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description Publicationkeyboard_double_arrow_right Article , Other literature type 2020 FrancePublisher:Elsevier BV Tarik Bouramtane; Suzanne Yameogo; Meryem Touzani; Abdessamad Tiouiouine; M’hamed El janati; Jamila Ouardi; Ilias Kacimi; Vincent Valles; Laurent Barbiero;International audience; 12 13 Abstract: 14 Several studies have revealed that the complexity in the distribution of drainage network patterns is not 15 random and controlled by major parameters, variable in space but also throughout geological time. Drainage 16 networks in the Eastern Anti-Atlas of Morocco consist of complex spatial arrangements with various types of 17 patterns, such as trellis, angular, dendritic and parallel. The objective was to distinguish, quantify and rank 18 the relationship that may exist between the different drainage networks patterns, geology and 19 geomorphology. A total of 230 basins were extracted from the ASTER-GDEM Elevation Data (USGS), which 20 were assigned 16 parameters reflecting their topography, morphometry, slope and geology. The statistical 21 treatment of the dataset (16 variables x 230 observations) was carried out through principal component 22 analysis (PCA), linear discriminant analysis (LDA) and agglomerative hierarchical clustering (AHC), in order to 23 investigate the complexity of drainage network patterns and their distribution. The PCA showed that the 24 topographical, slope and geological parameters, i.e. primarily the parameter associated with structural 25 control, best explains the variation in the type of the drainage pattern. The LDA made it possible to distinguish 26 between the four types of drainage patterns with a success rate of 90%, using 3 discriminant functions that 27 were better correlated with geological and slope parameters. LDA and AHC statistical treatments show 28 confusion between the parallel, trellis and angular patterns, on the one hand, due to similar factors 29 responsible for their formation, and on the other because of transitions phenomenon from one drainage 30 pattern to another over time or space. Such possible drainage network shifting may be explained by the 31 geological events that have occurred in the Eastern Anti Atlas from Lower Mesozoic to the Quaternary. 32 33
Journal of African E... arrow_drop_down Journal of African Earth SciencesArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routesbronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Journal of African E... arrow_drop_down Journal of African Earth SciencesArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2019 Netherlands, Spain, Italy, Netherlands, Italy, Spain, Italy, Italy, Italy, Italy, Netherlands, Netherlands, Italy, Spain, France, Netherlands, Spain, Italy, Netherlands, Italy, ItalyPublisher:Elsevier BV Funded by:EC | INPhINIT, ANR | DAEMONS, ANR | UnivEarthS +1 projectsEC| INPhINIT ,ANR| DAEMONS ,ANR| UnivEarthS ,ANR| USPCThe KM3NeT Collaboration,; Aiello, S.; Akrame, S. E.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aublin, J.; Avgitas, T.; Bagatelas, C.; Barbarino, G.; Baret, B.; Barrios-Martí, J.; Belias, A.; Berbee, E.; van den Berg, A.; Bertin, V.; Biagi, S.; Biagioni, A.; Biernoth, C.; Boumaaza, J.; Bourret, S.; Bouta, M.; Bouwhuis, M.; Bozza, C.; Brânzas, H.; Bruchner, M.; Bruijn, R.; Brunner, J.; Buis, E.; Buompane, R.; Busto, J.; Calvo, D.; Capone, A.; Celli, S.; Chabab, M.; Chau, N.; Cherubini, S.; Chiarella, V.; Chiarusi, T.; Circella, M.; Cocimano, R.; Coelho, J. A. B.; Coleiro, A.; Colomer Molla, M.; Coniglione, R.; Coyle, P.; Creusot, A.; Cuttone, G.; D'Onofrio, A.; Dallier, R.; De Sio, C.; Di Palma, I.; Díaz, A. F.; Diego-Tortosa, D.; Distefano, C.; Domi, A.; Donà, R.; Donzaud, C.; Dornic, D.; Dörr, M.; Durocher, M.; Eberl, T.; van Eijk, D.; El Bojaddaini, I.; Eljarrari, H.; Elsaesser, D.; Enzenhöfer, A.; Fermani, P.; Ferrara, G.; Filipovic, M. D.; Fusco, L. A.; Gal, T.; Garcia, A.; Garufi, F.; Gialanella, L.; Giorgio, E.; Giuliante, A.; Gozzini, S. R.; Gracia, R.; Graf, K.; Grasso, D.; Grégoire, T.; Grella, G.; Hallmann, S.; Hamdaoui, H.; van Haren, H.; Heid, T.; Heijboer, A.; Hekalo, A.; Hernández-Rey, J. J.; Hofestädt, J.; Illuminati, G.; James, C. W.; Jongen, M.; de Jong, M.; de Jong, P.; Kadler, M.; Kalaczynski, P.; Kalekin, O.; Katz, U. F.; Khan Chowdhury, N. R.; Kiessling, D.; Koffeman, E. N.; Kooijman, P.; Kouchner, A.; Kreter, M.; Kulikovskiy, V.; Kunhikannan-Kannichankandy, M.; Lahmann, R.; Larosa, G.; Le Breton, R.; Leone, F.; Leonora, E.; Levi, G.; Lincetto, M.; Lonardo, A.; Longhitano, F.; Lopez Coto, D.; Lotze, M.; Maderer, L.; Maggi, G.; Manczak, J.; Mannheim, K.; Margiotta, A.; Marinelli, A.; Markou, C.; Martin, L.; Martínez-Mora, J. A.; Martini, A.; Marzaioli, F.; Mele, R.; Melis, K. W.; Migliozzi, P.; Migneco, E.; Mijakowski, P.; Miranda, L. S.; Mollo, C. M.; Morganti, M.; Moser, M.; Moussa, A.; Muller, R.; Musumeci, M.; Nauta, L.; Navas, S.; Nicolau, C. A.; Nielsen, C.; Ó Fearraigh, B.; Organokov, M.; Orlando, A.; Ottonello, S.; Panagopoulos, V.; Papalashvili, G.; Papaleo, R.; Păvălaş, G. E.; Pellegrino, C.; Perrin-Terrin, M.; Piattelli, P.; Pikounis, K.; Pisanti, O.; Poirè, C.; Polydefki, G.; Popa, V.; Post, M.; Pradier, T.; Pühlhofer, G.; Pulvirenti, S.; Quinn, L.; Raffaelli, F.; Randazzo, N.; Razzaque, S.; Real, D.; Resvanis, L.; Reubelt, J.; Riccobene, G.; Richer, M.; Rigalleau, L.; Rovelli, A.; Saffer, M.; Salvadori, I.; Samtleben, D. F. E.; Sánchez Losa, A.; Sanguineti, M.; Santangelo, A.; Santonocito, D.; Sapienza, P.; Schumann, J.; Sciacca, V.; Seneca, J.; Sgura, I.; Shanidze, R.; Sharma, A.; Simeone, F.; Sinopoulou, A.; Spisso, B.; Spurio, M.; Stavropoulos, D.; Trovato, A.;KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the detection of high-energy neutrinos of cosmic origin. Thanks to its geographical location on the Northern hemisphere, KM3NeT/ARCA can observe upgoing neutrinos from most of the Galactic Plane, including the Galactic Centre. Given its effective area and excellent pointing resolution, KM3NeT/ARCA will measure or significantly constrain the neutrino flux from potential astrophysical neutrino sources. At the same time, it will test flux predictions based on gamma-ray measurements and the assumption that the gamma-ray flux is of hadronic origin. Assuming this scenario, discovery potentials and sensitivities for a selected list of Galactic sources and to generic point sources with an $E^{-2}$ spectrum are presented. These spectra are assumed to be time independent. The results indicate that an observation with $3\sigma$ significance is possible in about six years of operation for the most intense sources, such as Supernovae Remnants RX\,J1713.7-3946 and Vela Jr. If no signal will be found during this time, the fraction of the gamma-ray flux coming from hadronic processes can be constrained to be below 50\% for these two objects. Comment: 32 pages, 9 figures, submitted to Astroparticle Physics
IRIS - Università de... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; NARCISArticle . 2019NARCISArticle . 2019Full-Text: https://pure.uva.nl/ws/files/64663217/Sensitivity_of_the_KM3NeT_ARCA_neutrino_telescope.pdfData sources: NARCISRecolector de Ciencia Abierta, RECOLECTAArticle . 2019License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; RiuNet; Recolector de Ciencia Abierta, RECOLECTA; NARCISOther literature type . Article . 2019 . Peer-reviewedLicense: Elsevier TDMArchivio della ricerca- Università di Roma La SapienzaArticle . 2019Data sources: Archivio della ricerca- Università di Roma La SapienzaIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019Recolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2020 . 2019UPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCLeiden University Scholarly Publications RepositoryOther literature type . 2019License: CC BY NC NDData sources: Leiden University Scholarly Publications RepositoryArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernohttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 70 citations 70 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 246visibility views 246 download downloads 1,085 Powered bymore_vert IRIS - Università de... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; NARCISArticle . 2019NARCISArticle . 2019Full-Text: https://pure.uva.nl/ws/files/64663217/Sensitivity_of_the_KM3NeT_ARCA_neutrino_telescope.pdfData sources: NARCISRecolector de Ciencia Abierta, RECOLECTAArticle . 2019License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; RiuNet; Recolector de Ciencia Abierta, RECOLECTA; NARCISOther literature type . Article . 2019 . Peer-reviewedLicense: Elsevier TDMArchivio della ricerca- Università di Roma La SapienzaArticle . 2019Data sources: Archivio della ricerca- Università di Roma La SapienzaIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019Recolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2020 . 2019UPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCLeiden University Scholarly Publications RepositoryOther literature type . 2019License: CC BY NC NDData sources: Leiden University Scholarly Publications RepositoryArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernohttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2019 FrancePublisher:Wiley Authors: Houda El Kerni; Hasnaa Chennaoui Aoudjehane; David Baratoux; Mohammed Aoudjehane; +14 AuthorsHouda El Kerni; Hasnaa Chennaoui Aoudjehane; David Baratoux; Mohammed Aoudjehane; André Charrière; Hassan Ibouh; Pierre Rochette; Yoann Quesnel; Minoru Uehara; Thomas Kenkmann; G. Wulf; Michael H. Poelchau; van Binh Nguyen; Hassan Aboulahris; Hassan Makhoukhi; Georges Aumaître; Didier Bourlès; Karim Keddadouche;doi: 10.1111/maps.13347
