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Wyszukujesz frazę "Moya, P." wg kryterium: Autor


Tytuł:
Antifungal activity of Trichoderma VOCs against Pyrenophora teres, the causal agent of barley net blotch
Autorzy:
Moya, P.
Girotti, J.R.
Toledo, A.V.
Sisterna, M.N.
Tematy:
biological control
biopesticide
fungi
gas chromatography
mass spectrometry
pathogen
Pyrenophora teres
Trichoderma
antifungal activity
volatile organic compound
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Czytelnia Czasopism PAN
Powiązania:
https://bibliotekanauki.pl/articles/65288.pdf  Link otwiera się w nowym oknie
Opis:
Many species of Trichoderma produce secondary metabolites such as volatile organic compounds (VOCs) that reduce plant diseases and promote their growth. In this work we evaluated the antagonistic effects of VOCs released by eight strains of two Trichoderma species against Pyrenophora teres Drechsler, the causal agent of barley net blotch. Antagonism was estimated based on the percentage of mycelial growth inhibition according to the confronted cultures method. VOCs extraction and identification were performed by gas chromatography and mass spectrometry, through different methodologies for VOCs emitted by antagonists and pathogens alone or when confronted. VOCs produced by all Trichoderma strains inhibited mycelial growth of the pathogen in a range of 3 to 32%, showing weak and unpigmented mycelia with vacuolization. In addition, P. teres stimulated the release of VOCs by both Trichoderma species. The major groups of VOCs detected were sesquiterpenes, followed by diterpenes, terpenoids and eight-carbon compounds. This is the first report about characterization of volatiles emitted by Trichoderma in the presence of P. teres.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Grain discoloration in different genotypes of durum wheat (Triticum durum L.) in Argentina: associated mycobiota and peroxidase activity
Autorzy:
Cipollone, M.J.
Moya, P.
Martinez, I.
Saparrat, M.
Sisterna, M.
Tematy:
durum wheat
grain discoloration
mycobiota
peroxidase activity
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Czytelnia Czasopism PAN
Powiązania:
https://bibliotekanauki.pl/articles/2084746.pdf  Link otwiera się w nowym oknie
Opis:
Wheat grain discoloration, a worldwide disease that lowers grain quality and decreases grain yield, does not have a single etiology. It has been proposed that it is a consequence of an abiotic mechanism, a response to environmental conditions or enzymatic activity. It has also been suggest that it is a biotic mechanism, a fungal infection principally by Alternaria spp. and Bipolaris sorokiniana. The present work was carried out to analyze the possible etiology of this disease in nine durum wheat genotypes from two localities of southern Buenos Aires province (Argentina) on two sowing dates. Incidence (percentage of grain discoloration) was recorded and mycobiota associated with this pathology was registered following ISTA rules. Peroxidase activity in an extract obtained from grains belonging to genotypes of the locality that showed the highest incidence was measured. The incidence among genotypes, localities and sowing dates varied, although the genotypes with the higher and lower values of incidence were the same for all the variables tested. The fungus Alternaria spp. was isolated the most frequently followed by Fusarium spp., while Bipolaris sorokiniana was found the least frequently. Peroxidase activity showed that all the treatments had similar levels of enzymatic activity, but there was no clear differentiation between controls either between genotypes with the lowest or the highest incidence values. This suggests that peroxidase activity did not have a clear relationship with grain discoloration. In this research, it is presumed that fungal infection is the main cause of this disease.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Mechanical properties of some granular agricultural materials used in silo design
Autorzy:
Moya, M.
Aguado, P.J.
Ayuga, F.
Wydawca:
Polska Akademia Nauk. Instytut Agrofizyki PAN
Powiązania:
https://bibliotekanauki.pl/articles/26147.pdf  Link otwiera się w nowym oknie
Opis:
The aim of this research was to provide values for different material properties considered in either traditional or more recent numerical silo design methods. Different samples of granular agricultural materials commonly stored in silos were tested. Common geotechnical devices have been used in order to make the replications easier. Based on these experiments it was determined that the different material properties were not affected by the test velocity, except in the case of Poisson ratio. From a practical point of view, the test velocity correlates well with the sliding velocity of grain during discharge. The values obtained for material properties considered in traditional silo design methods were similar to those reported by other authors. No significant differences were observed in the results obtained when using either the square shear box or the circular shear cell. The same conclusion was reached when comparing the results from direct shear tests with preconsolidated and unconsolidated samples. This means that simplified devices and procedures can be used in agricultural grains against other products. Finally, a table with the recommended values for the different parameters determined for each sample tested was provided in this work.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Determination of the friction coefficients of chestnut (Castanea sativa Mill.) sawn timber
Autorzy:
Villar-Garcia, J.R.
Vidal-Lopez, P.
Corbacho, A.J.
Moya, M.
Tematy:
wood
mechanical properties
friction coefficient
direct shear test
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Instytut Agrofizyki PAN
Powiązania:
https://bibliotekanauki.pl/articles/2082657.pdf  Link otwiera się w nowym oknie
Opis:
This work provides the values of both the static and the kinetic friction coefficients for chestnut (Castanea sativa Mill.) of Spanish origin. Knowledge concerning these coefficients has its main application in the study of agroindustrial structures and machinery with timber members in contact. This determination was developed taking into account the timber anisotropy to establish surfaces and directions of slipping. A modified direct shear test device was used to conduct the tests and reproduce the tribological system. This procedure was functional and reliable and considered suitable for standardizing the friction measurement between timber surfaces, since this device is widely distributed in geotechnical and materials laboratories and the European codes do not specify a procedure or device to carry it out. The average values obtained were 0.46 for the static coefficient and 0.33 for the kinetic one, without considering the surfaces and directions of slipping. These values ranged between 0.36 and 0.55 for the static friction coefficient and between 0.28 and 0.39 for the kinetic friction coefficient depending on the direction considered and also taking into account the anisotropy of the timber. A good correlation was obtained between both coefficients, thus allowing for the estimation of the kinetic coefficient from the static one.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Defect Recovery in α-Fe e$\text{}^{-}$-irradiated at 300 K
Autorzy:
Dai, G. H.
