Zobrazeno 1 - 10
of 1 377
pro vyhledávání: '"Pons, R."'
Publikováno v:
Phys. Rev. B 102, 235101 (2020)
We discuss twisted bilayer graphene (TBG) based on a theorem of flat band ferromagnetism put forward by Mielke and Tasaki. According to this theorem, ferromagnetism occurs if the single particle density matrix of the flat band states is irreducible a
Externí odkaz:
http://arxiv.org/abs/2007.04076
Autor:
Lacombe, K., Amoros, C., Atteia, J. -L., Bajat, A., Bouchet, L., Dezalay, J. -P., Guillemot, P., Houret, B., Lebrun, F., Mate, S., Pons, R., Triou, H., Waegebaert, V.
Publikováno v:
Exp Astron (2019) 47: 245
We discuss the need for very large detection planes for the detection of hard X-ray transients in the multi-messenger era that started with the quasi-simultaneous detection of GRB~170817A by \textit{Fermi}/GBM and \textit{INTEGRAL}/SPI on one hand an
Externí odkaz:
http://arxiv.org/abs/1909.09015
Publikováno v:
Seminars in Musculoskeletal Radiology; 2024 Supplement 1, Vol. 28, pS1-S24, 24p
Autor:
Godet, O., Nasser, G., Atteia, J. -L., Cordier, B., Mandrou, P., Barret, D., Triou, H., Pons, R., Amoros, C., Bordon, S., Gevin, O., Gonzalez, F., Götz, D., Gros, A., Houret, B., Lachaud, C., Lacombe, K., Marty, W., Mercier, K., Rambaud, D., Ramon, P., Rouaix, G., Schanne, S., Waegebaert, V
We present ECLAIRs, the Gamma-ray burst (GRB) trigger camera to fly on-board the Chinese-French mission SVOM. ECLAIRs is a wide-field ($\sim 2$\,sr) coded mask camera with a mask transparency of 40\% and a 1024 $\mathrm{cm}^2$ detection plane coupled
Externí odkaz:
http://arxiv.org/abs/1406.7759
Publikováno v:
Magnetohydrodynamics (0024-998X). Oct-Dec2022, Vol. 58 Issue 4, p483-490. 8p.
Autor:
Planck HFI Core Team, Ade, P. A. R., Aghanim, N., Ansari, R., Arnaud, M., Ashdown, M., Aumont, J., Banday, A. J., Bartelmann, M., Bartlett, J. G., Battaner, E., Benabed, K., Benot, A., Bernard, J. -P., Bersanelli, M., Bhatia, R., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bradshaw, T., Brelle, E., Bucher, M., Camus, P., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Charra, J., Charra, M., Chary, R. -R., Chiang, C., Church, S., Clements, D. L., Colombi, S., Couchot, F., Coulais, A., Cressiot, C., Crill, B. P., Crook, M., de Bernardis, P., Delabrouille, J., Delouis, J. -M., Désert, F. -X., Dolag, K., Dole, H., Doré, O., Douspis, M., Efstathiou, G., Eng, P., Filliard, C., Forni, O., Fosalba, P., Fourmond, J. -J., Ganga, K., Giard, M., Girard, D., Giraud-Héraud, Y., Gispert, R., Gorski, K. M., Gratton, S., Griffin, M., Guyot, G., Haissinski, J., Harrison, D., Helou, G., Henrot-Versillé, S., Hernandez-Monteagudo, C., Hildebrandt, S. R., Hills, R., Hivon, E., Hobson, M., Holmes, W. A., Huenberger, K. M., Jae, A. H., Jones, W. C., Kaplan, J., Kneissl, R., Knox, L., Lagache, G., Lamarre, J. -M., Lami, P., Lange, A. E., Lasenby, A., Lavabre, A., Lawrence, C. R., Leriche, B., Leroy, C., Longval, Y., Macas-Perez, J. F., Maciaszek, T., MacTavish, C. J., Maei, B., Mandolesi, N., Mann, R., Mansoux, B., Masi, S., Matsumura, T., McGehee, P., Melin, J. -B., Mercier, C., Miville-Deschnes, M. -A., Moneti, A., Montier, L., Mortlock, D., Murphy, A., Nati, F., Nettereld, C. B., Norgaard-Nielsen, H. U., North, C., Noviello, F., Novikov, D., Osborne, S., Paine, C., Pajot, F., Patanchon, G., Peacocke, T., Pearson, T. J., Perdereau, O., Perotto, L., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Pons, R., Ponthieu, N., Prezeau, G., Prunet, S., Puget, J. -L., Reach, W. T., Renault, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rusholme, B., Santos, D., Savini, G., Schaefer, B. M., Shellard, P., Spencer, L., Starck, J. -L., Stassi, P., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sygnet, J. -F., Tauber, J. A., Thum, C., Torre, J. -P., Touze, F., Tristram, M., Van Leeuwen, F., Vibert, L., Vibert, D., Wade, L. A., Wandelt, B. D., White, S. D. M., Wiesemeyer, H., Woodcraft, A., Yurchenko, V., Yvon, D., Zacchei, A.
The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six wide bands centered at 100, 143, 217, 353, 545 and 857 GHz at an angula
Externí odkaz:
http://arxiv.org/abs/1101.2039
Autor:
Beuermann, K., Buhlmann, J., Diese, J., Dreizler, S., Hessman, F. V., Husser, T. -O., Miller, G. -F., Nickol, N., Pons, R., Ruhr, D., Schmuelling, H., Schwope, A. D., Sorge, T., Ulrichs, L., Winget, D. E., Winget, K. I.
Planets orbiting post-common envelope binaries provide fundamental information on planet formation and evolution, especially for the yet nearly unexplored class of circumbinary planets. We searched for such planets in \odp, an eclipsing short-period
Externí odkaz:
http://arxiv.org/abs/1011.3905
Autor:
Lacombe, K., Dezalay, J-P., Houret, B., Amoros, C., Atteia, J-L., Bouchet, L., Cordier, B., Gevin, O., Godet, O., Gonzalez, F., Guillemot, Ph., Limousin, O., Pons, R., Ramon, P., Waegebaert, V.
Publikováno v:
In Astroparticle Physics December 2018 103:131-141
Autor:
Mandrou, P., Schanne, S., Cordier, B., Pons, R., Barret, D., Amoros, C., Lacombe, K., Fesquet, M., Limousin, O., Sizun, P., Lebrun, F., Gonzalez, F., Jouret, M.
The X and Gamma-ray telescope ECLAIRs is foreseen to be launched on a low Earth orbit (h=630 km, i=30 degrees) aboard the SVOM satellite (Space-based multi-band astronomical Variable Objects Monitor), a French-Chinese mission with Italian contributio
Externí odkaz:
http://arxiv.org/abs/0809.1057
Autor:
Ehanno, M., Amoros, C., Barret, D., Lacombe, K., Pons, R., Rouaix, G., Gevin, O., Limousin, O., Lugiez, F., Bardoux, A., Penquer, A.
Publikováno v:
Adv.SpaceRes.40:1259-1262,2007
We report on the development of an innovative CdTe detector plane (DPIX) optimized for the detection and localization of gamma-ray bursts in the X-ray band (below 100 keV). DPIX is part of an R&D program funded by the French Space Agency (CNES). DPIX
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701423