Zobrazeno 1 - 10
of 1 489
pro vyhledávání: '"Chauvin M"'
Autor:
Chauvin, M., Meinsohn, M.-C., Dasari, S., May, P., Iyer, S., Nguyen, N.M.P., Oliva, E., Lucchini, Z., Nagykery, N., Kashiwagi, A., Mishra, R., Maser, R., Wells, J., Bult, C.J., Mitra, A.K., Donahoe, Patricia K., Pépin, D.
Publikováno v:
In Cell Reports 25 July 2023 42(7)
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Ohashi, N., Stana, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
Publikováno v:
Nature Astronomy volume 2, pages 652-655 (2018)
Black-hole binary (BHB) systems comprise a stellar-mass black hole and a closely orbiting companion star. Matter is transferred from the companion to the black hole, forming an accretion disk, corona and jet structures. The resulting release of gravi
Externí odkaz:
http://arxiv.org/abs/1812.09907
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
The linear polarisation fraction and angle of the hard X-ray emission from the Crab provide unique insight into high energy radiation mechanisms, complementing the usual imaging, timing and spectroscopic approaches. Results have recently been present
Externí odkaz:
http://arxiv.org/abs/1802.07775
Autor:
Chauvin, M., Florén, H. -G., Friis, M., Jackson, M., Kamae, T., Kataoka, J., Kawano, T., Kiss, M., Mikhalev, V., Mizuno, T., Ohashi, N., Stana, T., Tajima, H., Takahashi, H., Uchida, N., Pearce, M.
Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expected to be linearly polarized. X-ray polarimetry provides a unique diagno
Externí odkaz:
http://arxiv.org/abs/1706.09203
Autor:
Chauvin, M., Friis, M., Jackson, M., Kawano, T., Kiss, M., Mikhalev, V., Ohashi, N., Stana, T., Takahashi, H., Pearce, M.
Polarimetric observations of celestial sources in the hard X-ray band stand to provide new information on emission mechanisms and source geometries. PoGO+ is a Compton scattering polarimeter (20-150 keV) optimised for the observation of the Crab (pul
Externí odkaz:
http://arxiv.org/abs/1703.07627
Autor:
Chauvin, M., Florén, H. -G., Jackson, M., Kamae, T., Kawano, T., Kiss, M., Kole, M., Mikhalev, V., Moretti, E., Olofsson, G., Rydström, S., Takahashi, H., Iyudin, A., Arimoto, M., Fukazawa, Y., Kataoka, J., Kawai, N., Mizuno, T., Ryde, F., Tajima, H., Takahashi, T., Pearce, M.
We have measured the linear polarisation of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the polarisation fraction and angle stands to disentangle geom
Externí odkaz:
http://arxiv.org/abs/1511.02735
Autor:
Abderrazak, M., Abolo, H., Abras, N., Aissou, M., Albertini, S., Alfonsi, P., Andre, A., Arimont, J.M., Arnalsteen, L., Atger, J., Attias, A., Aumont, O., Auvray, S., Bachmann, R., Barabino, G., Barsotti, P., Beauchesne, B., Beaupel, N., Beliard, A., Bellouard, A., Beloeil, H., Ben Salem, F., Benhamou, A., Billard, V., Binhas, M., Binot, D., Blache, J.L., Blet, A., Bongiovanni, J.P., Bonnal, A., Bonnet, M., Boret, H., Bossard, A.E., Bothereau, H., Bouarroudj, N., Bouayed, A., Bouchard, F., Boumadani, M., Bousquet, M., Bouygues, V., Bozio, G., Brek, A., Cadi, P., Caillon, P., Camerlo, A., Capito, C., Cardin, J.L., Castiglioni, M., Catinois, M.L., Cattan, P., Chambrier, C., Chambrier, G., Chapuis, O., Chauvin, M., Chokairi, S., Chopin Laly, X., Collange, V., Cotte, E., Cuellar, E., D'errico, E., Dahmani, S., Danan, M., De La Fontaine, C., De