol. Dept. 104 Also at Earthquake Research Institute, University of Tokyo, Bunkyo, Tokyo 113-0032, Japan. The corresponding posttrial significance is 18% (0.9σ in the one-sided sigma convention). 7,-11\buildrel{\circ}\over{.} 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}}. For the ANTARES samples, a spline parameterization of the point-spread function (PSF) is used as the spatial signal PDF. 28 Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer Str. Université du Sud Toulon-Var, CNRS-INSU/IRD UM 110, F-83957, La Garde Cedex, France, 40 The Astrophysical Journal, 2017c): where the contribution of each neutrino flavor f to the track and shower channels is considered. 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. Events from the Southern Sky correspond to downgoing events for IceCube. The charged particles are produced in neutrino interactions with the target medium, inside or near the instrumented volume. The trial-corrected significance of the cluster is 42%, corresponding to 0.2σ in the one-sided convention. of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA, 78 Comparative molecular chemistry of molybdenum and tungsten and its relation to hydroxylase and oxotransferase enzymes. 47, Issue. 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. Which functional groups of the molybdopterin ligand should be considered when modeling the active sites of the molybdenum and tungsten cofactors? 0). Oxo-carboxylato-molybdenum(vi) complexes possessing dithiolene ligands related to the active site of type II DMSOR family molybdoenzymes. of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA, 68 Mechanistic Investigation of the Oxygen-Atom-Transfer Reactivity of Dioxo-molybdenum(VI) Complexes. of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, USA, 93 For a soft spectral index, the contribution of high-energy neutrinos is suppressed and ANTARES dominates in most of the Southern Sky. (in units of {10}^{-6}\ {\mathrm{GeV}}^{-1}\,{\mathrm{cm}}^{-2}\,{{\rm{s}}}^{-1}). Das entspricht 40.000 Euro pro Monat. scalar relativistic basis sets for the elements Rb–Xe. (A A S ) journals as soon as they are published. Dithiolene complexes and the nature of molybdopterin. The list of the astronomical candidates is shown in Table 4, together with their equatorial coordinates, fitted number of signal events, fitted spectral index, pretrial p-value, and 90% C.L. APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs de Paris, Sorbonne Paris Cité, France, 9 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. 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. Mechanistic Insight into the Reactivity of Oxotransferases by Novel Asymmetric Dioxomolybdenum(VI) Model Complexes. Sein aktueller Verein ist 1.FC Nürnberg, er spielt dort im Sturm - Mittelstürmer. Dept. The green line indicates the sensitivity of the combined analysis. Dept. These observations represent a major breakthrough in the field, and thus further investigations are strongly motivated. The ANTARES and IceCube neutrino telescopes rely on the same principle for detecting cosmic neutrinos. 2019) and based on the methods described by Vissani et al. A computational investigation into the catalytic activity of a diselenolene sulfite oxidase biomimetic complex. No significant evidence for cosmic neutrino sources is found, and upper limits on the flux from the various searches are presented. 2017b) neutrino telescopes collected during nine (Adrian-Martinez et al. The ANTARES data were collected between early 2007 and the end of 2015. 2, p. 245. Upper limits on the neutrino flux from 57 astrophysical candidate sources were presented. 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. LPHEA, Faculty of Science—Semlali, Cadi Ayyad University, P.O.B. The posttrial significance is 3% (1.9σ in the one-sided sigma convention). 2017b) is a cubic-kilometer-sized detector located at the South Pole, between 1450 and 2450 m below the surface of the Antarctic ice. 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. 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. Symphoria: the success of modeling the active site function of oxo-molybdoenzymes. ) dithiolate complex containing bulky hydrophobic groups. Figure 7. of Physics and Astronomy, Uppsala University, Box 516, SE-75120 Uppsala, Sweden, 72 © 2020. Characterization of a reduced molybdenum-oxo compound derived from an oxo-transfer process under stoichiometric conditions. Dept. Note. Neither significant point-like nor extended neutrino emission over the background expectation was found. This overview shows the selected player's opponents and his performance record against them. Dept. Table 2. In the first search, the scanned region is defined by the whole Southern Sky. of Physics, TU Dortmund University, D-44221 Dortmund, Germany, 89 SOMM17/6104/UGR), Generalitat Valenciana: Grisolía (ref. Export citation and abstract In this Letter a search is performed at the ATLAS experiment for slow-moving charged The vertical dashed line marks the decl. filmgeschÄftsfÜhrung / accountants. Please reconnect, Authors & archiv und recherche / archive research. 