Li, X. H.
Moser, P.
Moya, G.
Van Duysen, J. C.
Tematy:
61.70.Bv
61.80.Fe
78.70.Bj
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Instytut Fizyki PAN
Powiązania:
https://bibliotekanauki.pl/articles/1928989.pdf  Link otwiera się w nowym oknie
Opis:
Defect annealing recovery has been studied, by measuring positron lifetime spectra, in high-purity α-iron irradiated at 300 K with 3 MeV electrons to a fluency of 7 × 10$\text{}^{19}$ cm$\text{}^{-2}$. Vacancy clusters containing 6-10 single vacancies were observed immediately after irradiation during which they were possibly forming (the so-called "irradiation annealing"). With increasing temperature, the agglomerates continually grow in size at the expense of their concentration, giving rise to the formation of microvoids (> 15 vacancies). Also present were other types of defects, probably immobile vacancies trapped by impurity (e.g. carbon) atoms and dislocation/loops generated presumably from collapse of voids during the relatively high dose irradiation and/or the annealing. The immobile vacancies eventually became movable at around 350 K, supplying the growing clusters and thus leading to a stabilization in their concentration till around 500 K. Between 500 and 700 K, microvoids gradually evaporated, but the dislocation-associated defects were able to survive annealing at temperatures as high as 700 K. The void size and concentration and their evolution have been evaluated on the basis of both the to date theoretical and experimental studies. The temperature dependence was also, observed of positron trapping into vacancy agglomerates of various sizes.Za
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Subjective status and perceived legitimacy across countries
Autorzy:
Inbar, Yoel
Bocian, Konrad
Bukowski, Marcin
Lammers, Joris
Zimmerman, Jennifer L.
Korzh, Maria
Lim, Li
Motyl, Matt
Bodroža, Bojana
Peker, Müjde
Dragon, Piotr
Spears, Russell
Kuppens, Toon
Kumar Karunagharan, Jaya
Spruyt, Bram
Essien, Iniobong
Crawford, Jarret T.
Croizet, Jean‐Claude
Hong, Ryan Y.
Laham, Simon M.
Vazquez, Alexandra
Butera, Fabrizio
Igou, Eric R.
Prims, J. P.
Chryssochoou, Xenia
Graf, Sylvie
Ntani, Spyridoula
Shepherd, Lee
Becker, Julia C.
Melton, Zachary J.
Degner, Juliane
Sobkow, Agata
Teixeira, Catia P.
van Hiel, Alain
Bourguignon, David
Jiménez‐Moya, Gloria
Međedović, Janko
Platow, Michael J.
Saab, Rim
van der Toorn, Jojanneke
Rubin, Mark
Kende, Anna
Batruch, Anatolia
Butler, Sarah E.
Badea, Constantina
Houdek, Petr
Sümer, Nebi
Sankaran, Sindhuja
Jimenez Leal, William
Sweetman, Joseph
Yzerbyt, Vincent
Jetten, Jolanda
Sibley, Chris G.
Owuamalam, Chuma Kevin
Brandt, Mark J.
Ujhelyi, Adrienn
Vásquez‐Echeverría, Alejandro
Andrighetto, Luca
Durante, Federica
Manstead, Antony S. R.
Reyna, Christine
de Lemus, Soledad
Easterbrook, Matthew J.
Forgas, Joseph P.
Stroebaek, Pernille
Autin, Frederique
Halama, Peter
Vianello, Michelangelo
Toma, Claudia
González, Roberto
Vranka, Marek
Han, Gyuseog
Babincak, Peter
Conway, Paul
Bae, Jaechang
Opis:
The relationships between subjective status and perceived legitimacy are important for understanding the extent to which people with low status are complicit in their oppression. We use novel data from 66 samples and 30 countries (N = 12,788) and find that people with higher status see the social system as more legitimate than those with lower status, but there is variation across people and countries. The association between subjective status and perceived legitimacy was never negative at any levels of eight moderator variables, although the positive association was sometimes reduced. Although not always consistent with hypotheses, group identification, self‐esteem, and beliefs in social mobility were all associated with perceived legitimacy among people who have low subjective status. These findings enrich our understanding of the relationship between social status and legitimacy.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Autorzy:
Atteia, J.-L.
Blanco-Pillado, J.J.
Funk, S.
Ellis, J.
Ioannisian, A.
Miramonti, L.
Navas, S.
Nielsen, A.B.
Sahlmann, H.
Mazumdar, A.
Marcianò, A.
Pasic, V.
Pérez de los Heros, C.
Bahamonde, S.
Capozziello, S.
Joaquim, F.R.
Martín-Moruno, P.
Miller, A.L.
Stoica, S.
Martinez, Mario
Bosso, P.
Heefer, S.
Schiffer, M.
Addazi, A.
Sigl, G.
Sopuerta, C.F.
Prester, D. Dominis
Cerci, D. Sunar
Risse, M.
Saridakis, E.N.
Tinyakov, P.
Cerci, S.
Blas, D.
Calcagni, G.
Kerszberg, D.
Cortes, J.L.
Micanovic, S.
Reyes, M.A.
Tavakoli, Y.
Masip, M.
Glicenstein, J.-F.
Stergioulas, N.
Spurio, M.
Stuttard, T.
Luciano, G.G.
Escamilla-Rivera, C.
Boncioli, D.
Vagenas, E.C.
Birnholtz, O.
Demirci, M.
Rubiera-Garcia, D.
Coelho, J.A.B.
Méndez, F.
Jetzer, P.
Pasechnik, R.
Amelino-Camelia, G.
Clesse, S.
Obers, N.A.
Nardini, G.
Gubitosi, G.
Tureanu, A.
Basilakos, S.
Manganaro, M.
Milosevic, M.
Paganini, C.F.
Lim, E.
Thiemann, T.
Di Luca, M.G.
Mattingly, D.
Torri, M.D.C.
Benisty, D.
Oriti, D.
Held, A.