AbstractSince the discovery of shatter cones (SCs) near the village of Agoudal (Morocco, Central High Atlas Mountains) in 2013, the absence of one or several associated circular structures led to speculation about the age of the impact event, the number, and the size of the impact crater or craters. Additional constraints on the crater size, age, and erosion rates are obtained here from geological, structural, and geophysical mapping and from cosmogenic nuclide data. Our geological maps of the Agoudal impact site at the scales of 1:30,000 (6 km2) and 1:15,000 (2.25 km2) include all known occurrences of SCs in target rocks, breccias, and vertical to overturned strata. Considering that strata surrounding the impact site are subhorizontal, we argue that disturbed strata are related to the impact event. Three types of breccias have been observed. Two of them (br1‐2 and br2) could be produced by erosion–sedimentation–consolidation processes, with no evidence for impact breccias, while breccia (br1) might be impact related. The most probable center of the structure is estimated at 31°59′13.73ʺN, 5°30′55.14ʺW using the concentric deviation method applied to the orientation of strata over the disturbed area. Despite the absence of a morphological expression, the ground magnetic and electromagnetic surveys reveal anomalies spatially associated with disturbed strata and SC occurrences. The geophysical data, the structural observations, and the area of occurrence of SCs in target rocks are all consistent with an original size of 1.4–4.2 km in diameter. Cosmogenic nuclide data (36Cl) constrain the local erosion rates between 220 ± 22 m Ma−1 and 430 ± 43 m Ma−1. These erosion rates may remove the topographic expression of such a crater and its ejecta in a time period of about 0.3–1.9 Ma. This age is older than the Agoudal iron meteorite age (105 ± 40 kyr). This new age constraint excludes the possibility of a genetic relationship between the Agoudal iron meteorite fall and the formation of the Agoudal impact site. A chronolgy chart including the Atlas orogeny, the alternation of sedimentation and erosion periods, and the meteoritic impacts is presented based on all obtained and combined data.
Horizon / Pleins tex... arrow_drop_down Meteoritics and Planetary ScienceArticle . 2019 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!more_vert Horizon / Pleins tex... arrow_drop_down Meteoritics and Planetary ScienceArticle . 2019 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1111/maps.13347&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2019 Netherlands, France, Italy, Italy, Netherlands, Germany, Netherlands, Italy, Italy, Netherlands, Belgium, Czech Republic, Brazil, Belgium, Italy, Italy, Italy, Netherlands, Italy, ItalyPublisher:Frontiers Media SA Funded by:ANR | SUPER, NSF | Pierre Auger Project, EC | EPLANETANR| SUPER ,NSF| Pierre Auger Project ,EC| EPLANETA. Aab; P. Abreu; M. Aglietta; I. F. M. Albuquerque; J. M. Albury; I. Allekotte; A. Almela; J. Alvarez Castillo; J. Alvarez-Muñiz; G. A. Anastasi; L. Anchordoqui; B. Andrada; S. Andringa; C. Aramo; H. Asorey; P. Assis; G. Avila; A. M. Badescu; A. Bakalova; A. Balaceanu; F. Barbato; R. J. Barreira Luz; S. Baur; K. H. Becker; J. A. Bellido; C. Berat; M. E. Bertaina; X. Bertou; P. L. Biermannb; J. Biteau; S. G. Blaess; A. Blanco; J. Blazek; C. Bleve; M. Boháˇcová; D. Boncioli; C. Bonifazi; N. Borodai; A. M. Botti; J. Bracke; T. Bretz; A. Bridgeman; F. L. Briechle; P. Buchholz; A. Bueno; S. Buitink; M. Buscemi; K. S. Caballero-Mora; L. Caccianiga; L. Calcagni; A. Cancio; F. Canfora; J. M. Carceller; R. Caruso; A. Castellina; F. Catalani; G. Cataldi; L. Cazon; M. Cerda; J. A. Chinellato; J. Chudoba; L. Chytka; R. W. Clay; A. C. Cobos Cerutti; R. Colalillo; A. Coleman; M. R. Coluccia; R. Conceição; A. Condorelli; G. Consolati; F. Contreras; F. Convenga; M. J. Cooper; S. Coutu; C. E. Covault; B. Daniel; S. Dasso; K. Daumiller; B. R. Dawson; J. A. Day; R. M. de Almeida; S. J. de Jong; G. De Mauro; J. R. T. de Mello Neto; I. De Mitri; J. de Oliveira; F. O. de Oliveira Salles; V. de Souza; J. Debatin; M. del Río; O. Deligny; N. Dhital; M. L. Díaz Castro; F. Diogo; C. Dobrigkeit; J. C. D’Olivo; Q. Dorosti; R. C. dos Anjos; M. T. Dova; A. Dundovic; J. Ebr; R. Engel; M. Erdmann; C. O. Escobarc; A. Etchegoyen; H. Falcke; J. Farmer; G. Farrar; A. C. Fauth; N. Fazzinic; F. Feldbusch; F. Fenu; L. P. Ferreyro; J. M. Figueira; A. Filipˇciˇc; M. M. Freire; T. Fujii; f; A. Fuster; B. García; H. Gemmeke; A. Gherghel-Lascu; P. L. Ghia; U. Giaccari; M. Giammarchi; M. Giller; D. Głas; J. Glombitza; F. Gobbi; G. Golup; M. Gómez Berisso; P. F. Gómez Vitale; J. P. Gongora; N. González; I. Goos; D. Góra; A. Gorgi; M. Gottowik; T. D. Grubb; F. Guarino; G. P. Guedes; E. Guido; R. Halliday; M. R. Hampel; P. Hansen; D. Harari; T. A. Harrison; V. M. Harvey; A. Haungs; T. Hebbeker; D. Heck; P. Heimann; G. C. Hill; C. Hojvatc; E. M. Holt; P. Homola; J. R. Hörandel; P. Horvath; M. Hrabovský; T. Huege; J. Hulsman; A. Insolia; P. G. Isar; I. Jandt; J. A. Johnsen; M. Josebachuili; J. Jurysek; A. Kääpä; K. H. Kampert; B. Keilhauer; N. Kemmerich; J. Kemp; H. O. Klages; M. Kleifges; J. Kleinfeller; R. Krause; D. Kuempel; G. Kukec Mezek; A. Kuotb Awad; B. L. Lago; D. LaHurd; R. G. Lang; R. Legumina; M. A. Leigui de Oliveira; V. Lenok; A. Letessier-Selvon; I. Lhenry-Yvon; O. C. Lippmann; D. Lo Presti; L. Lopes; R. López; A. López Casado; R. Lorek; Q. Luce; A. Lucero; M. Malacari; G. Mancarella; D. Mandat; B. C. Manning; P. Mantschc; L. Miramonti; L. Valore; F. Zuccarello;An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results are reviewed, such as stringent upper bounds that were placed to a flux of diffuse cosmogenic neutrinos and photons, bounds placed on neutrinos emitted from compact binary mergers that were detected by LIGO and Virgo during their first and second observing runs, as well as searches for high energy photons and neutrons from the Galactic center that constrain the properties of the putative Galactic PeVatron, observed by the H.E.S.S. collaboration. The observation of directional correlations between ultra-high energy cosmic rays and either high energy astrophysical neutrinos or specific source populations, weighted by their electromagnetic radiation, are also discussed. They constitute additional multi-messenger approaches aimed at identifying the sources of high energy cosmic rays. info:eu-repo/semantics/published SCOPUS: re.j
NARCIS; Radboud Repo... arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019Archivio Istituzionale della Ricerca- Università del Salento; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; Frontiers in Astronomy and Space Sciences; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoReview . Other literature type . Article . 2019 . Peer-reviewedLicense: CC BYData sources: Archivio Istituzionale della Ricerca- Università del Salento; University of Groningen Research Portal; Crossref; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; NARCIS; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaPublikationsserver der RWTH Aachen UniversityArticle . 2019Data sources: Publikationsserver der RWTH Aachen UniversityVrije Universiteit Brussel Research PortalOther literature type . 2019Data sources: Vrije Universiteit Brussel Research PortalFrontiers in Astronomy and Space SciencesArticle . 2019Data sources: METIS Research Information SystemOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 18 citations 18 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!more_vert NARCIS; Radboud Repo... arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019Archivio Istituzionale della Ricerca- Università del Salento; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; Frontiers in Astronomy and Space Sciences; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoReview . Other literature type . Article . 2019 . Peer-reviewedLicense: CC BYData sources: Archivio Istituzionale della Ricerca- Università del Salento; University of Groningen Research Portal; Crossref; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; NARCIS; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaPublikationsserver der RWTH Aachen UniversityArticle . 2019Data sources: Publikationsserver der RWTH Aachen UniversityVrije Universiteit Brussel Research PortalOther literature type . 2019Data sources: Vrije Universiteit Brussel Research PortalFrontiers in Astronomy and Space SciencesArticle . 2019Data sources: METIS Research Information SystemOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2018 Spain, Spain, FrancePublisher:Elsevier BV Funded by:EC | EUROFLEETSEC| EUROFLEETSLafosse, M.; Gorini, C. (Christian); Le Roy, P.; Alonso, B. (Belén); D'Acremont, E. (Elia); Ercilla, G. (Gemma); Rabineau, M. (Marina); Vázquez, J.T. (Juan Tomás); Rabaute, A.; Ammar, A.;handle: 10261/172851 , 10508/15121
In active basins, tectonics can segment the continental shelf and control its stratigraphic architecture and physiography. Segmentation can explain the local evolution and morphology of the continental shelf because of sea-level variations, local tectonic segmentation and hydrodynamic processes. Here we investigate the tectonically active Morocco continental margin (southern Alboran Sea) using high-resolution seismic profiles and multibeam bathymetric data. The active faults bounding the transtensive Nekor basin triggered the segmentation of the shelf into three sectors showing different subsidence rates: a western sector corresponding to an extensive fault relay, a central sector corresponding to the subsiding Al-Hoceima Bay and an eastern sector corresponding to the footwall of the Trougout senestral normal fault. Results show that the staircase morphology of the shelf corresponds to successive submarine terraces at the shelf edge (ST1), mid-shelf (ST2) and inner-shelf (ST3) around −110 m,-80 m, and −40 to −20 m deep, respectively. The terraces correspond to the top of prograding wedges seaward and are erosive landward. They are correlated with stillstand from the Last Glacial Maximum to the Holocene highstand. Above the terraces, sub-aqueous dune fields are interpreted as degraded and deposited during the post-glacial transgression. In the central sector, typical delta front seafloor undulations on the shelf and crescent shaped bedforms at the head of marine incisions on the upper slope denote a fluvial influence during the Holocene. Seismic stratigraphy analysis revealed the preservation of six seismic units bounded by polygenic regional unconformities (S1, S2, S3, S4 and S5). Based on comparison with other Mediterranean margins, S1 to S5 are attributed to 4th order maximum regressive surface. We discuss the local preservation of the system tracts as a function of the vertical motion and the physiography of this tectonically active domain. This study provides useful clues for future local paleo-seismic analysis and to advance our understanding of sedimentary processes in active areas This work was funded by the French program Actions Marges, the EUROFLEETS program (FP7/2007-2013; n°228344), project FICTS-2011-03-01. Seismic reflection data were processed using the Seismic UNIX SU and Geovecteur software. [...]. This work also benefited from a State Grant from the French Agence Nationale de la Recherche (ANR) in the Program « Investissements d'avenir » reference ANR-10-LABX-19-01, Labex Mer and from the Fauces Project (Ref CTM2015-65461-C2-R; MINCIU/FEDER) financed by "Ministerio de Economía y Competitividad y al Fondo Europeo de Desarrollo Regional" (FEDER) 20 pages, 14 figures, 1 table Peer Reviewed