10001 Rabat, Morocco, 11 Shower-like events are induced by neutral current (NC) interactions, as well as by CC interactions of electron and tau neutrinos and antineutrinos, and are characterized by an almost spherically symmetric light emission around the shower maximum. 0. Moreover, the position of the source is either kept fixed or fitted within specific limits, depending on the type of search (see Section 5). The signal and background PDFs are given by the product of a directional and an energy-dependent term. Results of the Candidate List Search. All rights reserved. You will need to select a minimum of one corridor. 2,-40\buildrel{\circ}\over{.} Please note, The Astrophysical Journal Letters (ApJL) and Research Notes of the AAS (RNAAS) of Astronomy, University of Wisconsin, Madison, WI 53706, USA, 85 A. Albert1,2, M. André3, M. Anghinolfi4, G. Anton5, M. Ardid6, J.-J. iv The American Astronomical Society. Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland, 53 102 Also at Università di Padova, I-35131 Padova, Italy. A quantum chemical study. 10000, Morocco, 13 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. The countries are listed according to the national teams of the senior family member if the other family member played for a different country. 7, D-96049 Bamberg, Germany, 37 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. Pascal Köpke wurde am 03.09.1995 in Hanau geboren. montage assistent / assistant editor. 2017c), respectively, are combined to perform various searches for point-like and extended sources of neutrinos in the Southern Sky. INFN—Sezione di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa, Italy, 44 In this work, the point-source data samples of the ANTARES (Ageron et al. The largest excess above the background is found for a point-like source hypothesis, with best-fit {\hat{n}}_{{\rm{s}}}=2.9 and \hat{\gamma }=2.1, and a significance of 6% (1.6σ in the one-sided sigma convention). Kennzeichen der Band ist es, dass die Texte sehr puristisch sind. Exploiting these different characteristics allows for a significant gain in sensitivity for searches in the Southern Sky. Mono-oxo-bis-dithioveratrol-molybdate - in Solution a Model for Arsenite Oxidase and in the Solid State a Coordination Polymer with Unprecedented Binding Motifs. Dept. 2017c) is employed in this search. 2,-40\buildrel{\circ}\over{.} 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. Dept. Figure 4 depicts the pretrial p-values for all the investigated directions for a point-like source hypothesis. Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France, 8 Figure 5. Equipartition at Earth of the three neutrino flavors is assumed. of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA, 57 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. List of astrophysical objects analyzed in the candidate list search. 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. Search the world's information, including webpages, images, videos and more. (2014). INFN—Sezione di Napoli, Via Cintia I-80126 Napoli, Italy, 46 Trotzdem musste der FCN am Ende eine bittere 2:3-Niederlage in Braunschweig hinnehmen. 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. National Center for Energy Sciences and Nuclear Techniques, B.P. Project Leader(s): Köpke, Prof.Dr. You need an eReader or compatible software to experience the benefits of the ePub3 file format. In each box, the unbinned likelihood maximization is performed, with the source position being an additional parameter that is free to vary inside the 1° × 1° boundaries. 1, D-91058 Erlangen, Germany, 6 It has a worldwide membership of around 50 000 comprising physicists from all sectors, as well as those with an interest in physics. A pretrial p-value of 1.3 × 10−5 is obtained for this cluster. BibTeX Karlsruhe Institute of Technology, Institut für Kernphysik, D-76021 Karlsruhe, Germany, 60 upper limits on the one-flavor neutrino flux normalization for an {E}_{\nu }^{-2.0} and an {E}_{\nu }^{-2.5} spectrum. of Physics, University of California, Berkeley, CA 94720, USA, 63 Polymer-Supported Dioxido-MoVI Complexes as Truly Functional Molybdenum Oxotransferase Model Systems. (2007), in the following indicated as RXJ 1713.7-3946 (1), and the one recently introduced for KM3NeT neutrino source search estimations (Aiello et al. Neutrinos are stable, neutral, and weakly interacting particles and, in contrast to cosmic rays, they are not deflected by magnetic fields. Sagittarius A*, the SMBH located at the center of our Galaxy, (α, δ) = (26642, − 2901), is a candidate source of particular interest. Dr. Remeis-Sternwarte and ECAP, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. Dept. The Monomerization of a Binuclear Molybdenum(VI) Dioxo Complex by an Unusual Silylation Reaction. For each box, the best-fit values of the number of signal events, {\hat{n}}_{{\rm{s}}}, spectral index, \hat{\gamma }, source equatorial coordinates, \hat{\delta } and \hat{\alpha }, and the test statistic, Q, are obtained. 