Search

Your search keyword '"Derome, L."' showing total 494 results
Start Over Author "Derome, L."

Refine your results

494 results on '"Derome, L."'

201. Virgo: a laser interferometer to detect gravitational waves

Author

Accadia, T, primary, Acernese, F, additional, Alshourbagy, M, additional, Amico, P, additional, Antonucci, F, additional, Aoudia, S, additional, Arnaud, N, additional, Arnault, C, additional, Arun, K G, additional, Astone, P, additional, Avino, S, additional, Babusci, D, additional, Ballardin, G, additional, Barone, F, additional, Barrand, G, additional, Barsotti, L, additional, Barsuglia, M, additional, Basti, A, additional, Bauer, Th S, additional, Beauville, F, additional, Bebronne, M, additional, Bejger, M, additional, Beker, M G, additional, Bellachia, F, additional, Belletoile, A, additional, Beney, J L, additional, Bernardini, M, additional, Bigotta, S, additional, Bilhaut, R, additional, Birindelli, S, additional, Bitossi, M, additional, Bizouard, M A, additional, Blom, M, additional, Boccara, C, additional, Boget, D, additional, Bondu, F, additional, Bonelli, L, additional, Bonnand, R, additional, Boschi, V, additional, Bosi, L, additional, Bouedo, T, additional, Bouhou, B, additional, Bozzi, A, additional, Bracci, L, additional, Braccini, S, additional, Bradaschia, C, additional, Branchesi, M, additional, Briant, T, additional, Brillet, A, additional, Brisson, V, additional, Brocco, L, additional, Bulik, T, additional, Bulten, H J, additional, Buskulic, D, additional, Buy, C, additional, Cagnoli, G, additional, Calamai, G, additional, Calloni, E, additional, Campagna, E, additional, Canuel, B, additional, Carbognani, F, additional, Carbone, L, additional, Cavalier, F, additional, Cavalieri, R, additional, Cecchi, R, additional, Cella, G, additional, Cesarini, E, additional, Chassande-Mottin, E, additional, Chatterji, S, additional, Chiche, R, additional, Chincarini, A, additional, Chiummo, A, additional, Christensen, N, additional, Clapson, A C, additional, Cleva, F, additional, Coccia, E, additional, Cohadon, P -F, additional, Colacino, C N, additional, Colas, J, additional, Colla, A, additional, Colombini, M, additional, Conforto, G, additional, Corsi, A, additional, Cortese, S, additional, Cottone, F, additional, Coulon, J -P, additional, Cuoco, E, additional, D'Antonio, S, additional, Daguin, G, additional, Dari, A, additional, Dattilo, V, additional, David, P Y, additional, Davier, M, additional, Day, R, additional, Debreczeni, G, additional, Carolis, G De, additional, Dehamme, M, additional, Fabbro, R Del, additional, Pozzo, W Del, additional, Prete, M del, additional, Derome, L, additional, Rosa, R De, additional, DeSalvo, R, additional, Dialinas, M, additional, Fiore, L Di, additional, Lieto, A Di, additional, Emilio, M Di Paolo, additional, Virgilio, A Di, additional, Dietz, A, additional, Doets, M, additional, Dominici, P, additional, Dominjon, A, additional, Drago, M, additional, Drezen, C, additional, Dujardin, B, additional, Dulach, B, additional, Eder, C, additional, Eleuteri, A, additional, Enard, D, additional, Evans, M, additional, Fabbroni, L, additional, Fafone, V, additional, Fang, H, additional, Ferrante, I, additional, Fidecaro, F, additional, Fiori, I, additional, Flaminio, R, additional, Forest, D, additional, Forte, L A, additional, Fournier, J -D, additional, Fournier, L, additional, Franc, J, additional, Francois, O, additional, Frasca, S, additional, Frasconi, F, additional, Freise, A, additional, Gaddi, A, additional, Galimberti, M, additional, Gammaitoni, L, additional, Ganau, P, additional, Garnier, C, additional, Garufi, F, additional, Gáspár, M E, additional, Gemme, G, additional, Genin, E, additional, Gennai, A, additional, Gennaro, G, additional, Giacobone, L, additional, Giazotto, A, additional, Giordano, G, additional, Giordano, L, additional, Girard, C, additional, Gouaty, R, additional, Grado, A, additional, Granata, M, additional, Granata, V, additional, Grave, X, additional, Greverie, C, additional, Groenstege, H, additional, Guidi, G M, additional, Hamdani, S, additional, Hayau, J -F, additional, Hebri, S, additional, Heidmann, A, additional, Heitmann, H, additional, Hello, P, additional, Hemming, G, additional, Hennes, E, additional, Hermel, R, additional, Heusse, P, additional, Holloway, L, additional, Huet, D, additional, Iannarelli, M, additional, Jaranowski, P, additional, Jehanno, D, additional, Journet, L, additional, Karkar, S, additional, Ketel, T, additional, Voet, H, additional, Kovalik, J, additional, Kowalska, I, additional, Kreckelbergh, S, additional, Krolak, A, additional, Lacotte, J C, additional, Lagrange, B, additional, Penna, P La, additional, Laval, M, additional, Marec, J C Le, additional, Leroy, N, additional, Letendre, N, additional, Li, T G F, additional, Lieunard, B, additional, Liguori, N, additional, Lodygensky, O, additional, Lopez, B, additional, Lorenzini, M, additional, Loriette, V, additional, Losurdo, G, additional, Loupias, M, additional, Mackowski, J M, additional, Maiani, T, additional, Majorana, E, additional, Magazzù, C, additional, Maksimovic, I, additional, Malvezzi, V, additional, Man, N, additional, Mancini, S, additional, Mansoux, B, additional, Mantovani, M, additional, Marchesoni, F, additional, Marion, F, additional, Marin, P, additional, Marque, J, additional, Martelli, F, additional, Masserot, A, additional, Massonnet, L, additional, Matone, G, additional, Matone, L, additional, Mazzoni, M, additional, Menzinger, F, additional, Michel, C, additional, Milano, L, additional, Minenkov, Y, additional, Mitra, S, additional, Mohan, M, additional, Montorio, J -L, additional, Morand, R, additional, Moreau, F, additional, Moreau, J, additional, Morgado, N, additional, Morgia, A, additional, Mosca, S, additional, Moscatelli, V, additional, Mours, B, additional, Mugnier, P, additional, Mul, F -A, additional, Naticchioni, L, additional, Neri, I, additional, Nocera, F, additional, Pacaud, E, additional, Pagliaroli, G, additional, Pai, A, additional, Palladino, L, additional, Palomba, C, additional, Paoletti, F, additional, Paoletti, R, additional, Paoli, A, additional, Pardi, S, additional, Parguez, G, additional, Parisi, M, additional, Pasqualetti, A, additional, Passaquieti, R, additional, Passuello, D, additional, Perciballi, M, additional, Perniola, B, additional, Persichetti, G, additional, Petit, S, additional, Pichot, M, additional, Piergiovanni, F, additional, Pietka, M, additional, Pignard, R, additional, Pinard, L, additional, Poggiani, R, additional, Popolizio, P, additional, Pradier, T, additional, Prato, M, additional, Prodi, G A, additional, Punturo, M, additional, Puppo, P, additional, Qipiani, K, additional, Rabaste, O, additional, Rabeling, D S, additional, Rácz, I, additional, Raffaelli, F, additional, Rapagnani, P, additional, Rapisarda, S, additional, Re, V, additional, Reboux, A, additional, Regimbau, T, additional, Reita, V, additional, Remilleux, A, additional, Ricci, F, additional, Ricciardi, I, additional, Richard, F, additional, Ripepe, M, additional, Robinet, F, additional, Rocchi, A, additional, Rolland, L, additional, Romano, R, additional, Rosińska, D, additional, Roudier, P, additional, Ruggi, P, additional, Russo, G, additional, Salconi, L, additional, Sannibale, V, additional, Sassolas, B, additional, Sentenac, D, additional, Solimeno, S, additional, Sottile, R, additional, Sperandio, L, additional, Stanga, R, additional, Sturani, R, additional, Swinkels, B, additional, Tacca, M, additional, Taddei, R, additional, Taffarello, L, additional, Tarallo, M, additional, Tissot, S, additional, Toncelli, A, additional, Tonelli, M, additional, Torre, O, additional, Tournefier, E, additional, Travasso, F, additional, Tremola, C, additional, Turri, E, additional, Vajente, G, additional, Brand, J F J van den, additional, Broeck, C Van Den, additional, Putten, S van der, additional, Vasuth, M, additional, Vavoulidis, M, additional, Vedovato, G, additional, Verkindt, D, additional, Vetrano, F, additional, Véziant, O, additional, Viceré, A, additional, Vinet, J -Y, additional, Vilalte, S, additional, Vitale, S, additional, Vocca, H, additional, Ward, R L, additional, Was, M, additional, Yamamoto, K, additional, Yvert, M, additional, Zendri, J -P, additional, and Zhang, Z, additional

