Zobrazeno 1 - 10
of 1 748
pro vyhledávání: '"Falvard A"'
Autor:
Fabbri, Stefano C., Sabatier, Pierre, Paris, Raphaël, Falvard, Simon, Feuillet, Nathalie, Lothoz, Amélie, St-Onge, Guillaume, Gailler, Audrey, Cordrie, Louise, Arnaud, Fabien, Biguenet, Maude, Coulombier, Thibault, Mitra, Saptarshee, Chaumillon, Eric
Publikováno v:
In Marine Geology May 2024 471
Autor:
Mitra, Saptarshee, Paris, Raphaël, Bernard, Laurent, Abbal, Rémi, Charrier, Pascal, Falvard, Simon, Costa, Pedro, Andrade, César
Publikováno v:
In Marine Geology April 2024 470
Autor:
Sajjad, S., Falvard, A.
In gamma-ray astronomy through Imaging Atmospheric Cherenkov Telescopes (IACT), the atmosphere is used as a calorimeter. Incident gamma-rays in the GeV-TeV energy range are observed through the electromagnetic showers they produce in the atmosphere a
Externí odkaz:
http://arxiv.org/abs/2010.13822
Publikováno v:
In Marine Geology October 2022 452
The future of ground based gamma ray astronomy lies in large arrays of Imaging Atmospheric Cherenkov Telescopes (IACT) with better capabilities: lower energy threshold, higher sensitivity, better resolution and background rejection. Currently, design
Externí odkaz:
http://arxiv.org/abs/0801.4742
Autor:
Jacholkowska, A., Lamanna, G., Nuss, E., Bolmont, J., Adloff, C., Alcaraz, J., Battiston, R., Brun, P., Burger, W. J., Choutko, V., Coignet, G., Falvard, A., Flandrini, E., Girard, L., Goy, C., Jedamzik, K., Kossakowski, R., Moultaka, G., Natale, S., Pochon, J., Pohl, M., Rosier-Lees, S., Sapinski, M., Noarbe, I. Sevilla, Vialle, JP.
Publikováno v:
Phys.Rev.D74:023518,2006
The detection of non-baryonic dark matter through its gamma-ray annihilation in the centre of our galaxy has been studied. The gamma fluxes according to different models have been simulated and compared to those expected to be observed with the Alpha
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508349
Autor:
Falvard, Simon, Paris, Raphaël, Belousova, Marina, Belousov, Alexander, Giachetti, Thomas, Cuven, Stéphanie
Publikováno v:
In Marine Geology 1 February 2018 396:160-170
Autor:
Nuss, E., Moultaka, G., Falvard, A., Giraud, E., Jacholkowska, A., Jedamzik, K., Lavalle, J., Piron, F., Sapinski, M., Salati, P., Taillet, R.
It is widely believed that dark matter exists within galaxies and clusters of galaxies. Under the assumption that this dark matter is composed of the lightest, stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indir
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212560
Autor:
Falvard, A., Giraud, E., Jacholkowska, A., Lavalle, J., Nuss, E., Piron, F., Sapinski, M., Salati, P., Taillet, R., Jedamzik, K., Moultaka, G.
Publikováno v:
Astropart.Phys. 20 (2004) 467-484
It is widely believed that dark matter exists within galaxies and clusters of galaxies. Under the assumption that this dark matter is composed of the lightest, stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indir
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210184
Autor:
Giraud, E., Meylan, G., Sapinski, M., Falvard, A., Jacholkowska, A., Jedamzik, K., Lavalle, J., Nuss, E., Moultaka, G., Piron, F., Salati, P., Taillet, R.
The distant globular cluster Palomar 13 has been found to have a very high mass-to-light ratio and its profile can be well fitted either by a King model with a tail, or with a NFW model. This cluster may be the first case of the many clumps predicted
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209230