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. 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. Dept. -pyrazolate ligands: crystal structure and oxo transfer properties. of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Dr., Anchorage, AK 99508, USA, 99 of Physics and Astronomy, University of Gent, B-9000 Gent, Belgium, 81 1 Dept. ) and W( 1,-40\buildrel{\circ}\over{.} of Physics, Yale University, New Haven, CT 06520, USA, 97 Both models describe a neutrino spectrum of the form of: where Eν is the neutrino energy and the values of the neutrino spectrum parameters Φ0, Γ, Ecut, and β are listed in Table 6. INFN—Sezione di Bari, Via E. Orabona 4, I-70126 Bari, Italy, 23 This analysis shows the strong potential to search for neutrino sources in the Southern Sky using the joint data sets of the ANTARES and IceCube telescopes. Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. Moscow State University, Skobeltsyn Institute of Nuclear Physics, Leninskie gory, 119991 Moscow, Russia, 38 Differently from high-energy photons, neutrinos are effectively not absorbed while traveling through cosmological distances and can escape from dense astrophysical environments. The first molybdenum dioxo compounds with η The largest excess over the background was observed at an angular extension of 00 with a significance of 6%. Universiteit van Amsterdam, Instituut voor Hoge-Energie Fysica, Science Park 105, 1098 XG Amsterdam, The Netherlands, 17 Wir besprechen ihre Perspektiven. (Vissani 2006; Villante & Vissani 2008; Vissani & Villante 2008), hereafter referred to as RXJ 1713.7-3946 (2). Royal Netherlands Institute for Sea Research (NIOZ) and Utrecht University, Landsdiep 4, 1797 SZ 't Horntje (Texel), The Netherlands, 33 This site uses cookies. of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA, 70 Why is the molybdenum-substituted tungsten-dependent formaldehyde ferredoxin oxidoreductase not active? Runs 2007 - 2008. Description. Back In contrast, ANTARES' detected events are predominantly atmospheric neutrinos because the Earth acts as a shield for atmospheric muons. Figure 4. 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. 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. The American Astronomical Society. This is a list of association football families. Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France, 10 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{.} Oxido-alcoholato/thiolato-molybdenum(VI) complexes with a dithiolene ligand generated by oxygen atom transfer to the molybdenum(IV) complexes. Synthesis and characterization of cyano and isocyano complexes of bis(dithiolato) molybdenum using Me The relative contribution Cj(δ, Φ) for each sample j, defined as the ratio of the expected mean number of signal events for the given sample to that for all samples, {C}^{j}={N}^{j}/{\sum }_{i=1}^{7}{N}^{i}, depends on the expected flux from the source Φ and decl. The ANTARES events were selected by applying cuts on the zenith angle, the angular error estimate, and parameters describing the quality of the reconstruction. In this analysis, two different models are considered for the neutrino emission: that proposed by Kappes et al. Dept. Der FCN hat jede Menge nominelle Mittelstürmer und hat trotzdem noch zwei weitere hinzugefügt. Dept. jÜrg bÄnziger. }/{{\rm{\Phi }}}_{0}. Sagittarius A* was tested as a point-like source and as an extended source. The 90% C.L. Juni 1996 sowie von Folge 1497 am 19. 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. Dept. Bioinorganic chemistry of molybdenum and tungsten enzymes: A structural–functional modeling approach. Citation A. Albert et al 2020 ApJ 892 92. The paper is organized as follows. Common backgrounds in both detectors are atmospheric muons and neutrinos originating from cosmic-ray interactions in Earth's atmosphere. Revised 2020 February 26 3 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. 8), for a point-like source hypothesis, with best-fit {\hat{n}}_{{\rm{s}}}=5.7 and \hat{\gamma }=2.5. Figure 2. de Física Teórica y del Cosmos & C.A.F.P.E., University of Granada, E-18071 Granada, Spain, 42 Several classes of astrophysical objects, such as supernova remnants, pulsar wind nebulae, and active galactic nuclei (AGNs) have been indicated as promising high-energy neutrino source candidates (Gaisser et al. The values of the best-fit parameters at the investigated location for the various tested source extensions are presented in Table 5, together with the observed p-value. 