Frias, M.D. Rodriguez
Hinderer, T.
Vitagliano, V.
D’Esposito, V.
Asorey, M.
Alves Batista, R.
Gutierrez-Sagredo, I.
Said, J. Levi
Uysal, A. Karasu
Niechciol, M.
Platania, A.
Strišković, J.
Kuroyanagi, S.
Gracia-Ruiz, R.
Das, S.
Satunin, P.
Sakellariadou, M.
Trześniewski, Tomasz
Ternes, C.A.
Haegel, L.
Tórtola, M.
Eichhorn, A.
Peracaula, J. Solà
Bajardi, F.
Palomares-Ruiz, S.
Ricciardone, A.
Pieroni, M.
Salamida, F.
Frassino, A.M.
Frattulillo, D.
Pfeifer, C.
Martínez-Miravé, P.
Chernyakova, M.
Giesel, K.
Dimitrijevic, D.
Guendelman, E.I.
Rosati, G.
Lämmerzahl, C.
Kazarian, N.
Lobo, I.P.
Mitsou, V.A.
Arzano, M.
Gergely, L.Á.
Martínez-Huerta, H.
Mercati, F.
di Matteo, A.
Kowalski-Glikman, J.
Baret, B.
López-Moya, M.
Herranz, F.J.
Carmona, J.M.
Colak, S.M.
Fabiano, G.
Piran, T.
Bolmont, J.
Urban, F.R.
Liberati, S.
Trimarelli, C.
Relancio, J.J.
Gamboa, J.
Gracia-Bondía, J.
Franchino-Viñas, S.A.
Sotiriou, T.P.
Oikonomou, F.
Moniz, P.
Mielczarek, Jakub
Alvarez-Muniz, J.
Antonelli, V.
Djordjevic, G.
Ballesteros, A.
Mukherjee, S.
Wallet, J.-C.
Mavromatos, N.
Schüssler, F.
Vernieri, D.
Fuster, A.
Giammarchi, M.
Barreiros, D.M.
Terzić, T.
Minic, D.
Rastgoo, S.
Sitarek, J.
Kampert, K.-H.
Katori, T.
Gent, A.
Martinez, Manel
Staicova, D.
Zornoza, J.D.
Illana, J.I.
Opis:
The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review, prepared within the COST Action CA18108 "Quantum gravity phenomenology in the multi-messenger approach", is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Prospects for γ-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array
Autorzy:
Burton, M.
Di Venere, L.
Terauchi, K.
Petrucci, P.-O.
Heller, M.
Pühlhofer, G.
Meyer, D.M.-A.
Cifuentes, A.
Vovk, I.
Vázquez Acosta, M.
Cuevas, O.
Pantaleo, F.R.
Pirola, G.
Berti, A.
Di Girolamo, T.
Pueschel, E.
Ostrowski, Michał
Roache, E.
Brunetti, G.
Aschersleben, J.
Kobayashi, Y.
Wohlleben, F.
de Bony de Lavergne, M.
Incardona, F.
Kluźniak, W.
Fegan, S.
Lamastra, A.
Dominik, R.M.
Caproni, A.
Aguasca-Cabot, A.
Patricelli, B.
Nagataki, S.
Ribeiro, D.
Lenain, J.-P.
Laporte, P.
Hoffmann, D.
Depaoli, D.
Kataoka, J.
Emery, G.
Di Piano, A.
Conte, F.
Sergijenko, O.
Fallah Ramazani, V.
Torradeflot, F.
Lemoine-Goumard, M.
Nickel, L.
Horan, D.
Petruk, O.
Vitale, V.
Vercellone, S.
Yamamoto, T.
Bottacini, E.
Tsiahina, A.
Rudak, B.
Feng, Q.
Pintore, F.
Sliusar, V.
Cotter, G.
Palatiello, M.
Janecek, P.
Paoletti, R.
O'Brien, P.
Gasbarra, C.
Riitano, L.
Brun, F.
Wechakama, M.
Pietropaolo, E.
Kleiner, T.
Rainò, S.
Romeo, G.
Chaty, S.
Barbosa Martins, V.
Servillat, M.
Kluge, G.
Eckner, C.
Tramacere, A.
Giarrusso, M.
Rhode, W.
Pumo, M.L.
Oya, I.
Schipani, P.
Katagiri, H.
Viana, A.
Terrier, R.
De Lotto, B.
Santos-Lima, R.
Molfese, C.
Moderski, R.
Longo, F.
Torresi, E.
Zacharias, M.
Alfaro, R.
Gallozzi, S.
Kushida, J.
Hara, S.
Peron, G.
Harvey, V.M.
Contreras, J.L.
Shang, R.Y.
De Simone, N.
Gaggero, D.
Hadasch, D.
Grolleron, G.
De la Torre Luque, P.
Zhdanov, V.I.
Araya, M.
Donini, A.
Láinez, M.
Mas-Aguilar, A.
Bulgarelli, A.
Vodeb, V.
Salzmann, H.
Bhattacharjee, P.
della Volpe, D.
Fukui, Y.
Kowal, G.
Castro-Tirado, A.J.
Murach, T.
Benbow, W.
Kantzas, D.
Nievas Rosillo, M.
Strišković, J.
Grenier, I.
Delagnes, E.
Blanch, O.
González, J.M.
Savchenko, V.
Rosales de Leon, A.
Baquero Larriva, A.
Gueta, O.
Nosek, D.
Mello, A.J.T.S.
Font Guiteras, L.
Rowell, G.
Jiménez Martínez, I.
Podobnik, F.
Jean, P.
Principe, G.
Amato, E.
del Valle, M.V.
Ribó, M.
Hrupec, D.
Tothill, N.
Leitgeb, F.
Meyer, M.
Will, M.
Melkumyan, D.
Schubert, J.L.
Esposito, P.
Escudero, J.
Molina, E.
Vallage, B.
Leuschner, F.
Bronzini, E.
Hamal, P.
Tavernier, T.
Munari, K.
de Souza, V.
Mackey, J.
Faure, A.
Dazzi, F.
Arrabito, L.