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2018Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTA; Marine and Petroleum GeologyArticle . 2018 . Peer-reviewedArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMarine and Petroleum GeologyArticle . 2018 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2018add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 19visibility views 19 download downloads 67 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2018Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTA; Marine and Petroleum GeologyArticle . 2018 . Peer-reviewedArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMarine and Petroleum GeologyArticle . 2018 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2018add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Review , Article 2017 France, BelgiumPublisher:Cambridge University Press (CUP) Benammi , Mouloud; Adnet , Sylvain; Marivaux , Laurent; Yans , Johan; Noiret , Corentin; Tabuce , Rodolphe; SURAULT , JÉRÔME; EL KATI , IMAD; Enault , Sebastien; BAIDDER , LAHSSEN; Saddiqi , Omar; Benammi , Mohamed;AbstractNew Palaeogene vertebrate localities were recently reported in the southern Dakhla area (southwestern Morocco). The Eocene sediment strata crops out on cliffs along the Atlantic Ocean coast. Vertebrate remains come from five conglomeratic sandstone beds and are principally represented by isolated teeth belonging to micromammals, selachians and bony fishes, a proboscidean assigned to ?Numidotheriumsp. and many remains of archaeocete whales (Basilosauridae). From fieldwork five lithostratigraphic sections were described, essentially based on the lithological characteristic of sediments. Despite the lateral variations of facies, correlations between these five sections were possible on the basis of fossil-bearing beds (A1, B1, B2, C1 and C2) and five lithological units were identified. The lower part of the section consists of rhythmically bedded, chert-rich marine siltstones and marls with thin black phosphorite with organic matter at the base. The overlying units include coarse-grained to microconglomeratic sandstones interbedded with silts, indicating deposition in a shallow-marine environment with fluvial influence. The natural remanence magnetization of a total of 50 samples was measured; the intensity of most of the samples is too weak however, before or after the first step of demagnetization. The palaeomagnetic data from the samples are very unstable, except for eight from three similar sandstone levels which show a normal polarity. Matched with biostratigraphic data on rodents, primates, the selachian, sirenian and cetacean faunas, the new carbon isotope chemostratigraphy on organics (1) refines the age of the uppermost C2 fossil-bearing bed to earliest Oligocene time and (2) confirms the Priabonian age of the B1 to C1 levels.
Geological Magazine arrow_drop_down Geological MagazineArticle . 2017 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefHyper Article en Ligne; Mémoires en Sciences de l'Information et de la Communication; Hal-DiderotOther literature type . Conference object . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/s0016756817000851&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 8 citations 8 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Geological Magazine arrow_drop_down Geological MagazineArticle . 2017 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefHyper Article en Ligne; Mémoires en Sciences de l'Information et de la Communication; Hal-DiderotOther literature type . Conference object . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type , Preprint 2017 Italy, Spain, Netherlands, Italy, Italy, Netherlands, Italy, Italy, Netherlands, Italy, Italy, France, Netherlands, Italy, SpainPublisher:Sissa Medialab Funded by:ANR | OCEVU, ANR | USPCANR| OCEVU ,ANR| USPCAlbert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J. -.J.; Avgitas, T.; Baret, B.; Barrios-MartÃ, J.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Bruijn, R.; Brunner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Cherkaoui El Moursli, R.; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; DÃaz, A. F.; Deschamps, A.; De Bonis, G.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; El Bojaddaini, I.; El Khayati, N.; Elsässer, D.; Enzenhöfer, A.; Ettahiri, A.; Fassi, F.; Felis, I.; Fusco, L. A.; Galatà , S.; Gay, P.; Giordano, V.; Glotin, H.; Grégoire, T.; Gracia Ruiz, R.; Graf, K.; Hallmann, S.; Van Haren, H.; Heijboer, A. J.; Hello, Y.; Hernández-Rey, J. J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C. W.; De Jong, M.; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; LefÃvre, D.; Leonora, E.; Lotze, M.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; MartÃnez-Mora, J. A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Navas, S.; Nezri, E.; Organokov, M.; PÇŽvÇŽlaÅŸ, G. E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sánchez-Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; SchÃ1⁄4ssler, F.; Sieger, C.; Spurio, M.; Stolarczyk, T.h.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, C.; Vallage, B.; Van Elewyck, V.; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J. D.; ZÃoñiga, J.; Gaggero, D.; Grasso, D.;The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization of this flux will shed light on Galactic accelerator features, gas distribution morphology and Galactic cosmic ray transport. The central Galactic plane can be the site of an enhanced neutrino production, thus leading to anisotropies in the extraterrestrial neutrino signal as measured by the IceCube Collaboration. The ANTARES neutrino telescope, located in the Mediterranean Sea, offers a favourable view on this part of the sky, thereby allowing for a contribution to the determination of this flux. The expected diffuse Galactic neutrino emission can be obtained linking a model of generation and propagation of cosmic rays with the morphology of the gas distribution in the Milky Way. In this paper, the so-called "Gamma model" introduced recently to explain the high-energy gamma ray diffuse Galactic emission, is assumed as reference. The neutrino flux predicted by the "Gamma model" depends of the assumed primary cosmic ray spectrum cut-off. Considering a radially-dependent diffusion coefficient, this proposed scenario is able to account for the local cosmic ray measurements, as well as for the Galactic gamma ray observations. Nine years of ANTARES data are used in this work to search for a possible Galactic contribution according to this scenario. All flavour neutrino interactions are considered. No excess of events is observed and an upper limit is set on the neutrino flux of $1.1$ ($1.2$) times the prediction of the "Gamma model" assuming the primary cosmic ray spectrum cut-off at 5 (50) PeV. This limit excludes the diffuse Galactic neutrino emission as the major cause of the "spectral anomaly" between the two hemispheres measured by IceCube. Comment: 8 pages, 3 figures, 1 table
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPC; NARCISOther literature type . Article . 2017 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useRecolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAPhysical Review DArticle . 2017UPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di SalernoHAL-Inserm; Hal-DiderotArticle . 2017Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2017https://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotConference object . 2017Archivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.301.0942&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 28 citations 28 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 205visibility views 205 download downloads 635 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPC; NARCISOther literature type . Article . 2017 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useRecolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAPhysical Review DArticle . 2017UPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di SalernoHAL-Inserm; Hal-DiderotArticle . 2017Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2017https://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotConference object . 2017Archivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Article 2017 FrancePublisher:American Geophysical Union (AGU) Biari, Y.; Klingelhoefer, F.; Sahabi, M.; Funck, T.; Benabdellouahed, M.; Schnabel, M.; Reichert, C.; Gutscher, M-A; Bronner, A.; Austin, J. A.;doi: 10.1002/2017tc004596
AbstractStudy of the deep structure of conjugate passive continental margins combined with detailed plate kinematic reconstructions can provide constraints on the mechanisms of rifting and formation of initial oceanic crust. In this study the central Atlantic conjugate margins are compared based on compilation of wide‐angle seismic profiles from NW Africa Nova Scotian and U.S. passive margins. The patterns of volcanism, crustal thickness, geometry, and seismic velocities in the transition zone suggest symmetric rifting followed by asymmetric oceanic crustal accretion. Conjugate profiles in the southern central Atlantic image differences in the continental crustal thickness. While profiles on the eastern U.S. margin are characterized by thick layers of magmatic underplating, no such underplate was imaged along the African continental margin. In the north, two wide‐angle seismic profiles acquired in exactly conjugate positions show that the crustal geometry of the unthinned continental crust and the necking zone are nearly symmetric. A region including seismic velocities too high to be explained by either continental or oceanic crust is imaged along the Canadian side, corresponding on the African side to an oceanic crust with slightly elevated velocities. These might result from asymmetric spreading creating seafloor by faulting the existing lithosphere on the Canadian side and the emplacement of magmatic oceanic crust including pockets of serpentinite on the Moroccan margin. After isochron M25, a large‐scale plate reorganization might then have led to an increase in spreading velocity and the production of thin magmatic crust on both sides.
