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Wyszukujesz frazę "Edwards, D." wg kryterium: Autor


Tytuł:
Capturing the social and cultural values of European forests: insights from “EFORWOOD”
Autorzy:
Edwards, D.
Tematy:
capturing
social value
cultural value
Europe
forest
insight
EFORWOOD project
recreation
Pokaż więcej
Wydawca:
Instytut Badawczy Leśnictwa
Powiązania:
https://bibliotekanauki.pl/articles/38629.pdf  Link otwiera się w nowym oknie
Opis:
This paper draws from research carried out as part of the EU-funded project ‘EFORWOOD-IP: Tools for Sustainability Impact Assessment of the European Forestry-Wood Chain’. The paper reports on a literature review to develop a generic template of social and cultural values and indicators associated with forests in Europe, and research to develop ‘forest recreational use’ as an indicator to assess the social impacts of changes in forest management as part of European impact assessment procedures.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Short-term survival of ammonites in New Jersey after the end-Cretaceous bolide impact
Autorzy:
Landman, N.H.
Garb, M.P.
Rovelli, R.
Ebel, D.S.
Edwards, L.E.
Tematy:
short-term survival
ammonite
New Jersey
Cretaceous
bolide impact
Ammonoidea
biostratigraphy
extinction
Paleogene
boundary
Pokaż więcej
Wydawca:
Polska Akademia Nauk. Instytut Paleobiologii PAN
Powiązania:
https://bibliotekanauki.pl/articles/22198.pdf  Link otwiera się w nowym oknie
Opis:
A section containing the Cretaceous/Paleogene (= Cretaceous/Tertiary) boundary in Monmouth County, New Jersey, preserves a record of ammonites extending from the end of the Cretaceous into possibly the beginning of the Danian. The section includes the upper part of the Tinton Formation and lower part of the Hornerstown Formation. The top of the Tinton Formation is represented by a richly fossiliferous unit (the Pinna Layer) that contains many bivalves in life position as well as ammonite jaws preserved inside body chambers. Ammonites include Pachydiscus (Neodesmoceras) mokotibensis, Sphenodiscus lobatus, Eubaculites carinatus, E. latecarinatus, Discoscaphites iris, D. sphaeroidalis, D. minardi, and D. jerseyensis. The Pinna Layer probably represents a relatively short interval of time lasting tens to hundreds of years; it is conformably overlain by the Burrowed Unit, which contains a single fragment of Discoscaphites sp. and several fragments of E. latecarinatus, as well as several isolated specimens of ammonite jaws including two of Eubaculites. Examination of the mode of preservation of the ammonites and jaws suggests that they were fossilized during deposition of the Burrowed Unit and were not reworked from older deposits. Based on the ammonites and dinoflagellates in the Pinna Layer and the Burrowed Unit, these strata traditionally would be assigned to the uppermost Maastrichtian, corresponding to calcareous nannofossil Subzone CC26b. However, a weak iridium anomaly (500–600 pg/g) is present at the base of the Pinna Layer, which presumably represents the record of the bolide impact. Correlation with the iridium layer at the Global Stratotype Section and Point at El Kef, Tunisia, would, therefore, imply that these assemblages are actually Danian, provided that the iridium anomaly is in place and the ammonites and dinoflagellates are not reworked. If the iridium anomaly is in place, or even if it has migrated downward from the top of the Pinna Layer, the ammonites would have survived the impact at this site for a brief interval of time lasting from a few days to hundreds of years.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
Autorzy:
Beshley, V.
Viana, A.
Sangiorgi, P.
Pavletić, L.
Ferrand, G.
Prast, J.
De Angelis, A.
Alves Batista, R.
Biland, A.
Strišković, J.
Yanagita, S.
Brill, A.
Weniger, C.
Meyer, M.
Stolarczyk, T.
Hernández Cadena, S.
Boisson, C.
Morcuende-Parrilla, D.
Palatiello, M.
Vitale, V.
Sanchez, D.
Zaharijas, G.
van Eldik, C.
Gent, A.
Holder, J.
Agudo, I.
Mundell, C.
Sano, H.
Iarlori, M.
de Cássia dos Anjos, R.
Pumo, M. L.
Dmytriiev, A.
Yoshikoshi, T.
Vovk, I.
Mukherjee, R.
Janecek, P.
Gianotti, F.
Orlando, S.
Mirzoyan, R.
Sciacca, E.
Siejkowski, H.
Zhdanov, V. I.
Miener, T.
Antonelli, L. A.
Wierzcholska, A.
Miranda, J. M.
Leone, F.
Stanič, S.
Travnicek, P.
Zacharias, M.
Armstrong, T.
Grasso, D.
Moralejo, A.
Pareschi, G.
Rhode, W.
Çolak, M.
Bernardini, E.
Bordas, P.
Nosek, D.
López-Coto, R.
Leto, G.
Sánchez-Conde, M.