Published
2012
Full Text
View/download PDF

203. Design and construction of a Cherenkov imager for charge measurement of nuclear cosmic rays

Author

Bourrion, O, primary, Bernard, C, additional, Bondoux, D, additional, Bouly, J L, additional, Bouvier, J, additional, Boyer, B, additional, Brinet, M, additional, Buenerd, M, additional, Damieux, G, additional, Derome, L, additional, Eraud, L, additional, Foglio, R, additional, Fombaron, D, additional, Grondin, D, additional, Lee, M H, additional, Lutz, L, additional, Marton, M, additional, Menchaca-Rocha, A, additional, Pelissier, A, additional, Périé, J N, additional, Putze, A, additional, Roudier, S, additional, Sallaz-Damaz, Y, additional, Seo, E S, additional, Scordilis, J P, additional, and Yoon, Y S, additional

Published
2011
Full Text
View/download PDF

204. STATUS AND RECENT RESULTS FROM THE CREAM EXPERIMENT

Author

SEO, E. S., primary, AHN, H. S., additional, BHOYAR, P., additional, EATON, J., additional, GANEL, O., additional, HAN, J. H., additional, HAQUE, A., additional, KIM, K. C., additional, KIM, M. H., additional, LEE, M. H., additional, LEE, S. E., additional, LUTZ, L., additional, MALININ, A., additional, OFOHA, O., additional, RYU, S. S., additional, SMITH, B. P., additional, VARTANYAN, A., additional, WALPOLE, P., additional, WU, J., additional, YOO, J. H., additional, YOON, Y. S., additional, ANDERSON, T., additional, CONKLIN, N. B., additional, COUTU, S., additional, GESKE, M., additional, MOGNET, S. I., additional, BARBIER, L., additional, LINK, J. T., additional, MITCHELL, J. W., additional, BARRAU, A., additional, BUÉNERD, M., additional, COSTE, B., additional, DEROME, L., additional, MANGIN-BRINET, M., additional, PUTZE, A., additional, SALLAZ-DAMAZ, Y., additional, BAZER-BACHI, R., additional, BEATTY, J. J., additional, BRANDT, T. J., additional, BIGONGIARI, G., additional, MAESTRO, P., additional, ZEI, R., additional, JEON, J. A., additional, NA, G., additional, NAM, J., additional, NAM, S., additional, PARK, I. H., additional, PARK, N. H., additional, YANG, J., additional, MENCHACA-ROCHA, A., additional, and NUTTER, S., additional