ArchiMer - Instituti... arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017tc004596&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 40 citations 40 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 10visibility views 10 download downloads 2 Powered bymore_vert ArchiMer - Instituti... arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017tc004596&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2017 FrancePublisher:Elsevier BV Funded by:ARC | Discovery Early Career Re...ARC| Discovery Early Career Researcher Award - Grant ID: DE150100326Authors: Massinissa Benabdellouahed; Frauke Klingelhoefer; Marc-André Gutscher; Marina Rabineau; +9 AuthorsMassinissa Benabdellouahed; Frauke Klingelhoefer; Marc-André Gutscher; Marina Rabineau; Y. Biari; M. Hafid; João C. Duarte; Michael Schnabel; Agnès Baltzer; Kevin Pedoja; P. Le Roy; Christian Reichert; Mohamed Sahabi;(IF 2.69; Q1); International audience; Re-examination of marine geophysical data from the continental margin of West Morocco reveals a broad zone characterized by deformation, active faults and updoming offshore the High Atlas (Morocco margin), situated next to the Tafelney Plateau. Both seismic reflection and swath-bathymetric data, acquired during Mirror marine geophysical survey in 2011, indicate recent uplift of the margin including uplift of the basement.This deformation, which we propose to name the Atlantic Atlas tectonic arch, is interpreted to result largely through uplift of the basement, which originated during the Central Atlantic rifting stage - or even during phases of Hercynian deformation. This has produced a large number of closely spaced normal and reverse faults, “piano key faults”, originating from the basement and affecting the entire sedimentary sequence, as well as the seafloor.The presence of four terraces in the Essaouira canyon system at about 3500 meters water depth and “piano key faults” and the fact that these also affect the seafloor, indicate that the Atlantic Atlas is still active north of Agadir canyon.We propose that recent uplift is causing morphogenesis of four terraces in the Essaouira canyon system. In this paper the role of both Canary plume migration and ongoing convergence between the African and Eurasian plates in the formation of the Atlantic Atlas are discussed as possibilities to explain the presence of a tectonic arch in the region. The process of reactivation of passive margins is still not well understood. The region north of Agadir canyon represents a key area to better understand this process.
Tectonophysics arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la CommunicationArticle . 2017Full-Text: https://hal.science/hal-01533093/documentHAL Descartes; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routesbronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 14visibility views 14 download downloads 4 Powered bymore_vert Tectonophysics arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la CommunicationArticle . 2017Full-Text: https://hal.science/hal-01533093/documentHAL Descartes; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2017 Netherlands, Italy, Italy, Italy, Netherlands, Netherlands, France, Netherlands, Spain, Netherlands, Italy, Italy, Italy, Spain, ItalyPublisher:Springer Science and Business Media LLC Funded by:ANR | OCEVU, NWO | Poly-Heal, a novel self-h..., ANR | Amidex +2 projectsANR| OCEVU ,NWO| Poly-Heal, a novel self-healing material for coatings and films ,ANR| Amidex ,ANR| UnivEarthS ,ANR| USPCAntares, Collaboration; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J. J.; Avgitas, T.; Baret, B.; Barrios Martí, J.; Basa, S.; Bertin, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Bruijn, R.; Brunner, J.; Busto, J.; CAPONE, Antonio; Caramete, L.; Carr, J.; CELLI, SILVIA; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Deschamps, A.; DE BONIS, Giulia; Distefano, C.; DI PALMA, IRENE; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; El Bojaddaini, I.; Elsässer, D.; Enzenhöfer, A.; Felis, I.; Folger, F.; Fusco, L. A.; Galatà, S.; Gay, P.; Giordano, V.; Glotin, H.; Grégoire, T.; Gracia Ruiz, R.; Graf, K.; Hallmann, S.; van Haren, H.; Heijboer, A. J.; Hello, Y.; Hernández Rey, J. J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C. W.; de Jong, M.; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; Lefèvre, D.; Leonora, E.; Lotze, M.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez Mora, J. A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Nezri, E.; Organokov, M.; Păvălaş, G. E.; Pellegrino, C.; PERRINA, CHIARA; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sánchez Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schüssler, F.; Sieger, C.; Spurio, M.; Stolarczyk, T.h.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, C.; Vallage, B.; Van Elewyck, V.; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J. D.; Zúñiga, J.;handle: 11245.1/0b0a21ad-fd79-4418-82db-1b1ef0fb5818 , 11567/886120 , 11573/1013333 , 11588/928282 , 11368/3003183 , 10251/87656 , 1887/58838 , 2117/107297 , 11591/464256
pmid: 28775667
pmc: PMC5512345
handle: 11245.1/0b0a21ad-fd79-4418-82db-1b1ef0fb5818 , 11567/886120 , 11573/1013333 , 11588/928282 , 11368/3003183 , 10251/87656 , 1887/58838 , 2117/107297 , 11591/464256
pmid: 28775667
pmc: PMC5512345
The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l' energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Rgion Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. A novel algorithm to reconstruct neutrino-induced particle showers within the ANTARES neutrino telescope is presented. The method achieves a median angular resolution of 6º, for shower energies below 100 TeV. Applying this algorithm to 6 years of data taken with the ANTARES detector, 8 events with reconstructed shower energies above 10 TeV are observed. This is consistent with the expectation of about 5 events from atmospheric backgrounds, but also compatible with diffuse astrophysical flux measurements by the IceCube collaboration, from which 2 4 additional events are expected. A 90% C.L. upper limit on the diffuse astrophysical neutrino flux with a value per neutrino flavour of E2·Oi 90% =4.9 cm-2· sr-1 is set, applicable to the energy range from 23 TeV to 7.8 PeV, assuming an unbroken E-2 spectrum and neutrino flavour equipartition at Earth.