Holder, J.
Ong, R.A.
Biland, A.
Sano, H.
Rodriguez Fernandez, G.
Vecchi, M.
Reichherzer, P.
Zdziarski, A.A.
Stolarczyk, T.
Batista, P.I.
Heckmann, L.
Righi, C.
Knödlseder, J.
Majumdar, P.
Nikołajuk, M.
Meunier, J.-L.
Rulten, C.B.
Caroff, S.
Dwarkadas, V.V.
Reisenegger, A.
Suomijärvi, T.
Galanti, G.
Batzofin, R.
Ohishi, M.
Hoang, J.
Morlino, G.
Saturni, F.G.
Nishijima, K.
Carrasco, M.-S.
Schwefer, G.
Beck, G.
Pagliaro, A.
Iocco, F.
Santangelo, A.
Ballester, O.
Delgado, C.
Jankowsky, F.
De Frondat Laadim, F.
Verna, G.
Ghalumyan, A.
Einecke, S.
González, M.M.
Steppa, C.
Prast, J.
Ashkar, H.
Starling, R.
Juramy-Gilles, C.
Produit, N.
Márquez, I.
Vallania, P.
Manicò, G.
Agudo, I.
Romano, P.
Nakamori, T.
Giesbrecht, J.
Martínez, G.A.
Toussenel, F.
Burmistrov, L.
Michałowski, J.
dos Anjos, R.D.C.
Curtis-Ginsberg, Z.
Biederbeck, N.
Rando, R.
Karas, V.
Chen, A.W.
Miener, T.
Escobar Godoy, M.
Pérez-Romero, J.
Chytka, L.
Prandini, E.
Antonelli, L.A.
Vacula, M.
Pech, M.
Panebianco, G.
Rizi, V.
Alvarez-Crespo, N.
Giordano, F.
Schwanke, U.
Acero, F.
Patel, S.R.
Šarić, T.
Balazs, C.
Hnatyk, R.
Blazek, J.
Zuriaga-Puig, J.
Delgado Giler, A.G.
Fioretti, V.
Punch, M.
Grube, J.
Lindfors, E.
Mastropietro, M.
Scherer, A.
Molero, M.
Acharyya, A.
Leto, G.
Cortina, J.
Marty, C.
Morcuende, D.
Batkovic, I.
Suda, Y.
Kubo, H.
Tajima, H.
Braiding, C.
Abe, S.
Ventura, S.
Ponti, G.
Mizuno, T.
Paredes, J.M.
Jamrozy, Marek
Olmi, B.
Marsella, G.
Leone, F.
Pita, S.
Satalecka, K.
Becker Tjus, J.
Olive, J.-F.
Tosti, L.
White, R.
Bradascio, F.
Orienti, M.
Lazarević, S.
Falceta-Goncalves, D.
Vandenbroucke, J.
Piano, G.
Voutsinas, G.
Sarkar, A.
Mitchell, A.
Reimer, A.
Barres de Almeida, U.
Biteau, J.
de Naurois, M.
Morik, K.
Dorner, D.
Živec, M.
Fedorova, E.
Cerasole, D.
Bhattacharyya, S.
Reimer, O.
Gasparrini, D.
Calisse, P.G.
Chadwick, P.
Sol, H.
Barrio, J.A.
Filipovic, M.
Fröse, S.
Green, D.
Baxter, J.
Egberts, K.
Pohl, M.
Zavrtanik, D.
Feijen, K.
Kaufmann, S.
Orito, R.
Giglietto, N.
Dumora, D.
Green, J.G.
Jin, W.
Miranda, J.M.
Paneque, D.
Nemmen, R.
Sanchez, D.
Pierre, E.
Aramo, C.
Chernyakova, M.
Boisson, C.
Horvath, P.
Michailidis, M.
Sanuy, A.
Cantlay, B.K.
Kerszberg, D.
Bucciantini, N.
Baktash, A.
Muraczewski, A.
Nozaki, S.
Brown, A.M.
Hackfeld, J.
Balbo, M.
Mandat, D.
Rieger, F.
Luque-Escamilla, P.L.
Yamazaki, R.
Doro, M.
Cerruti, M.
De Lucia, M.
Pons, E.
Truzzi, S.
Polo, M.
Niemiec, J.
Schleicher, B.
Tibaldo, L.
Chiavassa, A.
Vorobiov, S.
Manganaro, M.
Backes, M.
Tian, W.W.
Vigorito, C.F.
Vuillaume, T.
Inoue, S.
Wolter, A.
Okumura, A.
Khélifi, B.
La Palombara, N.
Rosado, J.
Rico, J.
Grau, R.
Iarlori, M.
Abe, K.
Tak, D.
Takeishi, R.
Hnatyk, B.
Markoff, S.
Costa, A.
Tejedor, L.A.
Bissaldi, E.
Vassiliev, V.
Yoshikoshi, T.
Djuvsland, J.
Recchia, S.
D'Ammando, F.
Djannati-Ataï, A.
Hassan, T.
Moulin, E.
Schussler, F.
Semikoz, D.
De Caprio, V.
Sánchez-Conde, M.
Martinez, O.
Loporchio, S.
Caraveo, P.
Starecki, T.
Hie, J.
Hanlon, W.
Macias, O.
Duangchan, C.
Goulart Coelho, J.
Gréaux, L.
Martínez, M.
Santander, M.
Bertucci, B.
Fattorini, A.
Mariotti, M.
Conforti, V.
López-Coto, R.
Ohtani, Y.
Carquin, E.
Quirrenbach, A.
Aguirre-Santaella, A.
Jarnot, C.
Stanič, S.
Linhoff, M.
Glicenstein, J.-F.
Bordas, P.
Pavlović, D.
Siqueira, C.
Lapington, J.
Bernete Medrano, J.
Torres, D.F.
Noda, K.
Morselli, A.
Muraishi, H.
Iori, M.
Nieto, D.
Slowikowska, A.
Richtler, T.
Gammaldi, V.
Asano, K.
Dournaux, J.-L.
Takahashi, M.