Casanova, S.
Mizuno, T.
Cascone, E.
Lombardi, S.
Chernyakova, M.
Gascon, D.
Vecchi, M.
Ventura, S.
Coronado-Blazquez, J.
Rodriguez Ramirez, J. C.
Orlando, E.
Suda, Y.
Miceli, M.
Caraveo, P.
Prokoph, H.
Quirrenbach, A.
Foffano, L.
Nagai, A.
Tosti, L.
Horan, D.
Rojas, G.
Green, J.
Ferrara, G.
Inoue, S.
Garczarczyk, M.
Siqueira, C.
Fukami, S.
Cotter, G.
Hnatyk, B.
Nozaki, S.
Asano, K.
Angüner, E. O.
Maurin, G.
Varner, G. S.
Martínez, M.
Bosnjak, Z.
Alispach, C.
Tejedor, L. A.
Williams, D. A.
Chudoba, J.
Pfrang, K.
Todero Peixoto, C. J.
Recchia, S.
Giglietto, N.
Markoff, S.
Russo, F.
Ballester, O.
Fiandrini, E.
Pérez-Romero, J.
Rando, R.
Coniglione, R.
Kubo, H.
Komin, N.
Feng, Q.
Adam, R.
Mariotti, M.
Pagliaro, A.
Maier, G.
Damone, L. A.
Rico, J.
Brown, A. M.
Rinchiuso, L.
Straumann, U.
Vuillaume, T.
Garcia, E.
della Volpe, D.
Berge, D.
Sokolenko, A.
Barrio, J. A.
de Oña Wilhelmi, E.
Ohishi, M.
Jurysek, J.
Horvath, P.
Saturni, F. G.
Ribó, M.
Rieger, F.
Rodriguez Fernandez, G.
Fioretti, V.
Gueta, O.
Cristofari, P.
Sarkar, S.
Vigorito, C. F.
Okumura, A.
Grillo, A.
Shalchi, A.
Burtovoi, A.
Acharyya, A.
Richtler, T.
Iocco, F.
Cerruti, M.
Fontaine, G.
Kerszberg, D.
De Martino, D.
Cauz, D.
Manicò, G.
Shellard, R. C.
Barkov, M.
Leigui de Oliveira, M. A.
Eckner, C.
Truzzi, S.
Delgado Giler, A. G.
Medina Miranda, D.
Ascasíbar, Y.
Nemmen, R.
Piano, G.
Vorobiov, S.
Zechlin, H.
Vázquez Acosta, M.
Berti, A.
Orienti, M.
Seglar-Arroyo, M.
Blazek, J.
Mangano, S.
Mallamaci, M.
Bozhilov, V.
Jamrozy, Marek
Will, M.
Suomijarvi, T.
Sanuy, A.
Fornieri, O.
Pantaleo, F. R.
López, M.
Laporte, P.
Marquez, P.
Tavecchio, F.
Zampieri, L.
Baquero Larriva, A.
Ambrosi, G.
Conte, F.
Morselli, A.
Pillera, R.
Knödlseder, J.
Renier, Y.
Sæther Hatlen, E.
Salesa Greus, F.
Romeo, G.
Stamerra, A.
Queiroz, F.
Vink, J.
Domínguez, A.
Reimer, O.
Nakamori, T.
Hrabovsky, M.
Giordano, F.
Bernlöhr, K.
Brun, P.
Lindfors, E.
Goldoni, P.
Ekoume, T. R. N.
Benito, M.
White, M.
Katarzyński, K.
Reisenegger, A.
Sliusar, V.
Di Pierro, F.
Depaoli, D.
Persic, M.
Barbosa Martins, V.
Ohtani, Y.
Balazs, C.
Rudak, B.
Luque-Escamilla, P. L.
Pe'er, A.
Servillat, M.
Tothill, N.
Prandini, E.
Jin, W.
Orlandini, M.
Becker Tjus, J.
Bregeon, J.
Iori, M.
Doro, M.
Carosi, A.
Orito, R.
Lenain, J.
Wagner, S. J.
de Souza, V.
Parmiggiani, N.
Burton, M.
Chen, A.
Blanch, O.
Pintore, F.
Silk, J.
Delgado, C.
Schussler, F.
Falceta-Goncalves, D.
Alfaro, J.
Costa, A.
Becerra, J.
Mbarubucyeye, J. D.
Fiori, M.
Santos, E. M.
Hrupec, D.
Nieto, D.
Poireau, V.
Teshima, M.
Mode, B.
Daniel, M. K.
Hassan, T.
Ostrowski, Michał
Schwanke, U.
Zavrtanik, M.
Romano, P.
Ebr, J.
Caproni, A.
Paredes, J. M.
Cameron, R.
Zakaria, A. A.
Patricelli, B.
Gourgouliatos, K.
Salina, G.
Vandenbroucke, J.
Verna, G.
Fegan, S.
Araudo, A.