NARCIS arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAEurope PubMed CentralArticle . 2017Full-Text: http://europepmc.org/articles/PMC5512345Data sources: PubMed CentralLeiden University Scholarly Publications Repository; NARCISOther literature type . Article . 2017Recolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCEuropean Physical Journal C: Particles and Fields; NARCISArticle . 2017 . Peer-reviewedLicense: CC BYArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La Sapienzahttps://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 250visibility views 250 download downloads 599 Powered bymore_vert NARCIS arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAEurope PubMed CentralArticle . 2017Full-Text: http://europepmc.org/articles/PMC5512345Data sources: PubMed CentralLeiden University Scholarly Publications Repository; NARCISOther literature type . Article . 2017Recolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCEuropean Physical Journal C: Particles and Fields; NARCISArticle . 2017 . Peer-reviewedLicense: CC BYArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La Sapienzahttps://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Article , Other literature type 2020 FrancePublisher:Elsevier BV Tarik Bouramtane; Suzanne Yameogo; Meryem Touzani; Abdessamad Tiouiouine; M’hamed El janati; Jamila Ouardi; Ilias Kacimi; Vincent Valles; Laurent Barbiero;International audience; 12 13 Abstract: 14 Several studies have revealed that the complexity in the distribution of drainage network patterns is not 15 random and controlled by major parameters, variable in space but also throughout geological time. Drainage 16 networks in the Eastern Anti-Atlas of Morocco consist of complex spatial arrangements with various types of 17 patterns, such as trellis, angular, dendritic and parallel. The objective was to distinguish, quantify and rank 18 the relationship that may exist between the different drainage networks patterns, geology and 19 geomorphology. A total of 230 basins were extracted from the ASTER-GDEM Elevation Data (USGS), which 20 were assigned 16 parameters reflecting their topography, morphometry, slope and geology. The statistical 21 treatment of the dataset (16 variables x 230 observations) was carried out through principal component 22 analysis (PCA), linear discriminant analysis (LDA) and agglomerative hierarchical clustering (AHC), in order to 23 investigate the complexity of drainage network patterns and their distribution. The PCA showed that the 24 topographical, slope and geological parameters, i.e. primarily the parameter associated with structural 25 control, best explains the variation in the type of the drainage pattern. The LDA made it possible to distinguish 26 between the four types of drainage patterns with a success rate of 90%, using 3 discriminant functions that 27 were better correlated with geological and slope parameters. LDA and AHC statistical treatments show 28 confusion between the parallel, trellis and angular patterns, on the one hand, due to similar factors 29 responsible for their formation, and on the other because of transitions phenomenon from one drainage 30 pattern to another over time or space. Such possible drainage network shifting may be explained by the 31 geological events that have occurred in the Eastern Anti Atlas from Lower Mesozoic to the Quaternary. 32 33
Journal of African E... arrow_drop_down Journal of African Earth SciencesArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.jafrearsci.2019.103707&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Journal of African E... arrow_drop_down Journal of African Earth SciencesArticle . 2020 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.jafrearsci.2019.103707&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2019 Netherlands, Spain, Italy, Netherlands, Italy, Spain, Italy, Italy, Italy, Italy, Netherlands, Netherlands, Italy, Spain, France, Netherlands, Spain, Italy, Netherlands, Italy, ItalyPublisher:Elsevier BV Funded by:EC | INPhINIT, ANR | DAEMONS, ANR | UnivEarthS +1 projectsEC| INPhINIT ,ANR| DAEMONS ,ANR| UnivEarthS ,ANR| USPCThe KM3NeT Collaboration,; Aiello, S.; Akrame, S. E.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aublin, J.; Avgitas, T.; Bagatelas, C.; Barbarino, G.; Baret, B.; Barrios-Martí, J.; Belias, A.; Berbee, E.; van den Berg, A.; Bertin, V.; Biagi, S.; Biagioni, A.; Biernoth, C.; Boumaaza, J.; Bourret, S.; Bouta, M.; Bouwhuis, M.; Bozza, C.; Brânzas, H.; Bruchner, M.; Bruijn, R.; Brunner, J.; Buis, E.; Buompane, R.; Busto, J.; Calvo, D.; Capone, A.; Celli, S.; Chabab, M.; Chau, N.; Cherubini, S.; Chiarella, V.; Chiarusi, T.; Circella, M.; Cocimano, R.; Coelho, J. A. B.; Coleiro, A.; Colomer Molla, M.; Coniglione, R.; Coyle, P.; Creusot, A.; Cuttone, G.; D'Onofrio, A.; Dallier, R.; De Sio, C.; Di Palma, I.; Díaz, A. F.; Diego-Tortosa, D.; Distefano, C.; Domi, A.; Donà, R.; Donzaud, C.; Dornic, D.; Dörr, M.; Durocher, M.; Eberl, T.; van Eijk, D.; El Bojaddaini, I.; Eljarrari, H.; Elsaesser, D.; Enzenhöfer, A.; Fermani, P.; Ferrara, G.; Filipovic, M. D.; Fusco, L. A.; Gal, T.; Garcia, A.; Garufi, F.; Gialanella, L.; Giorgio, E.; Giuliante, A.; Gozzini, S. R.; Gracia, R.; Graf, K.; Grasso, D.; Grégoire, T.; Grella, G.; Hallmann, S.; Hamdaoui, H.; van Haren, H.; Heid, T.; Heijboer, A.; Hekalo, A.; Hernández-Rey, J. J.; Hofestädt, J.; Illuminati, G.; James, C. W.; Jongen, M.; de Jong, M.; de Jong, P.; Kadler, M.; Kalaczynski, P.; Kalekin, O.; Katz, U. F.; Khan Chowdhury, N. R.; Kiessling, D.; Koffeman, E. N.; Kooijman, P.; Kouchner, A.; Kreter, M.; Kulikovskiy, V.; Kunhikannan-Kannichankandy, M.; Lahmann, R.; Larosa, G.; Le Breton, R.; Leone, F.; Leonora, E.; Levi, G.; Lincetto, M.; Lonardo, A.; Longhitano, F.; Lopez Coto, D.; Lotze, M.; Maderer, L.; Maggi, G.; Manczak, J.; Mannheim, K.; Margiotta, A.; Marinelli, A.; Markou, C.; Martin, L.; Martínez-Mora, J. A.; Martini, A.; Marzaioli, F.; Mele, R.; Melis, K. W.; Migliozzi, P.; Migneco, E.; Mijakowski, P.; Miranda, L. S.; Mollo, C. M.; Morganti, M.; Moser, M.; Moussa, A.; Muller, R.; Musumeci, M.; Nauta, L.; Navas, S.; Nicolau, C. A.; Nielsen, C.; Ó Fearraigh, B.; Organokov, M.; Orlando, A.; Ottonello, S.; Panagopoulos, V.; Papalashvili, G.; Papaleo, R.; Păvălaş, G. E.; Pellegrino, C.; Perrin-Terrin, M.; Piattelli, P.; Pikounis, K.; Pisanti, O.; Poirè, C.; Polydefki, G.; Popa, V.; Post, M.; Pradier, T.; Pühlhofer, G.; Pulvirenti, S.; Quinn, L.; Raffaelli, F.; Randazzo, N.; Razzaque, S.; Real, D.; Resvanis, L.; Reubelt, J.; Riccobene, G.; Richer, M.; Rigalleau, L.; Rovelli, A.; Saffer, M.; Salvadori, I.; Samtleben, D. F. E.; Sánchez Losa, A.; Sanguineti, M.; Santangelo, A.; Santonocito, D.; Sapienza, P.; Schumann, J.; Sciacca, V.; Seneca, J.; Sgura, I.; Shanidze, R.; Sharma, A.; Simeone, F.; Sinopoulou, A.; Spisso, B.; Spurio, M.; Stavropoulos, D.; Trovato, A.;KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the detection of high-energy neutrinos of cosmic origin. Thanks to its geographical location on the Northern hemisphere, KM3NeT/ARCA can observe upgoing neutrinos from most of the Galactic Plane, including the Galactic Centre. Given its effective area and excellent pointing resolution, KM3NeT/ARCA will measure or significantly constrain the neutrino flux from potential astrophysical neutrino sources. At the same time, it will test flux predictions based on gamma-ray measurements and the assumption that the gamma-ray flux is of hadronic origin. Assuming this scenario, discovery potentials and sensitivities for a selected list of Galactic sources and to generic point sources with an $E^{-2}$ spectrum are presented. These spectra are assumed to be time independent. The results indicate that an observation with $3\sigma$ significance is possible in about six years of operation for the most intense sources, such as Supernovae Remnants RX\,J1713.7-3946 and Vela Jr. If no signal will be found during this time, the fraction of the gamma-ray flux coming from hadronic processes can be constrained to be below 50\% for these two objects. Comment: 32 pages, 9 figures, submitted to Astroparticle Physics
IRIS - Università de... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; NARCISArticle . 2019NARCISArticle . 2019Full-Text: https://pure.uva.nl/ws/files/64663217/Sensitivity_of_the_KM3NeT_ARCA_neutrino_telescope.pdfData sources: NARCISRecolector de Ciencia Abierta, RECOLECTAArticle . 2019License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; RiuNet; Recolector de Ciencia Abierta, RECOLECTA; NARCISOther literature type . Article . 2019 . Peer-reviewedLicense: Elsevier TDMArchivio della ricerca- Università di Roma La SapienzaArticle . 2019Data sources: Archivio della ricerca- Università di Roma La SapienzaIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019Recolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2020 . 2019UPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCLeiden University Scholarly Publications RepositoryOther literature type . 2019License: CC BY NC NDData sources: Leiden University Scholarly Publications RepositoryArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernohttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 70 citations 70 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 246visibility views 246 download downloads 1,085 Powered bymore_vert IRIS - Università de... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; NARCISArticle . 2019NARCISArticle . 2019Full-Text: https://pure.uva.nl/ws/files/64663217/Sensitivity_of_the_KM3NeT_ARCA_neutrino_telescope.pdfData sources: NARCISRecolector de Ciencia Abierta, RECOLECTAArticle . 2019License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAAstroparticle Physics; RiuNet; Recolector de Ciencia Abierta, RECOLECTA; NARCISOther literature type . Article . 2019 . Peer-reviewedLicense: Elsevier TDMArchivio della ricerca- Università di Roma La SapienzaArticle . 2019Data sources: Archivio della ricerca- Università di Roma La SapienzaIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019Recolector de Ciencia Abierta, RECOLECTA; Repositorio Institucional Universidad de GranadaOther literature type . Article . 2020 . 2019UPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2019 . Peer-reviewedLicense: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCLeiden University Scholarly Publications RepositoryOther literature type . 2019License: CC BY NC NDData sources: Leiden University Scholarly Publications RepositoryArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernohttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: DataciteArchivio della Ricerca - Università di SalernoArticle . 2019Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2019 FrancePublisher:Wiley Authors: Houda El Kerni; Hasnaa Chennaoui Aoudjehane; David Baratoux; Mohammed Aoudjehane; +14 AuthorsHouda El Kerni; Hasnaa Chennaoui Aoudjehane; David Baratoux; Mohammed Aoudjehane; André Charrière; Hassan Ibouh; Pierre Rochette; Yoann Quesnel; Minoru Uehara; Thomas Kenkmann; G. Wulf; Michael H. Poelchau; van Binh Nguyen; Hassan Aboulahris; Hassan Makhoukhi; Georges Aumaître; Didier Bourlès; Karim Keddadouche;doi: 10.1111/maps.13347
AbstractSince the discovery of shatter cones (SCs) near the village of Agoudal (Morocco, Central High Atlas Mountains) in 2013, the absence of one or several associated circular structures led to speculation about the age of the impact event, the number, and the size of the impact crater or craters. Additional constraints on the crater size, age, and erosion rates are obtained here from geological, structural, and geophysical mapping and from cosmogenic nuclide data. Our geological maps of the Agoudal impact site at the scales of 1:30,000 (6 km2) and 1:15,000 (2.25 km2) include all known occurrences of SCs in target rocks, breccias, and vertical to overturned strata. Considering that strata surrounding the impact site are subhorizontal, we argue that disturbed strata are related to the impact event. Three types of breccias have been observed. Two of them (br1‐2 and br2) could be produced by erosion–sedimentation–consolidation processes, with no evidence for impact breccias, while breccia (br1) might be impact related. The most probable center of the structure is estimated at 31°59′13.73ʺN, 5°30′55.14ʺW using the concentric deviation method applied to the orientation of strata over the disturbed area. Despite the absence of a morphological expression, the ground magnetic and electromagnetic surveys reveal anomalies spatially associated with disturbed strata and SC occurrences. The geophysical data, the structural observations, and the area of occurrence of SCs in target rocks are all consistent with an original size of 1.4–4.2 km in diameter. Cosmogenic nuclide data (36Cl) constrain the local erosion rates between 220 ± 22 m Ma−1 and 430 ± 43 m Ma−1. These erosion rates may remove the topographic expression of such a crater and its ejecta in a time period of about 0.3–1.9 Ma. This age is older than the Agoudal iron meteorite age (105 ± 40 kyr). This new age constraint excludes the possibility of a genetic relationship between the Agoudal iron meteorite fall and the formation of the Agoudal impact site. A chronolgy chart including the Atlas orogeny, the alternation of sedimentation and erosion periods, and the meteoritic impacts is presented based on all obtained and combined data.