Walter, R.
La Barbera, A.
Zavrtanik, M.
López-Oramas, A.
de Gouveia Dal Pino, E.M.
Williams, D.A.
Razzaque, S.
Tutone, A.
Saito, T.
Hernández Cadena, S.
Amans, J.-P.
Mazin, D.
Alves Batista, R.
Inada, T.
Dörner, J.
Cristofari, P.
Spiga, D.
Liodakis, I.
Travnicek, P.
De Martino, D.
Mizote, M.
Gaug, M.
Spencer, S.T.
de Menezes, R.
Orlando, E.
Kissmann, R.
Kornecki, P.
Capuzzo-Dolcetta, R.
Brose, R.
Hofmann, W.
Novotny, V.
Sarkar, S.
van Scherpenberg, J.
Chudoba, J.
Parmiggiani, N.
Seiji, S.
Becerra González, J.
Bernlöhr, K.
Lombardi, S.
Plard, C.
Kosack, K.
Moya Zamanillo, V.
Burelli, I.
Sguera, V.
Diebold, S.
Dalchenko, M.
Campoy-Ordaz, A.
Ferrarotto, F.
Kohri, K.
Costantini, H.
Persic, M.
Bosnjak, Z.
Sadeh, I.
Goldoni, P.
Yoshida, T.
Göksu, H.
Specovius, A.
Rodríguez-Vázquez, J.J.
Voisin, V.
Viaux, N.
Evoli, C.
Fukazawa, Y.
Hervet, O.
Stawarz, Łukasz
Ferrand, G.
López-Moya, M.
Bolmont, J.
Sinha, A.
Kagaya, M.
Teshima, M.
Russo, F.
Orlandini, M.
Tanaka, S.J.
Pensec, U.
Foffano, L.
Malyshev, D.
Beshley, V.
Tripodo, G.
Granot, J.
D'Amico, G.
Fiandrini, E.
Coimbra Araujo, C.H.
Komin, N.
Regeard, M.
Elsässer, D.
Fiasson, A.
Neyroud, N.
Sharma, P.
Stamerra, A.
Priyadarshi, C.
Montaruli, T.
Peresano, M.
Ettori, S.
Queiroz, F.
Ebr, J.
Garczarczyk, M.
Alfaro, J.
Wierzcholska, A.
Sangiorgi, P.
Zaharijas, G.
Adam, R.
van Eldik, C.
Carosi, R.
Wagner, S.J.
Pecimotika, M.
Capalbi, M.
Bylund, T.
Zech, A.
Touzard, V.
Gianotti, F.
Arcaro, C.
Miceli, D.
Augusto Stuani, L.
Tosti, G.
Bi, B.
Di Pierro, F.
Marquez, P.
Baack, D.
Dell'aiera, M.
Maurin, G.
Siejkowski, H.
Seglar Arroyo, M.
Angüner, E.O.
Fontaine, G.
Ascasíbar, Y.
Jurysek, J.
Cassol, F.
Dubos, C.
Di Tria, R.
Saha, L.
Tibolla, O.
Hütten, M.
Cascone, E.
Hiroshima, N.
Vigliano, A.
Opis:
Galaxy clusters are expected to be both dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly, they are excellent targets to search for signals of DM annihilation and decay at γ-ray energies and are predicted to be sources of large-scale γ-ray emission due to hadronic interactions in the intracluster medium (ICM). In this paper, we estimate the sensitivity of the Cherenkov Telescope Array (CTA) to detect diffuse γ-ray emission from the Perseus galaxy cluster. We first perform a detailed spatial and spectral modelling of the expected signal for both the DM and the CRp components. For each case, we compute the expected CTA sensitivity accounting for the CTA instrument response functions. The CTA observing strategy of the Perseus cluster is also discussed. In the absence of a diffuse signal (non-detection), CTA should constrain the CRp to thermal energy ratio X$_{500}$ within the characteristic radius R$_{500}$ down to about $X_{500}< 3 \times10^{-3}$, for a spatial CRp distribution that follows the thermal gas and a CRp spectral index α$_{CRp}$ = 2.3. Under the optimistic assumption of a pure hadronic origin of the Perseus radio mini-halo and depending on the assumed magnetic field profile, CTA should measure α$_{CRp}$ down to about Δα$_{CRp}$ ≃ 0.1 and the CRp spatial distribution with 10% precision, respectively. Regarding DM, CTA should improve the current ground-based γ-ray DM limits from clusters observations on the velocity-averaged annihilation cross-section by a factor of up to ∼ 5, depending on the modelling of DM halo substructure. In the case of decay of DM particles, CTA will explore a new region of the parameter space, reaching models with $\tau_{χ} > 10^{27}$ s for DM masses above 1 TeV. These constraints will provide unprecedented sensitivity to the physics of both CRp acceleration and transport at cluster scale and to TeV DM particle models, especially in the decay scenario.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Prospects for a survey of the galactic plane with the Cherenkov Telescope Array
Autorzy:
Beshley, V.
Curtis-Ginsberg, Z.
Seglar Arroyo, M.
Castrejon, N.
Steppa, C.
Barrio, J.A.
Viana, A.
Sangiorgi, P.
Slowikowska, A.
Bolmont, J.
Font Guiteras, L.
Kostunin, D.
del Peral, L.
Abe, S.
López-Moya, M.
Reimer, A.
Sizun, P.
Ferrand, G.
Tibolla, O.
Alves Batista, R.
Biland, A.
Green, D.
Kagaya, M.
Kornecki, P.
Kieda, D.B.
Leuschner, F.
Dörner, J.
Hernández Cadena, S.
Boisson, C.
Stolarczyk, T.
Palatiello, M.
Vitale, V.
Ambrosino, F.
Zaharijas, G.
Morcuende, D.
van Eldik, C.
Reichherzer, P.
Pierre, E.
Holder, J.
Agudo, I.
Luque-Escamilla, P.L.
Fröse, S.
Sano, H.
Iarlori, M.
Kosack, K.
Dubus, G.
Dumora, D.
Vignatti, J.