Published
2011
Full Text
View/download PDF

210. Approaching the Spectral Knee in High Energy Cosmic Rays with CREAM

Author

S. Seo, E., primary, S. Ahn, H., additional, Allison, P., additional, Anderson, T., additional, G. Bagliesi, M., additional, Barbier, L., additional, Barrau, A., additional, Bazer-Bachi, R., additional, J. Beatty, J., additional, Bigongiari, G., additional, Bhoyar, P., additional, Boyle, P., additional, T. Brandt, T., additional, Buénerd, M., additional, B. Conklin, N., additional, Coutu, S., additional, Derome, L., additional, A. DuVernois, M., additional, Ganel, O., additional, Geske, M., additional, H. Han, J., additional, A. Jeon, J., additional, C. Kim, K., additional, H. Lee, M., additional, Link, J., additional, Lutz, L., additional, Malinin, A., additional, Mangin-Brinet, M., additional, S. Marrocchesi, P., additional, Maestro, P., additional, Menchaca-Rocha, A., additional, W. Mitchell, J., additional, I. Mognet, S., additional, Na, G., additional, Nam, S., additional, Nutter, S., additional, H. Park, I., additional, H. Park, N., additional, Putze, A., additional, Sallaz-Damaz, Y., additional, Swordy, S., additional, Wakely, S., additional, Walpole, P., additional, Wu, J., additional, Yang, J., additional, S. Yoon, Y., additional, Zei, R., additional, and Y. Zinn, S., additional

Published
2009
Full Text
View/download PDF

211. CHERCAM: The Cherenkov imager of the CREAM experiment

Author

Sallaz-Damaz, Y., primary, Barrau, A., additional, Bazer-Bachi, R., additional, Bourrion, O., additional, Bouvier, J., additional, Boyer, B., additional, Buénerd, M., additional, Derome, L., additional, Eraud, L., additional, Foglio, R., additional, Gallin-Martel, L., additional, Ganel, O., additional, Han, J.H., additional, Kim, K.C., additional, Lee, M.H., additional, Lutz, L., additional, Mangin-Brinet, M., additional, Malinine, A., additional, Menchaca-Rocha, A., additional, Périé, J.N., additional, Putze, A., additional, Scordilis, J.-P., additional, Seo, E.S., additional, Walpole, P., additional, Yoo, J.H., additional, Yoon, Y.S., additional, and Zinn, S.Y., additional

Published
2008
Full Text
View/download PDF

212. CHERCAM: a Cherenkov imager for the CREAM experiment

Author

BRINET, M., primary, BARRAU, A., additional, BOURRION, O., additional, BOUVIER, J., additional, BOYER, B., additional, BUENERD, M., additional, DEROME, L., additional, ERAUD, L., additional, FOGLIO, R., additional, GALLIN-MARTEL, L., additional, PUTZE, A., additional, SALLAZ-DAMAZ, Y., additional, SCORDILIS, J.-P., additional, BHOYAR, P., additional, GANEL, O., additional, HAN, J. H., additional, KIM, C. H., additional, LEE, M. H., additional, LUTZ, L., additional, MALININE, A., additional, SEO, E. S., additional, WALPOLE, P., additional, YOON, Y. S., additional, ZINN, S. Y., additional, BAZER-BACHI, R., additional, PERIE, J. N., additional, and MENCHACA-ROCHA, A., additional