Horizon / Pleins tex... arrow_drop_down Meteoritics and Planetary ScienceArticle . 2019 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu2 citations 2 popularity Average influence Average impulse Average Powered by BIP!more_vert Horizon / Pleins tex... arrow_drop_down Meteoritics and Planetary ScienceArticle . 2019 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2019 Netherlands, France, Italy, Italy, Netherlands, Germany, Netherlands, Italy, Italy, Netherlands, Belgium, Czech Republic, Brazil, Belgium, Italy, Italy, Italy, Netherlands, Italy, ItalyPublisher:Frontiers Media SA Funded by:ANR | SUPER, NSF | Pierre Auger Project, EC | EPLANETANR| SUPER ,NSF| Pierre Auger Project ,EC| EPLANETA. Aab; P. Abreu; M. Aglietta; I. F. M. Albuquerque; J. M. Albury; I. Allekotte; A. Almela; J. Alvarez Castillo; J. Alvarez-Muñiz; G. A. Anastasi; L. Anchordoqui; B. Andrada; S. Andringa; C. Aramo; H. Asorey; P. Assis; G. Avila; A. M. Badescu; A. Bakalova; A. Balaceanu; F. Barbato; R. J. Barreira Luz; S. Baur; K. H. Becker; J. A. Bellido; C. Berat; M. E. Bertaina; X. Bertou; P. L. Biermannb; J. Biteau; S. G. Blaess; A. Blanco; J. Blazek; C. Bleve; M. Boháˇcová; D. Boncioli; C. Bonifazi; N. Borodai; A. M. Botti; J. Bracke; T. Bretz; A. Bridgeman; F. L. Briechle; P. Buchholz; A. Bueno; S. Buitink; M. Buscemi; K. S. Caballero-Mora; L. Caccianiga; L. Calcagni; A. Cancio; F. Canfora; J. M. Carceller; R. Caruso; A. Castellina; F. Catalani; G. Cataldi; L. Cazon; M. Cerda; J. A. Chinellato; J. Chudoba; L. Chytka; R. W. Clay; A. C. Cobos Cerutti; R. Colalillo; A. Coleman; M. R. Coluccia; R. Conceição; A. Condorelli; G. Consolati; F. Contreras; F. Convenga; M. J. Cooper; S. Coutu; C. E. Covault; B. Daniel; S. Dasso; K. Daumiller; B. R. Dawson; J. A. Day; R. M. de Almeida; S. J. de Jong; G. De Mauro; J. R. T. de Mello Neto; I. De Mitri; J. de Oliveira; F. O. de Oliveira Salles; V. de Souza; J. Debatin; M. del Río; O. Deligny; N. Dhital; M. L. Díaz Castro; F. Diogo; C. Dobrigkeit; J. C. D’Olivo; Q. Dorosti; R. C. dos Anjos; M. T. Dova; A. Dundovic; J. Ebr; R. Engel; M. Erdmann; C. O. Escobarc; A. Etchegoyen; H. Falcke; J. Farmer; G. Farrar; A. C. Fauth; N. Fazzinic; F. Feldbusch; F. Fenu; L. P. Ferreyro; J. M. Figueira; A. Filipˇciˇc; M. M. Freire; T. Fujii; f; A. Fuster; B. García; H. Gemmeke; A. Gherghel-Lascu; P. L. Ghia; U. Giaccari; M. Giammarchi; M. Giller; D. Głas; J. Glombitza; F. Gobbi; G. Golup; M. Gómez Berisso; P. F. Gómez Vitale; J. P. Gongora; N. González; I. Goos; D. Góra; A. Gorgi; M. Gottowik; T. D. Grubb; F. Guarino; G. P. Guedes; E. Guido; R. Halliday; M. R. Hampel; P. Hansen; D. Harari; T. A. Harrison; V. M. Harvey; A. Haungs; T. Hebbeker; D. Heck; P. Heimann; G. C. Hill; C. Hojvatc; E. M. Holt; P. Homola; J. R. Hörandel; P. Horvath; M. Hrabovský; T. Huege; J. Hulsman; A. Insolia; P. G. Isar; I. Jandt; J. A. Johnsen; M. Josebachuili; J. Jurysek; A. Kääpä; K. H. Kampert; B. Keilhauer; N. Kemmerich; J. Kemp; H. O. Klages; M. Kleifges; J. Kleinfeller; R. Krause; D. Kuempel; G. Kukec Mezek; A. Kuotb Awad; B. L. Lago; D. LaHurd; R. G. Lang; R. Legumina; M. A. Leigui de Oliveira; V. Lenok; A. Letessier-Selvon; I. Lhenry-Yvon; O. C. Lippmann; D. Lo Presti; L. Lopes; R. López; A. López Casado; R. Lorek; Q. Luce; A. Lucero; M. Malacari; G. Mancarella; D. Mandat; B. C. Manning; P. Mantschc; L. Miramonti; L. Valore; F. Zuccarello;An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results are reviewed, such as stringent upper bounds that were placed to a flux of diffuse cosmogenic neutrinos and photons, bounds placed on neutrinos emitted from compact binary mergers that were detected by LIGO and Virgo during their first and second observing runs, as well as searches for high energy photons and neutrons from the Galactic center that constrain the properties of the putative Galactic PeVatron, observed by the H.E.S.S. collaboration. The observation of directional correlations between ultra-high energy cosmic rays and either high energy astrophysical neutrinos or specific source populations, weighted by their electromagnetic radiation, are also discussed. They constitute additional multi-messenger approaches aimed at identifying the sources of high energy cosmic rays. info:eu-repo/semantics/published SCOPUS: re.j
NARCIS; Radboud Repo... arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019Archivio Istituzionale della Ricerca- Università del Salento; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; Frontiers in Astronomy and Space Sciences; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoReview . Other literature type . Article . 2019 . Peer-reviewedLicense: CC BYData sources: Archivio Istituzionale della Ricerca- Università del Salento; University of Groningen Research Portal; Crossref; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; NARCIS; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaPublikationsserver der RWTH Aachen UniversityArticle . 2019Data sources: Publikationsserver der RWTH Aachen UniversityVrije Universiteit Brussel Research PortalOther literature type . 2019Data sources: Vrije Universiteit Brussel Research PortalFrontiers in Astronomy and Space SciencesArticle . 2019Data sources: METIS Research Information SystemOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 18 citations 18 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!more_vert NARCIS; Radboud Repo... arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019Archivio Istituzionale della Ricerca- Università del Salento; Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) - Universidade de São Paulo (USP); Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; Frontiers in Astronomy and Space Sciences; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoReview . Other literature type . Article . 2019 . Peer-reviewedLicense: CC BYData sources: Archivio Istituzionale della Ricerca- Università del Salento; University of Groningen Research Portal; Crossref; LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas; NARCIS; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; RE.PUBLIC@POLIMI Research Publications at Politecnico di MilanoIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesRepository of the Czech Academy of SciencesArticle . 2019Data sources: Repository of the Czech Academy of SciencesIRIS - Università degli Studi di CataniaArticle . 2019Data sources: IRIS - Università degli Studi di CataniaPublikationsserver der RWTH Aachen UniversityArticle . 2019Data sources: Publikationsserver der RWTH Aachen UniversityVrije Universiteit Brussel Research PortalOther literature type . 2019Data sources: Vrije Universiteit Brussel Research PortalFrontiers in Astronomy and Space SciencesArticle . 2019Data sources: METIS Research Information SystemOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3389/fspas.2019.00024&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2018 Spain, Spain, FrancePublisher:Elsevier BV Funded by:EC | EUROFLEETSEC| EUROFLEETSLafosse, M.; Gorini, C. (Christian); Le Roy, P.; Alonso, B. (Belén); D'Acremont, E. (Elia); Ercilla, G. (Gemma); Rabineau, M. (Marina); Vázquez, J.T. (Juan Tomás); Rabaute, A.; Ammar, A.;handle: 10261/172851 , 10508/15121
In active basins, tectonics can segment the continental shelf and control its stratigraphic architecture and physiography. Segmentation can explain the local evolution and morphology of the continental shelf because of sea-level variations, local tectonic segmentation and hydrodynamic processes. Here we investigate the tectonically active Morocco continental margin (southern Alboran Sea) using high-resolution seismic profiles and multibeam bathymetric data. The active faults bounding the transtensive Nekor basin triggered the segmentation of the shelf into three sectors showing different subsidence rates: a western sector corresponding to an extensive fault relay, a central sector corresponding to the subsiding Al-Hoceima Bay and an eastern sector corresponding to the footwall of the Trougout senestral normal fault. Results show that the staircase morphology of the shelf corresponds to successive submarine terraces at the shelf edge (ST1), mid-shelf (ST2) and inner-shelf (ST3) around −110 m,-80 m, and −40 to −20 m deep, respectively. The terraces correspond to the top of prograding wedges seaward and are erosive landward. They are correlated with stillstand from the Last Glacial Maximum to the Holocene highstand. Above the terraces, sub-aqueous dune fields are interpreted as degraded and deposited during the post-glacial transgression. In the central sector, typical delta front seafloor undulations on the shelf and crescent shaped bedforms at the head of marine incisions on the upper slope denote a fluvial influence during the Holocene. Seismic stratigraphy analysis revealed the preservation of six seismic units bounded by polygenic regional unconformities (S1, S2, S3, S4 and S5). Based on comparison with other Mediterranean margins, S1 to S5 are attributed to 4th order maximum regressive surface. We discuss the local preservation of the system tracts as a function of the vertical motion and the physiography of this tectonically active domain. This study provides useful clues for future local paleo-seismic analysis and to advance our understanding of sedimentary processes in active areas This work was funded by the French program Actions Marges, the EUROFLEETS program (FP7/2007-2013; n°228344), project FICTS-2011-03-01. Seismic reflection data were processed using the Seismic UNIX SU and Geovecteur software. [...]. This work also benefited from a State Grant from the French Agence Nationale de la Recherche (ANR) in the Program « Investissements d'avenir » reference ANR-10-LABX-19-01, Labex Mer and from the Fauces Project (Ref CTM2015-65461-C2-R; MINCIU/FEDER) financed by "Ministerio de Economía y Competitividad y al Fondo Europeo de Desarrollo Regional" (FEDER) 20 pages, 14 figures, 1 table Peer Reviewed