Vacula, M.
Yoshikoshi, T.
Coimbra Araujo, C.H.
Balbo, M.
Vovk, I.
Mukherjee, R.
Janecek, P.
Regeard, M.
Crestan, S.
Gaug, M.
Orlando, S.
Nikolić, L.
Siejkowski, H.
Bhattacharjee, P.
Gréaux, L.
Miener, T.
Macias, O.
Beiske, L.
Tian, W.W.
Wierzcholska, A.
Braiding, C.
Augusto Stuani, L.
Dubos, C.
Leone, F.
Nickel, L.
Stanič, S.
Travnicek, P.
Zacharias, M.
de Menezes, R.
Cifuentes, A.
Grasso, D.
Moralejo, A.
Renaud, M.
Rhode, W.
Greenshaw, T.
Bernardini, E.
Bordas, P.
De Frondat Laadim, F.
Olive, J.-F.
Nosek, D.
López-Coto, R.
Leto, G.
Sapienza, V.
Sánchez-Conde, M.
Feijen, K.
Holler, M.
Ruiter, A.J.
Mizuno, T.
Cascone, E.
Wohlleben, F.
Marsella, G.
Vodeb, V.
Rodríguez-Vázquez, J.J.
Lombardi, S.
Chernyakova, M.
Salzmann, H.
Dournaux, J.-L.
Novosyadlyj, B.
Vecchi, M.
Ventura, S.
Ziętara, Krzysztof
Lazendic-Galloway, J.
Lozano Bahilo, J.
Chen, A.W.
de Naurois, M.
Brose, R.
Duffy, S.
Orlando, E.
Suda, Y.
Miceli, M.
Burmistrov, L.
Bronzini, E.
Dalchenko, M.
Caraveo, P.
Pantaleo, F.R.
Quirrenbach, A.
Tripodo, G.
Jankowsky, F.
Carrasco, M.-S.
Pumo, M.L.
Terada, Y.
Foffano, L.
Liodakis, I.
Tsiahina, A.
Brunelli, G.
Jarnot, C.
Calisse, P.G.
Horan, D.
Ponti, G.
de Martino, D.
Mas-Aguilar, A.
Khélifi, B.
Chadwick, P.M.
Rigoselli, M.
Errando, M.
Inoue, S.
Rosales de Leon, A.
Garczarczyk, M.
Bonnoli, G.
Siqueira, C.
Cotter, G.
Hnatyk, B.
Di Tria, R.
Nozaki, S.
Asano, K.
Takeishi, R.
De la Torre Luque, P.
Menchiari, S.
Maurin, G.
Martínez, M.
Marcowith, A.
Muraczewski, A.
Bosnjak, Z.
Giesbrecht, J.
Prokhorov, D.
Lucarelli, F.
dos Anjos, R.D.C.
Olmi, B.
Gallozzi, S.
Giglietto, N.
Markoff, S.
Amans, J.-P.
Russo, F.
Suomijärvi, T.
Fiandrini, E.
Spencer, S.T.
Marinos, P.
Pérez-Romero, J.
Rando, R.
Vaclavek, L.
Kubo, H.
Schipani, P.
Della Valle, M.
Pech, M.
Komin, N.
Tanaka, S.J.
Feng, Q.
Adam, R.
Mariotti, M.
Djuvsland, J.
Pagliaro, A.
La Palombara, N.
Maier, G.
Villanueva, J.
Ferrarotto, F.
Vazquez Acosta, M.L.
Rico, J.
Lyard, E.
Zuriaga-Puig, J.
Gallant, Y.A.
Bylund, T.
de Ona Wilhelmi, E.
Vigorito, C.F.
Vuillaume, T.
Caroff, S.
della Volpe, D.
Meunier, J.-L.
Carquin, E.
Yamazaki, R.
Hara, S.
Ohishi, M.
Jurysek, J.
Horvath, P.
Kalekin, O.
Ribó, M.
Rieger, F.
Rodriguez Fernandez, G.
Jiménez Martínez, I.
Ravel, T.
Fioretti, V.
Gueta, O.
Guillemot, L.
Cristofari, P.
Sarkar, S.
Hermann, G.
Duangchan, C.
Okumura, A.
Arcaro, C.
Burtovoi, A.
Acharyya, A.
Schiavone, F.
Remy, Q.
Cantlay, B.K.
Richtler, T.
Iocco, F.
Cerruti, M.
Scherer, A.
Fontaine, G.
Incardona, F.
Kerszberg, D.
Fattorini, A.
Manicò, G.
Ballet, J.
Voutsinas, G.
Kataoka, J.
Baxter, J.
Molero, M.
Eckner, C.
Hinton, J.
Ascasíbar, Y.
Toussenel, F.
Nemmen, R.
Piano, G.
Petrucci, P.-O.
Vorobiov, S.
Malyshev, D.
Berti, A.
Orienti, M.
Mastropietro, M.
Blazek, J.
Jamrozy, Marek
Wechakama, M.
Funk, S.
Moya Zamanillo, V.
Heckmann, L.
Laporte, P.
Marquez, P.
Aschersleben, J.
Tavecchio, F.
Voisin, V.
Baquero Larriva, A.
Zampieri, L.
Ambrosi, G.
Conte, F.
Biederbeck, N.
Morselli, A.
Marty, C.
Escudero, J.
Knödlseder, J.
Egberts, K.
Di Piano, A.
Alvarez-Crespo, N.
Furniss, A.
Saha, L.
Amato, E.
Belmont, R.
Muraishi, H.
Stamerra, A.
Romeo, G.
Vink, J.
Queiroz, F.
Williams, D.A.
Domínguez, A.
Yoshida, T.
Reimer, O.
Nakamori, T.
Hrabovsky, M.
Giordano, F.
Bernlöhr, K.
Brown, A.M.
Green, J.G.
Pueschel, E.
Reposeur, T.
Viaux, N.
Lindfors, E.
Steinmassl, S.
Meyer, D.M.-A.
Goldoni, P.
Mello, A.J.T.S.
Arrabito, L.
Fukazawa, Y.