Published
2008
Full Text
View/download PDF

213. Approaching the Knee with Direct Measurements

Author

Seo, E.S., primary, Ahn, H.S., additional, Allison, P., additional, Bagliesi, M.G., additional, Barbier, L., additional, Barrau, A., additional, Bazer-Bachi, R., additional, Beatty, J.J., additional, Bigongiari, G., additional, Boyle, P., additional, Brandt, T.T., additional, Buénerd, M., additional, Childers, J.T., additional, Conklin, N.B., additional, Coutu, S., additional, Derome, L., additional, DuVernois, M.A., additional, Ganel, O., additional, Han, J.H., additional, Jeon, J.A., additional, Kim, K.C., additional, Lee, M.H., additional, Lutz, L., additional, Malinin, A., additional, Mangin-Brinet, M., additional, Marrocchesi, P.S., additional, Maestro, P., additional, Menchaca-Rocha, A., additional, Minnick, S., additional, Mognet, S.I., additional, Nam, S.W., additional, Nutter, S., additional, Park, I.H., additional, Park, N.H., additional, Putze, A., additional, Sallaz-Damaz, Y., additional, Sina, R., additional, Swordy, S., additional, Wakely, S., additional, Walpole, P., additional, Wu, J., additional, Yang, J., additional, Yoon, Y.S., additional, Zei, R., additional, and Zinn, S.Y., additional

Published
2008
Full Text
View/download PDF

214. Origin of the high energy proton component below the geomagnetic cutoff in near earth orbit

Author

Derome, L., Buenerd, M., Barrau, A., Bouchet, A., Menchaca-Rocha, A., Thuillier, T., Derome, L., Buenerd, M., Barrau, A., Bouchet, A., Menchaca-Rocha, A., and Thuillier, T.

Abstract

The high flux proton component observed by AMS below the geomagnetic cutoff can be well accounted for by assuming these particles to be secondaries originating from the interaction of Cosmic Ray protons with the atmosphere. Simulation results are reported, Comment: 7 pages, Latex, 4 Postscript figures. Final version (minor corrections) for Physics Letters. B

Published
2000
Full Text
View/download PDF

215. CHERCAM: A Cherenkov imager for the CREAM experiment

Author

Mangin-Brinet, M., primary, Barrau, A., additional, Bazer-Bachi, R., additional, Bourrion, O., additional, Bouvier, J., additional, Boyer, B., additional, Buénerd, M., additional, Derome, L., additional, Eraud, L., additional, Foglio, R., additional, Gallin-Martel, L., additional, Ganel, O., additional, Kim, C.H., additional, Lutz, L., additional, Malinine, A., additional, Menchaca-Rocha, A., additional, Périé, J.N., additional, Sallaz-Damaz, Y., additional, Scordilis, J.-P., additional, Seo, E.S., additional, Walpole, P., additional, and Zinn, S.Y., additional

Published
2007
Full Text
View/download PDF

217. Prototype study of the Cherenkov imager of the AMS experiment

Author

Aguayo, P., primary, Aguilar-Benitez, M., additional, Arruda, L., additional, Barao, F., additional, Barreira, G., additional, Barrau, A., additional, Baret, B., additional, Belmont, E., additional, Berdugo, J., additional, Boudoul, G., additional, Borges, J., additional, Buénerd, M., additional, Casadei, D., additional, Casaus, J., additional, Delgado, C., additional, Diaz, C., additional, Derome, L., additional, Eraud, L., additional, Gallin-Martel, L., additional, Giovacchini, F., additional, Goncalves, P., additional, Lanciotti, E., additional, Laurenti, G., additional, Malinine, A., additional, Mañá, C., additional, Marín, J., additional, Martinez, G., additional, Menchaca-Rocha, A., additional, Palomares, C., additional, Pereira, R., additional, Pimenta, M., additional, Protasov, K., additional, Sanchez, E., additional, Seo, E.-S., additional, Sevilla, I., additional, Torrentó, A., additional, Vargas-Trevino, M., additional, and Véziant, O., additional

Published
2006
Full Text
View/download PDF

218. Improvement in the shot noise of a laser interferometer gravitational wave detector by means of an output mode-cleaner

Author

Beauville, F, primary, Buskulic, D, additional, Derome, L, additional, Dominjon, A, additional, Flaminio, R, additional, Hermel, R, additional, Marion, F, additional, Masserot, A, additional, Massonnet, L, additional, Mours, B, additional, Moreau, F, additional, Mugnier, P, additional, Ramonet, J, additional, Tournefier, E, additional, Verkindt, D, additional, Veziant, O, additional, and Yvert, M, additional