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2018Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTA; Marine and Petroleum GeologyArticle . 2018 . Peer-reviewedArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMarine and Petroleum GeologyArticle . 2018 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2018add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.marpetgeo.2018.07.022&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 19visibility views 19 download downloads 67 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2018Data sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTA; Marine and Petroleum GeologyArticle . 2018 . Peer-reviewedArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMarine and Petroleum GeologyArticle . 2018 . Peer-reviewedLicense: Elsevier TDMData sources: CrossrefHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2018add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.marpetgeo.2018.07.022&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Review , Article 2017 France, BelgiumPublisher:Cambridge University Press (CUP) Benammi , Mouloud; Adnet , Sylvain; Marivaux , Laurent; Yans , Johan; Noiret , Corentin; Tabuce , Rodolphe; SURAULT , JÉRÔME; EL KATI , IMAD; Enault , Sebastien; BAIDDER , LAHSSEN; Saddiqi , Omar; Benammi , Mohamed;AbstractNew Palaeogene vertebrate localities were recently reported in the southern Dakhla area (southwestern Morocco). The Eocene sediment strata crops out on cliffs along the Atlantic Ocean coast. Vertebrate remains come from five conglomeratic sandstone beds and are principally represented by isolated teeth belonging to micromammals, selachians and bony fishes, a proboscidean assigned to ?Numidotheriumsp. and many remains of archaeocete whales (Basilosauridae). From fieldwork five lithostratigraphic sections were described, essentially based on the lithological characteristic of sediments. Despite the lateral variations of facies, correlations between these five sections were possible on the basis of fossil-bearing beds (A1, B1, B2, C1 and C2) and five lithological units were identified. The lower part of the section consists of rhythmically bedded, chert-rich marine siltstones and marls with thin black phosphorite with organic matter at the base. The overlying units include coarse-grained to microconglomeratic sandstones interbedded with silts, indicating deposition in a shallow-marine environment with fluvial influence. The natural remanence magnetization of a total of 50 samples was measured; the intensity of most of the samples is too weak however, before or after the first step of demagnetization. The palaeomagnetic data from the samples are very unstable, except for eight from three similar sandstone levels which show a normal polarity. Matched with biostratigraphic data on rodents, primates, the selachian, sirenian and cetacean faunas, the new carbon isotope chemostratigraphy on organics (1) refines the age of the uppermost C2 fossil-bearing bed to earliest Oligocene time and (2) confirms the Priabonian age of the B1 to C1 levels.
Geological Magazine arrow_drop_down Geological MagazineArticle . 2017 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefHyper Article en Ligne; Mémoires en Sciences de l'Information et de la Communication; Hal-DiderotOther literature type . Conference object . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/s0016756817000851&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 8 citations 8 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Geological Magazine arrow_drop_down Geological MagazineArticle . 2017 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefHyper Article en Ligne; Mémoires en Sciences de l'Information et de la Communication; Hal-DiderotOther literature type . Conference object . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/s0016756817000851&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Other literature type , Preprint 2017 Italy, Spain, Netherlands, Italy, Italy, Netherlands, Italy, Italy, Netherlands, Italy, Italy, France, Netherlands, Italy, SpainPublisher:Sissa Medialab Funded by:ANR | OCEVU, ANR | USPCANR| OCEVU ,ANR| USPCAlbert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J. -.J.; Avgitas, T.; Baret, B.; Barrios-MartÃ, J.; Basa, S.; Belhorma, B.; Bertin, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Bruijn, R.; Brunner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Cherkaoui El Moursli, R.; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; DÃaz, A. F.; Deschamps, A.; De Bonis, G.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; El Bojaddaini, I.; El Khayati, N.; Elsässer, D.; Enzenhöfer, A.; Ettahiri, A.; Fassi, F.; Felis, I.; Fusco, L. A.; Galatà , S.; Gay, P.; Giordano, V.; Glotin, H.; Grégoire, T.; Gracia Ruiz, R.; Graf, K.; Hallmann, S.; Van Haren, H.; Heijboer, A. J.; Hello, Y.; Hernández-Rey, J. J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C. W.; De Jong, M.; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; LefÃvre, D.; Leonora, E.; Lotze, M.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; MartÃnez-Mora, J. A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Navas, S.; Nezri, E.; Organokov, M.; PÇŽvÇŽlaÅŸ, G. E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sánchez-Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; SchÃ1⁄4ssler, F.; Sieger, C.; Spurio, M.; Stolarczyk, T.h.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, C.; Vallage, B.; Van Elewyck, V.; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J. D.; ZÃoñiga, J.; Gaggero, D.; Grasso, D.;The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization of this flux will shed light on Galactic accelerator features, gas distribution morphology and Galactic cosmic ray transport. The central Galactic plane can be the site of an enhanced neutrino production, thus leading to anisotropies in the extraterrestrial neutrino signal as measured by the IceCube Collaboration. The ANTARES neutrino telescope, located in the Mediterranean Sea, offers a favourable view on this part of the sky, thereby allowing for a contribution to the determination of this flux. The expected diffuse Galactic neutrino emission can be obtained linking a model of generation and propagation of cosmic rays with the morphology of the gas distribution in the Milky Way. In this paper, the so-called "Gamma model" introduced recently to explain the high-energy gamma ray diffuse Galactic emission, is assumed as reference. The neutrino flux predicted by the "Gamma model" depends of the assumed primary cosmic ray spectrum cut-off. Considering a radially-dependent diffusion coefficient, this proposed scenario is able to account for the local cosmic ray measurements, as well as for the Galactic gamma ray observations. Nine years of ANTARES data are used in this work to search for a possible Galactic contribution according to this scenario. All flavour neutrino interactions are considered. No excess of events is observed and an upper limit is set on the neutrino flux of $1.1$ ($1.2$) times the prediction of the "Gamma model" assuming the primary cosmic ray spectrum cut-off at 5 (50) PeV. This limit excludes the diffuse Galactic neutrino emission as the major cause of the "spectral anomaly" between the two hemispheres measured by IceCube. Comment: 8 pages, 3 figures, 1 table
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPC; NARCISOther literature type . Article . 2017 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useRecolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAPhysical Review DArticle . 2017UPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di SalernoHAL-Inserm; Hal-DiderotArticle . 2017Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2017https://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotConference object . 2017Archivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 28 citations 28 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 205visibility views 205 download downloads 635 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPC; NARCISOther literature type . Article . 2017 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useRecolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAPhysical Review DArticle . 2017UPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La SapienzaArchivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di SalernoHAL-Inserm; Hal-DiderotArticle . 2017Mémoires en Sciences de l'Information et de la Communication; HAL-CEAConference object . 2017https://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotConference object . 2017Archivio della Ricerca - Università di SalernoArticle . 2017Data sources: Archivio della Ricerca - Università di Salernoadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Article 2017 FrancePublisher:American Geophysical Union (AGU) Biari, Y.; Klingelhoefer, F.; Sahabi, M.; Funck, T.; Benabdellouahed, M.; Schnabel, M.; Reichert, C.; Gutscher, M-A; Bronner, A.; Austin, J. A.;doi: 10.1002/2017tc004596
AbstractStudy of the deep structure of conjugate passive continental margins combined with detailed plate kinematic reconstructions can provide constraints on the mechanisms of rifting and formation of initial oceanic crust. In this study the central Atlantic conjugate margins are compared based on compilation of wide‐angle seismic profiles from NW Africa Nova Scotian and U.S. passive margins. The patterns of volcanism, crustal thickness, geometry, and seismic velocities in the transition zone suggest symmetric rifting followed by asymmetric oceanic crustal accretion. Conjugate profiles in the southern central Atlantic image differences in the continental crustal thickness. While profiles on the eastern U.S. margin are characterized by thick layers of magmatic underplating, no such underplate was imaged along the African continental margin. In the north, two wide‐angle seismic profiles acquired in exactly conjugate positions show that the crustal geometry of the unthinned continental crust and the necking zone are nearly symmetric. A region including seismic velocities too high to be explained by either continental or oceanic crust is imaged along the Canadian side, corresponding on the African side to an oceanic crust with slightly elevated velocities. These might result from asymmetric spreading creating seafloor by faulting the existing lithosphere on the Canadian side and the emplacement of magmatic oceanic crust including pockets of serpentinite on the Moroccan margin. After isochron M25, a large‐scale plate reorganization might then have led to an increase in spreading velocity and the production of thin magmatic crust on both sides.