2014; Aartsen et al. 31, D-97074 Würzburg, Germany. Sie war in Gute Zeiten, Schlechte Zeiten ab Folge 713 von März 1995 bis Folge 1010 am 27. Dept. Dept. The oxygen-atom transfer reactions of Mo-diselenolene biomimetic complexes: A computational investigation. The 90% C.L. produktionsassistenz / production assistant. Accepted 2020 February 26 Click here to close this overlay, or press the "Escape" key on your keyboard. 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. of Physics, Marquette University, Milwaukee, WI 53201, USA, 54 on the one-flavor neutrino flux normalization from the analyzed candidates (green dots) reported in Table 4 as a function of the source decl. The fitted number of signal events and the p-value observed at the source position are presented in Table 6 for each spectrum hypothesis, together with the 90% C.L. 1014, R.P. High-resolution molybdenum K-edge X-ray absorption spectroscopy analyzed with time-dependent density functional theory. The second- and third-most significant sources are PKS1440-389 and HESSJ1458-608, with respective p-values of 0.85% and 3.6%. Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany, 74 The mission of the AAS is to enhance and share humanity's scientific understanding of the universe. Am Wochenende schnürte Nürnbergs Sturm-Neuzugang Pascal Köpke (25) gleich bei seinem Startdebüt seinen ersten Doppelpack. Bartol Research Institute and Dept. Er ist 26 Jahre alt und seine Staatsbürgerschaft ist Deutschland. 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. Dept. Dipartimento di Fisica dell'Università, Largo B. Pontecorvo 3, I-56127 Pisa, Italy, 45 We will gladly send you a new password via email. By setting {n}_{{\rm{s}}}^{\min } slightly above 0, the test statistic Q gets negative values for underfluctuation of the signal. Molybdenum and tungsten enzymes redox properties – A brief overview. Mechanism of Nitrate Reduction byDesulfovibrio desulfuricans Nitrate Reductase—A Theoretical Investigation. Microbial biosynthesis of alkanes is considered a promising method for the sustainable production of drop-in fuels and chemicals. Physik-department, Technische Universität München, D-85748 Garching, Germany, 86 0) at equatorial coordinates (\hat{\alpha },\hat{\delta })=(274\buildrel{\circ}\over{.} of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand, 49 Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany, 67 of the Galactic Center. In addition, special focus is given to the region around the Galactic Center, whereby a dedicated search at the location of SgrA* is performed, and to the location of the supernova remnant RXJ 1713.7-3946. The authors of the IceCube Collaboration acknowledge the support from the following agencies and institutions: USA—U.S. The green line indicates the results for the combined search. 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 Google has many special features to help you find exactly what you're looking for. For each model, the values of the neutrino spectrum parameters, Φ0, Γ, Ecut, and β entering Equation (5) are provided. In this analysis, the Neyman method (Neyman 1937) is used to derive sensitivities and limits. Kim Scheele wurde von Alexandra Finder gespielt. Nikhef, Science Park, Amsterdam, The Netherlands, 15 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 }}). Five types of searches for point-like and extended sources are performed in this analysis. Oskar Klein Centre and Dept. Necessity of fine tuning in Mo(iv) bis(dithiolene) complexes to warrant nitrate reduction. 2019). Dept. Dioxomolybdenum(vi) and dioxotungsten(vi) complexes supported by an amido ligand. 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). The values of the best-fit {\hat{n}}_{{\rm{s}}} and \hat{\gamma } are 20.3 and 3.0, respectively. Figure 3 shows the pretrial p-values for the investigated directions in the Galactic Center region for an extended source hypothesis with {\sigma }_{{\rm{s}}}=2\buildrel{\circ}\over{.} Journal of Molecular Catalysis A: Chemical. 31, D-97074 Würzburg, Germany 29 Dipartimento di Fisica e Astronomia dell’Università, Viale … of Physics, Mercer University, Macon, GA 31207-0001, USA, 98 Results of the Search at the Location of Sagittarius A*. 8), for a point-like source hypothesis. 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. 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. 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. Köpke und seine Kim - FCN-Stürmer liebt Promi-Tochter. selenolato complex to oxygen. of Astronomy, Ohio State University, Columbus, OH 43210, USA, 64 1995; Halzen & Hooper 2002; Becker 2008; Kelner & Aharonian 2008; Murase 2015). Photoinduced electron transfer from the oxo–Mo 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.

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