Published
2006
Full Text
View/download PDF

220. In-beam tests of the AMS RICH prototype with secondary ions

Author

Baret, B, primary, Aguayo, P, additional, Aguilar Benitez, M, additional, Arruda, L, additional, Barao, F, additional, Barrau, A, additional, Belmont, E, additional, Berdugo, J, additional, Boudoul, G, additional, Borges, J, additional, Buénerd, M, additional, Casadei, D, additional, Casaus, J, additional, Delgado, C, additional, Diaz, C, additional, Derome, L, additional, Eraud, L, additional, Gallin-Martel, L, additional, Giovacchini, F, additional, Goncalves, P, additional, Lanciotti, E, additional, Laurenti, G, additional, Malinine, A, additional, Mana, C, additional, Marin, J, additional, Martinez, G, additional, Menchaca-Rocha, A, additional, Palomares, C, additional, Pimenta, M, additional, Protasov, K, additional, Sanchez, E, additional, Seo, E-S, additional, Sevilla, I, additional, Torrento, A, additional, and Vargas-Trevino, M, additional

Published
2004
Full Text
View/download PDF

227. Injury and death of various Salmonellaserotypes due to acidic conditions

Author

Cox, N.A., Richardson, K.E., Cosby, D.E., Berrang, M.E., Cason, J.A., Rigsby, L.L., Holcombe, N., and DeRome, L.

Abstract

Acid injury could prevent detection of Salmonellain feed and feed-type samples. A previous study showed that after incubation in commonly used pre-enrichment media, mixed feeds and feed ingredients reached a pH (4.0 to 5.0), capable of injuring or killing Salmonella. Approximately 105colony forming units (CFU) of S.Enteritidis (SE), S.Heidelberg (SH), S.Kentucky (SK), or S.Typhimurium (ST) were individually placed into 50 mL of a citrate buffer at pH of 4, 4.5, or 5.0 for 6 or 24 h at 37°C. After holding at 37°C, each serotype was serially diluted in sterile physiological saline and plated onto xylose lysine tergitol 4 [for injury] and nutrient agar (NA) [for death]. These plates were enumerated and percent injury and/or death determined. The injury and death confirmed that pH 4.0 was detrimental to these Salmonellaserotypes. After 24 h at pH 4.0, 60% or more of all 4 serotypes were killed with 100% of S.Kentucky killed. At pH 5.0, 65 to 75% of these organisms were uninjured, with death between 15 to 20%. Researchers testing feed/feed ingredients for Salmonellamay not be aware of the acidic nature of the pre-enrichment step and the subsequent injury or death of any Salmonellapresent, whether healthy or stressed. Current protocols that are considered the “gold standard” may not be detecting Salmonellain samples containing fermentable substrates and extraneous microorganisms, which prevent the accurate detection of Salmonella.Injury or death of a few Salmonellacells could reduce the chance of recovery from any sample. More research is needed with additional Salmonellaserotypes and strains to fully understand the challenges of isolating Salmonellafrom feed.

Published
2016
Full Text
View/download PDF

231. Correction to: High precision particle astrophysics as a new window on the universe with an Antimatter Large Acceptance Detector In Orbit (ALADInO).

Author

Battiston, R., Bertucci, B., Adriani, O., Ambrosi, G., Baudouy, B., Blasi, P., Boezio, M., Campana, D., Derome, L., De Mitri, I., Di Felice, V., Donato, F., Duranti, M., Formato, V., Grasso, D., Gebauer, I., Iuppa, R., Masi, N., Maurin, D., and Mazziotta, M. N.