Paoletti, R.
Gasbarra, C.
Sliusar, V.
Di Pierro, F.
Depaoli, D.
Backes, M.
Esposito, P.
Kluźniak, W.
Persic, M.
Escarate, P.
Barbosa Martins, V.
Mestre, E.
Ohtani, Y.
Umana, G.
Balazs, C.
Touzard, V.
Rudak, B.
Terrier, R.
Sguera, V.
Peresano, M.
Bucciantini, N.
Tajima, H.
Grenier, I.
Servillat, M.
Tothill, N.
Michałowski, J.
Prandini, E.
Jin, W.
Lenain, J.-P.
Orlandini, M.
Panebianco, G.
Lazarević, S.
Iori, M.
Martin, P.
Doro, M.
Burelli, I.
Batzofin, R.
Carosi, A.
Juramy-Gilles, C.
Orito, R.
de Souza, V.
Parmiggiani, N.
Burton, M.
Giuffrida, R.
Tutone, A.
Smith, D.A.
Bonollo, A.
Blanch, O.
Pintore, F.
Dominik, R.M.
Delgado, C.
Schussler, F.
D'Aì, A.
Falceta-Goncalves, D.
Alfaro, J.
Costa, A.
Fiori, M.
Torradeflot, F.
Schubert, J.L.
Delgado Giler, A.G.
Nieto, D.
Teshima, M.
Ong, R.A.
Hassan, T.
Ostrowski, Michał
Schwanke, U.
Schwefer, G.
Zavrtanik, M.
Romano, P.
Ebr, J.
Caproni, A.
Moulin, E.
Patricelli, B.
Verna, G.
Kaufmann, S.
Santangelo, A.
Chambery, P.
Fegan, S.
Morik, K.
Produit, N.
Tavernier, T.
Paredes, J.M.
Kobayashi, Y.
Gaggero, D.
Karas, V.
Grondin, M.-H.
Emery, G.
Flores, H.
Munari, K.
Beck, G.
de Gouveia Dal Pino, E.M.
Heller, M.
Harvey, V.M.
Biteau, J.
Contreras, J.L.
Roache, E.
Batković, I.
Einecke, S.
Fiasson, A.
López-Oramas, A.
Miranda, J.M.
Loporchio, S.
Molfese, C.
Priyadarshi, C.
Dinesh, A.
Yang, L.
Kushida, J.
Bocchino, F.
Razzaque, S.
Hovatta, T.
Martínez, G.A.
Hadasch, D.
González, J.M.
Jean, P.
Costantini, H.
Campoy-Ordaz, A.
Diebold, S.
Bhattacharyya, S.
Mohrmann, L.
Kantzas, D.
Dell'aiera, M.
Wagner, S.J.
Murach, T.
Capuzzo-Dolcetta, R.
Niemiec, J.
Linhoff, M.
Petruk, O.
Cuevas, O.
Nikołajuk, M.
Noda, K.
Acero, F.
Aguasca-Cabot, A.
Zavrtanik, D.
Cortina, J.
Podobnik, F.
Stawarz, Łukasz
David, L.
Spiga, D.
Barres de Almeida, U.
Molina, E.
Paneque, D.
Tibaldo, L.
Pagano, I.
Abhir, J.
Conforti, V.
Kohri, K.
Mandat, D.
Hnatyk, R.
D'Ammando, F.
Díaz, C.
Martí, J.
Waegebaert, V.
Pecimotika, M.
Zanin, R.
Novotny, V.
Sol, H.
Vercellone, S.
Kleiner, T.
de Bony de Lavergne, M.
Oya, I.
Rulten, C.B.
Bonneau Arbeletche, L.
Trois, A.
Glombitza, J.
Cassol, F.
Schleicher, B.
Dadina, M.
Fukui, Y.
Kazanas, D.
Granot, J.
McKeague, S.
Bi, B.
Nagataki, S.
Pohl, M.
Dazzi, F.
Evoli, C.
Schovanek, P.
Hayashi, K.
Grau, R.
Saturni, F.G.
Brun, F.
Vallania, P.
Giuliani, A.
Carosi, R.
Montaruli, T.
Lapington, J.
Filipovic, M.
Pühlhofer, G.
Benbow, W.
Kissmann, R.
Miceli, D.
Mazin, D.
Godinovic, N.
De Caprio, V.
Hofmann, W.
Hervet, O.
Di Venere, L.
Pietropaolo, E.
Goulart Coelho, J.
Kowal, G.
Bertucci, B.
Pérez-Torres, M.A.
Sergijenko, O.
Saito, T.
Giarrusso, M.
Zhdanov, V.I.
Walter, R.
Šarić, T.
Donini, A.
Escanuela, C.
Ribeiro, D.
Grolleron, G.
Rowell, G.
Santander, M.
Starling, R.
Pons, E.
Inada, T.
Principe, G.
Torres, D.F.
Morlino, G.
Dwarkadas, V.V.
Zech, A.
Mackey, J.
White, R.
Chaty, S.
Angüner, E.O.
Michailidis, M.
D'Amico, G.
Hackfeld, J.
Seitenzahl, I.
De Lucia, M.
Pittori, C.
Aramo, C.
Sharma, P.
Mereghetti, S.
Galanti, G.
Bulgarelli, A.
Gammaldi, V.
Ghalumyan, A.
Vigliano, A.
Becerra González, J.
Sadeh, I.
Kluge, G.
Martinez, O.
Gasparrini, D.
Castro-Tirado, A.J.
Zdziarski, A.A.
Aguirre-Santaella, A.
Láinez, M.
Peron, G.
La Barbera, A.
Patel, S.R.
Gunji, S.
Katagiri, H.
Escobar Godoy, M.
Rizi, V.
Pihet, M.
Punch, M.
Mitchell, A.
Cerasole, D.
De Lotto, B.
Galaz, G.
Bissaldi, E.
Živec, M.
Bernete, J.
Chiavassa, A.
Hanlon, W.
Vassiliev, V.
Moderski, R.
Santos-Lima, R.
Djannati-Ataï, A.