ArchiMer - Instituti... arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017tc004596&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 40 citations 40 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 10visibility views 10 download downloads 2 Powered bymore_vert ArchiMer - Instituti... arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerHAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/2017tc004596&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2017 FrancePublisher:Elsevier BV Funded by:ARC | Discovery Early Career Re...ARC| Discovery Early Career Researcher Award - Grant ID: DE150100326Authors: Massinissa Benabdellouahed; Frauke Klingelhoefer; Marc-André Gutscher; Marina Rabineau; +9 AuthorsMassinissa Benabdellouahed; Frauke Klingelhoefer; Marc-André Gutscher; Marina Rabineau; Y. Biari; M. Hafid; João C. Duarte; Michael Schnabel; Agnès Baltzer; Kevin Pedoja; P. Le Roy; Christian Reichert; Mohamed Sahabi;(IF 2.69; Q1); International audience; Re-examination of marine geophysical data from the continental margin of West Morocco reveals a broad zone characterized by deformation, active faults and updoming offshore the High Atlas (Morocco margin), situated next to the Tafelney Plateau. Both seismic reflection and swath-bathymetric data, acquired during Mirror marine geophysical survey in 2011, indicate recent uplift of the margin including uplift of the basement.This deformation, which we propose to name the Atlantic Atlas tectonic arch, is interpreted to result largely through uplift of the basement, which originated during the Central Atlantic rifting stage - or even during phases of Hercynian deformation. This has produced a large number of closely spaced normal and reverse faults, “piano key faults”, originating from the basement and affecting the entire sedimentary sequence, as well as the seafloor.The presence of four terraces in the Essaouira canyon system at about 3500 meters water depth and “piano key faults” and the fact that these also affect the seafloor, indicate that the Atlantic Atlas is still active north of Agadir canyon.We propose that recent uplift is causing morphogenesis of four terraces in the Essaouira canyon system. In this paper the role of both Canary plume migration and ongoing convergence between the African and Eurasian plates in the formation of the Atlantic Atlas are discussed as possibilities to explain the presence of a tectonic arch in the region. The process of reactivation of passive margins is still not well understood. The region north of Agadir canyon represents a key area to better understand this process.
Tectonophysics arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la CommunicationArticle . 2017Full-Text: https://hal.science/hal-01533093/documentHAL Descartes; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.tecto.2017.03.024&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 14visibility views 14 download downloads 4 Powered bymore_vert Tectonophysics arrow_drop_down ArchiMer - Institutional Archive of IfremerOther literature type . 2017Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la CommunicationArticle . 2017Full-Text: https://hal.science/hal-01533093/documentHAL Descartes; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2017add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.tecto.2017.03.024&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2017 Netherlands, Italy, Italy, Italy, Netherlands, Netherlands, France, Netherlands, Spain, Netherlands, Italy, Italy, Italy, Spain, ItalyPublisher:Springer Science and Business Media LLC Funded by:ANR | OCEVU, NWO | Poly-Heal, a novel self-h..., ANR | Amidex +2 projectsANR| OCEVU ,NWO| Poly-Heal, a novel self-healing material for coatings and films ,ANR| Amidex ,ANR| UnivEarthS ,ANR| USPCAntares, Collaboration; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J. J.; Avgitas, T.; Baret, B.; Barrios Martí, J.; Basa, S.; Bertin, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Bruijn, R.; Brunner, J.; Busto, J.; CAPONE, Antonio; Caramete, L.; Carr, J.; CELLI, SILVIA; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Deschamps, A.; DE BONIS, Giulia; Distefano, C.; DI PALMA, IRENE; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; El Bojaddaini, I.; Elsässer, D.; Enzenhöfer, A.; Felis, I.; Folger, F.; Fusco, L. A.; Galatà, S.; Gay, P.; Giordano, V.; Glotin, H.; Grégoire, T.; Gracia Ruiz, R.; Graf, K.; Hallmann, S.; van Haren, H.; Heijboer, A. J.; Hello, Y.; Hernández Rey, J. J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C. W.; de Jong, M.; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; Lefèvre, D.; Leonora, E.; Lotze, M.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez Mora, J. A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Nezri, E.; Organokov, M.; Păvălaş, G. E.; Pellegrino, C.; PERRINA, CHIARA; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sánchez Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schüssler, F.; Sieger, C.; Spurio, M.; Stolarczyk, T.h.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, C.; Vallage, B.; Van Elewyck, V.; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J. D.; Zúñiga, J.;handle: 11245.1/0b0a21ad-fd79-4418-82db-1b1ef0fb5818 , 11567/886120 , 11573/1013333 , 11588/928282 , 11368/3003183 , 10251/87656 , 1887/58838 , 2117/107297 , 11591/464256
pmid: 28775667
pmc: PMC5512345
handle: 11245.1/0b0a21ad-fd79-4418-82db-1b1ef0fb5818 , 11567/886120 , 11573/1013333 , 11588/928282 , 11368/3003183 , 10251/87656 , 1887/58838 , 2117/107297 , 11591/464256
pmid: 28775667
pmc: PMC5512345
The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l' energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Rgion Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. A novel algorithm to reconstruct neutrino-induced particle showers within the ANTARES neutrino telescope is presented. The method achieves a median angular resolution of 6º, for shower energies below 100 TeV. Applying this algorithm to 6 years of data taken with the ANTARES detector, 8 events with reconstructed shower energies above 10 TeV are observed. This is consistent with the expectation of about 5 events from atmospheric backgrounds, but also compatible with diffuse astrophysical flux measurements by the IceCube collaboration, from which 2 4 additional events are expected. A 90% C.L. upper limit on the diffuse astrophysical neutrino flux with a value per neutrino flavour of E2·Oi 90% =4.9 cm-2· sr-1 is set, applicable to the energy range from 23 TeV to 7.8 PeV, assuming an unbroken E-2 spectrum and neutrino flavour equipartition at Earth.
NARCIS arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAEurope PubMed CentralArticle . 2017Full-Text: http://europepmc.org/articles/PMC5512345Data sources: PubMed CentralLeiden University Scholarly Publications Repository; NARCISOther literature type . Article . 2017Recolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCEuropean Physical Journal C: Particles and Fields; NARCISArticle . 2017 . Peer-reviewedLicense: CC BYArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La Sapienzahttps://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 250visibility views 250 download downloads 599 Powered bymore_vert NARCIS arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAOther literature type . Article . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTAEurope PubMed CentralArticle . 2017Full-Text: http://europepmc.org/articles/PMC5512345Data sources: PubMed CentralLeiden University Scholarly Publications Repository; NARCISOther literature type . Article . 2017Recolector de Ciencia Abierta, RECOLECTAArticle . 2017Data sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCOther literature type . Article . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCEuropean Physical Journal C: Particles and Fields; NARCISArticle . 2017 . Peer-reviewedLicense: CC BYArchivio della ricerca- Università di Roma La SapienzaArticle . 2017Data sources: Archivio della ricerca- Università di Roma La Sapienzahttps://doi.org/10.48550/arxiv...Article . 2017License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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