Subjects
ANTIMATTER, ASTROPHYSICS, DETECTORS
Abstract

A Correction to this paper has been published: https://doi.org/10.1007/s10686-021-09771-3 [ABSTRACT FROM AUTHOR]

Published
2021
Full Text
View/download PDF

232. A VME based CCD imaging system for the VIRGO interferometer control

Author

Bellachia, F, primary, Boget, D, additional, Carron, T, additional, Castelazzi, D, additional, Daguin, G, additional, Derome, L, additional, Drezen, C, additional, Flaminio, R, additional, Grave, X, additional, Lacotte, J.C, additional, Marion, F, additional, Massonnet, L, additional, Morand, R, additional, Mours, B, additional, Sannibale, V, additional, and Verkindt, D, additional

Published
1998
Full Text
View/download PDF

233. Status and noise limit of the VIRGO antenna

Author

Gammaitoni, L., primary, Babusci, D., additional, Fang, H., additional, Giordano, G., additional, Iannarelli, M., additional, Matone, G., additional, Turri, E., additional, Mazzoni, M., additional, Stanga, R., additional, Calloni, E., additional, Cavaliere, S., additional, Di Fiore, L., additional, Evangelista, G., additional, Garifi, F., additional, Grado, A., additional, Milano, L., additional, Solimeno, S., additional, Cagnoli, G., additional, Cattuto, C., additional, Kovalik, J., additional, Marchesoni, F., additional, Punturo, M., additional, Bernardini, M., additional, Bozzi, A., additional, Braccini, S., additional, Bradaschia, C., additional, Casciano, C., additional, Cella, G., additional, Ciampa, A., additional, Cuoco, E., additional, Curci, G., additional, D’Ambrosio, E., additional, Dattilo, V., additional, De Carolis, G., additional, De Salvo, R., additional, Di Virgilio, A., additional, Enard, D., additional, Errico, A., additional, Feng, G., additional, Ferrante, I., additional, Fidecaro, F., additional, Frasconi, F., additional, Gaddi, A., additional, Gennai, A., additional, Gennaro, G., additional, Giazotto, A., additional, La Penna, P., additional, Losurdo, G., additional, Maggiore, M., additional, Mancini, S., additional, Palla, F., additional, Pan, H. B., additional, Paoletti, F., additional, Pasqualetti, A., additional, Passaquieti, R., additional, Passuello, D., additional, Poggiani, R., additional, Popolizio, P., additional, Raffaelli, F., additional, Rapisarda, S., additional, Taddei, R., additional, Vicere, A., additional, Zhang, Z., additional, Astone, P., additional, Bronzini, F., additional, Frasca, S., additional, Majorana, E., additional, Palomba, C., additional, Perciballi, M., additional, Puppo, P., additional, Rapagnani, P., additional, Ricci, F., additional, Boccara, C., additional, Daban, J. B., additional, Leliboux, M., additional, Loriette, V., additional, Nahoum, R., additional, Roger, J-P., additional, Ganau, P., additional, Lagrange, B., additional, Mackowski, J. M., additional, Michel, C., additional, Morgago, N., additional, Pinard, L., additional, Remillieux, A., additional, Arnault, C., additional, Barrand, C., additional, Beney, J-L., additional, Bilhaut, R., additional, Brisson, V., additional, Cavalier, F., additional, Chiche, R., additional, Coulon, J-P., additional, Cuzon, S., additional, Davier, M., additional, Dehamme, M., additional, Dialinas, M., additional, Eder, C., additional, Gaspard, M., additional, Hello, P., additional, Heusse, P., additional, Hrisoho, A., additional, Jules, E., additional, Marrucho, J-C., additional, Mencik, M., additional, Marin, P., additional, Matone, L., additional, Reboux, A., additional, Roudier, P., additional, Taurigna, M., additional, Bellachia, F., additional, Bermond, M., additional, Boget, D., additional, Caron, B., additional, Carron, T., additional, Castellazzi, D., additional, Chollet, F., additional, Daguin, G., additional, David, P-Y., additional, Derome, L., additional, Drezen, C., additional, Dufournaud, D., additional, Flamino, R., additional, Giacobone, L., additional, Girard, C., additional, Grave, X., additional, Hermel, R., additional, Lacotte, J-C., additional, Le Marec, J-C., additional, Lieunard, B., additional, Marion, F., additional, Massonnet, L., additional, Mehmel, C., additional, Morand, R., additional, Mours, B., additional, Mugnier, P., additional, Sannibale, V., additional, Sottile, R., additional, Verkindt, D., additional, Yvert, M., additional, Acker, Y., additional, Barillet, R., additional, Barsuglia, M., additional, Berthet, J-P., additional, Brillet, A., additional, Cachenaut, J., additional, Cleva, F., additional, Heitmann, H., additional, Innocent, J-M., additional, Lucenay, J-C., additional, Man, N. C., additional, Manh, P-T., additional, Marck, J-A., additional, Pelat, D., additional, Reita, V., additional, and Vinet, J-Y., additional