Elsässer, D.
Di Girolamo, T.
Pavlović, D.
Glicenstein, J.-F.
Rosado, J.
Nievas Rosillo, M.
Longo, F.
Chytka, L.
Hiroshima, N.
Lamastra, A.
Plard, C.
Lemoine-Goumard, M.
Abhishek, A.
Bottacini, E.
Opis:
Approximately one hundred sources of very-high-energy (VHE) gamma rays are known in the Milky Way, detected with a combination of targeted observations and surveys. A survey of the entire Galactic Plane in the energy range from a few tens of GeV to a few hundred TeV has been proposed as a Key Science Project for the upcoming Cherenkov Telescope Array Observatory (CTAO). This article presents the status of the studies towards the Galactic Plane Survey (GPS). We build and make publicly available a sky model that combines data from recent observations of known gamma-ray emitters with state-of-the-art physically-driven models of synthetic populations of the three main classes of established Galactic VHE sources (pulsar wind nebulae, young and interacting supernova remnants, and compact binary systems), as well as of interstellar emission from cosmic-ray interactions in the Milky Way. We also perform an optimisation of the observation strategy (pointing pattern and scheduling) based on recent estimations of the instrument performance. We use the improved sky model and observation strategy to simulate GPS data corresponding to a total observation time of 1620 hours spread over ten years. Data are then analysed using the methods and software tools under development for real data. Under our model assumptions and for the realisation considered, we show that the GPS has the potential to increase the number of known Galactic VHE emitters by almost a factor of five. This corresponds to the detection of more than two hundred pulsar wind nebulae and a few tens of supernova remnants at average integral fluxes one order of magnitude lower than in the existing sample above 1 TeV, therefore opening the possibility to perform unprecedented population studies. The GPS also has the potential to provide new VHE detections of binary systems and pulsars, to confirm the existence of a hypothetical population of gamma-ray pulsars with an additional TeV emission component, and to detect bright sources capable of accelerating particles to PeV energies (PeVatrons). Furthermore, the GPS will constitute a pathfinder for deeper follow-up observations of these source classes. Finally, we show that we can extract from GPS data an estimate of the contribution to diffuse emission from unresolved sources, and that there are good prospects of detecting interstellar emission and statistically distinguishing different scenarios. Thus, a survey of the entire Galactic plane carried out from both hemispheres with CTAO will ensure a transformational advance in our knowledge of Galactic VHE source populations and interstellar emission.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Dark matter line searches with the Cherenkov Telescope Array
Autorzy:
Burton, M.
Siegert, T.
Prouza, M.
Di Venere, L.
Terauchi, K.
Orlando, S.
Pühlhofer, G.
Heller, M.
Rodríguez Frías, M.D.
Meyer, D.M.-A.
Cifuentes, A.
Vovk, I.
Vázquez Acosta, M.
Cuevas, O.
Pantaleo, F.R.
Pirola, G.
Berti, A.
Di Girolamo, T.
Pueschel, E.
Pihet, M.
Ostrowski, Michał
Roache, E.
Testa, V.
Aschersleben, J.
Abhir, J.
Kobayashi, Y.
Wohlleben, F.
de Bony de Lavergne, M.
Incardona, F.
Fegan, S.
Lamastra, A.
Dominik, R.M.
Abhishek, A.
Aguasca-Cabot, A.
Caproni, A.
Patricelli, B.
Sæther Hatlen, E.
Ribeiro, D.
Lenain, J.-P.
Laporte, P.
Hayashi, K.
Voitsekhovskyi, V.
Kataoka, J.
Depaoli, D.
Ducci, L.
Cicciari, G.M.
Emery, G.
Hovatta, T.
Di Piano, A.
Conte, F.
Sergijenko, O.
Visentin, E.
Torradeflot, F.
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Rodríguez-Vázquez, J.J.
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Ferrand, G.
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Foffano, L.
Malyshev, D.
Tripodo, G.
Granot, J.
D'Amico, G.
Fiandrini, E.
Coimbra Araujo, C.H.
Komin, N.
Regeard, M.
Elsässer, D.
Zhang, W.
Fiasson, A.
Kieda, D.B.
Stamerra, A.
Priyadarshi, C.
Montaruli, T.
Peresano, M.
Ettori, S.
Queiroz, F.
Ebr, J.
Garczarczyk, M.
Alfaro, J.
Wierzcholska, A.
Sangiorgi, P.
Zaharijas, G.
Adam, R.
Moralejo, A.
van Eldik, C.
Carosi, R.
Wagner, S.J.
Pecimotika, M.
Bylund, T.
De Angelis, A.
Zech, A.
Gianotti, F.
Arcaro, C.
Miceli, D.
Tosti, G.
Di Pierro, F.
Marquez, P.
Cailleux, J.
Dell'aiera, M.
Siejkowski, H.
Seglar Arroyo, M.
Fontaine, G.
Jurysek, J.
Kazanas, D.
Cassol, F.
Dubos, C.
Di Tria, R.
Glombitza, J.
Saha, L.
Errando, M.
Tibolla, O.
Sol, H.
Hiroshima, N.
Vigliano, A.
Opis:
Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from astrophysical or instrumental backgrounds. We provide an updated assessment of the sensitivity of the Cherenkov Telescope Array (CTA) to such signals, based on observations of the Galactic centre region as well as of selected dwarf spheroidal galaxies. We find that current limits and detection prospects for dark matter masses above 300 GeV will be significantly improved, by up to an order of magnitude in the multi-TeV range. This demonstrates that CTA will set a new standard for gamma-ray astronomy also in this respect, as the world's largest and most sensitive high-energy gamma-ray observatory, in particular due to its exquisite energy resolution at TeV energies and the adopted observational strategy focussing on regions with large dark matter densities. Throughout our analysis, we use up-to-date instrument response functions, and we thoroughly model the effect of instrumental systematic uncertainties in our statistical treatment. We further present results for other potential signatures with sharp spectral features, e.g. box-shaped spectra, that would likewise very clearly point to a particle dark matter origin.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł

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