Wailly, P., Degauque, C., Delacoste, F., Denet, C., Denost, Q., Desaint, P., Descamps, E., Desfourneaux., V, Desmet, J., Desolneux, G., Dileon, S., Dolbeau, J.B., Douard, R., Dufour, F., Dupont-Bierre, E., Dupré, A., Entremont, A., Faucheron, J.L., Fernoux, P., Figuet, S., Finianos, A., Flamein, R., Fletcher, D., Fontes, J.P., Fourn, E., Gergeanu, S., Germain, A., Gignoux, B., Goater, P., Gres., P, Grigoroiu, M., Grillo, P., Guignard, B., Guinier, D., Guiot, J.L., Gutton, C., Hadjadj, H., Hail, K., Hausermann, M.H., Hennequin, S., Homsy-Hubert, B., Jambet, S., Janecki, T., Jannier-Guillou, V., Jaspart, J., Joly, F., Joris, J., Journe, F., Kattou, F., Kemoun, G., Khalaf, M., Klack, F., Kothonidis, K., Kurdi, O., Laforest, A., Lamblin, A., Lammens, S., Laporte, S., Launay-Savary, M.V., Le Maho, A.L., Lemée, J.M., Leonard, D., Leporrier, J., Lorin, J.L., Magne, E., Maisonnette, F., Malherbe, V., Manceau, G., Mariani, P., Massalou, D., Massard, J.L., Mauvais, F., Mbuyamba, J., Mbuyamba Katapile, J., Mehila, T., Meillat, H., Mergui, C., Michaud, P., Milou, F., Mirre, F., Mor Martinez, C., Mouchon, S., Mouilhade, F., Nguyen, Y.L., Ostermann Bucher, S., Page, M., Parent, S., Payen, A.L., Pedicone, R., Peluchon, P., Pichot-Delahaye, V., Piquard, A., Pirlet, I., Plard, L., Poiblanc, M., Poinas, G., Poincenot, J., Ponchel, C., Pontallier, A., Pop, R., Potiron, E., Proske, J.M., Prunet, B., Ras, E., Raspado, O., Raux, M., Regimbeau, J.M., Remue, C., Renacco, F., Riboud, R., Richard-Payen, A.L., Rio, D., Sage, M., Sage, P.Y., Saint Denis, M., Salaun, P., Samyn, B., Sbai Idrissi, M., Schmitt, G., Secq, E., Seddiki, A., Sens, N., Sirieix, D., Siriser, F., Tarcea, M., Tavernier, M., Tete, B., Theissen-Laval, O., Thevenot, A., Thievenaz, R., Vacher, B., Verhaeghe, R., Verrier, J.F., Vieuille, C., Voilin, C., Vuagnat, C., Zaepfel, S., Venara, Aurélien, Hamel, Jean-Francois, Beyer-Berjot, Laura, Vignaud, Timothée, Slim, Karem
Publikováno v:
In Surgery Open Digestive Advance June 2021 2
Autor:
Chauvin, M., Florén, H. -G., Jackson, M., Kamae, T., Kawano, T., Kiss, M., Kole, M., Mikhalev, V., Moretti, E., Olofsson, G., Rydström, S., Takahashi, H., Lind, J., Strömberg, J. -E., Welin, O., Iyudin, A., Shifrin, D., Pearce, M.
In the 50 years since the advent of X-ray astronomy there have been many scientific advances due to the development of new experimental techniques for detecting and characterising X-rays. Observations of X-ray polarisation have, however, not undergon
Externí odkaz:
http://arxiv.org/abs/1508.03345
Autor:
Chauvin, M., Jackson, M., Kawano, T., Kiss, M., Kole, M., Mikhalev, V., Moretti, E., Takahashi, H., Pearce, M.
Polarimetric studies of astrophysical sources can make important contributions to resolve the geometry of the emitting region and determine the photon emission mechanism. PoGOLite is a balloon-borne polarimeter operating in the hard X-ray band (25-24
Externí odkaz:
http://arxiv.org/abs/1505.08093
Autor:
Dacher, J.-N., Gandjbakhch, E., Taieb, J., Chauvin, M., Anselme, F., Bartoli, A., Boyer, L., Cassagnes, L., Cochet, H., Dubourg, B., Fauchier, L., Gras, D., Klug, D., Laurent, G., Mansourati, J., Marijon, E., Maury, P., Piot, O., Pontana, F., Sacher, F., Sadoul, N., Boveda, S., Jacquier, A.
Publikováno v:
In Diagnostic and Interventional Imaging September 2020 101(9):507-517