Kobayashi, Y.
Gaggero, D.
Contreras, J. L.
Chikawa, M.
Gnatyk, R.
Prado, R. R.
Oka, T.
Edwards, T. D. P.
Vallage, B.
Beck, G.
Lopez, A.
Lamanna, G.
Scuderi, S.
Franco, F. J.
Halim, A.
Heller, M.
Wiemann, R.
Testa, V.
Biteau, J.
Fiasson, A.
Hughes, G.
Alfaro, R.
De Palma, F.
Loporchio, S.
Safi-Harb, S.
Catalani, F.
Humensky, T. B.
Kushida, J.
Yang, L.
Bocchino, F.
Tonev, D.
Razzaque, S.
Hovatta, T.
Arqueros, F.
Manganaro, M.
Chiaro, G.
Prouza, M.
Costantini, H.
Zdziarski, A. A.
Diebold, S.
Fedorova, E.
Mohrmann, L.
Ninci, D.
Zaric, D.
Capuzzo-Dolcetta, R.
Niemiec, J.
D'Aimath, A.
Petruk, O.
Jouvin, L.
Glicenstein, J.
Spencer, S.
Nikołajuk, M.
Martínez-Huerta, H.
Noda, K.
Biasuzzi, B.
Zavrtanik, D.
Słowikowska, A.
Barres de Almeida, U.
Molina, E.
Tibaldo, L.
Pagano, I.
Conforti, V.
Adams, C.
Kohri, K.
Mandat, D.
D'Ammando, F.
Amati, L.
Martí, J.
Zanin, R.
Pecimotika, M.
Watson, J.
Hütten, M.
Sol, H.
Vercellone, S.
Oya, I.
Bonneau Arbeletche, L.
Pilszyk, B.
Lohse, T.
Giavitto, G.
Cassol, F.
Fukui, Y.
Kazanas, D.
Granot, J.
Vergani, S.
Pohl, M.
Dazzi, F.
Evoli, C.
Rodriguez, J.
Capasso, M.
Brun, F.
Vallania, P.
Giuliani, A.
Carosi, R.
Montaruli, T.
Lapington, J.
Filipovic, M.
Pühlhofer, G.
Benbow, W.
Kissmann, R.
Bruno, P.
Mazin, D.
De Caprio, V.
Martínez, G.
Hofmann, W.
Di Venere, L.
Pietropaolo, E.
Marculewicz, M.
Bringmann, T.
Ong, R. A.
Ashley, M.
Hörandel, J.
Bertucci, B.
de Gouveia Dal Pino, E. M.
Sergijenko, O.
Giarrusso, M.
Walter, R.
Donini, A.
Malta Nunes de Almeida, R.
Ribeiro, D.
Rowell, G.
Santander, M.
Starling, R.
Inada, T.
Principe, G.
Zech, A.
Mach, E.
González, M. M.
White, R.
Bastieri, D.
Chaty, S.
Aramo, C.
Wischnewski, R.
Sharma, P.
Taylor, L.
Bulgarelli, A.
Gammaldi, V.
Ghalumyan, A.
Karukes, E.
Sadeh, I.
Martinez, O.
Piatteli, P.
Aguirre-Santaella, A.
Sawangwit, U.
Kherlakian, M. C.
Gunji, S.
Rainò, S.
Rizi, V.
Buscemi, M.
Seweryn, K.
De Lotto, B.
Galaz, G.
Bissaldi, E.
Živec, M.
Chiavassa, A.
Tokanai, F.
Vassiliev, V.
Aloisio, R.
Moderski, R.
Santos-Lima, R.
Chadwick, P.
Tosti, G.
Elsässer, D.
Minev, M.
Di Girolamo, T.
Maggio, C.
Vagelli, V.
Świerk, P.
Rosado, J.
Longo, F.
Przybilski, H.
Hiroshima, N.
Ohira, Y.
Bottacini, E.
Opis:
We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray signal from pair-annihilating dark matter particles in the region around the Galactic centre. We find that CTA will open a new window of discovery potential, significantly extending the range of robustly testable models given a standard cuspy profile of the dark matter density distribution. Importantly, even for a cored profile, the projected sensitivity of CTA will be sufficient to probe various well-motivated models of thermally produced dark matter at the TeV scale. This is due to CTA's unprecedented sensitivity, angular and energy resolutions, and the planned observational strategy. The survey of the inner Galaxy will cover a much larger region than corresponding previous observational campaigns with imaging atmospheric Cherenkov telescopes. CTA will map with unprecedented precision the large-scale diffuse emission in high-energy gamma rays, constituting a background for dark matter searches for which we adopt state-of-the-art models based on current data. Throughout our analysis, we use up-to-date event reconstruction Monte Carlo tools developed by the CTA consortium, and pay special attention to quantifying the level of instrumental systematic uncertainties, as well as background template systematic errors, required to probe thermally produced dark matter at these energies.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł

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