Published
1998
Full Text
View/download PDF

234. Constraining Galactic cosmic-ray parameters with Z ⩽2 nuclei.

Author

Coste, B., Derome, L., Maurin, D., and Putze, A.

Subjects
*GALACTIC cosmic rays, *MARKOV chain Monte Carlo, *PROBABILITY density function, *ASTROPHYSICS, *INTERSTELLAR medium
Abstract

Context. The secondary-to-primary B/C ratio is widely used for studying Galactic cosmic-ray propagation processes. The 2H/4He and 3He/4He ratios probe a different Z/A regime, which provides a test for the "universality" of propagation. Aims. We revisit the constraints on diffusion-model parameters set by the quartet (1H, 2H, 3He, 4He), using the most recent data as well as updated formulae for the inelastic and production cross-sections. Methods. Our analysis relies on the USINE propagation package and a Markov Chain Monte Carlo technique to estimate the probability density functions of the parameters. Simulated data were also used to validate analysis strategies. Results. The fragmentation of CNO cosmic rays (resp. NeMgSiFe) on the interstellar medium during their propagation contributes to 20% (resp. 20%) of the 2H and 15% (resp. 10%) of the 3He flux at high energy. The C to Fe elements are also responsible for up to 10% of the 4He flux measured at 1 GeV/n. The analysis of 3He/4He (and to a lesser extent 2H/4He) data shows that the transport parameters are consistent with those from the B/C analysis: the diffusion model with δ ~ 0.7 (diffusion slope), Vc ~ 20 km s-1 (galactic wind), Va ~ 40 km s-1 (reacceleration) is favoured, but the combination δ ~ 0.2, Vc ~ 0, and Va ~ 80 km s-1 is a close second. The confidence intervals on the parameters show that the constraints set by the quartet data can compete with those derived from the B/C data. These constraints are tighter when adding the 3He (or 2H) flux measurements, and the tightest when the He flux is added as well. For the latter, the analysis of simulated and real data shows an increased sensitivity to biases. Using the secondary-toprimary ratio along with a loose prior on the source parameters is recommended to obtain the most robust constraints on the transport parameters. Conclusions. Light nuclei should be systematically considered in the analysis of transport parameters. They provide independent constraints that can compete with those obtained from the B/C analysis. [ABSTRACT FROM AUTHOR]

Published
2012
Full Text
View/download PDF

235. Characterization study of silica aerogel for Cherenkov imaging

Author

Sallaz-Damaz, Y., Derome, L., Mangin-Brinet, M., Loth, M., Protasov, K., Putze, A., Vargas-Trevino, M., Véziant, O., Buénerd, M., Menchaca-Rocha, A., Belmont, E., Vargas-Magaña, M., Léon-Vargas, H., Ortiz-Velàsquez, A., Malinine, A., Baraõ, F., Pereira, R., Bellunato, T., Matteuzzi, C., and Perego, D.L.

Subjects
*CHERENKOV counters, *SILICA gel, *CHERENKOV radiation, *REFRACTIVE index, *LASER beams, *COSMIC rays
Abstract

Abstract: Different methods to measure the characteristics of silica aerogel tiles used as Cherenkov radiator in the CREAM and AMS experiments have been investigated to optimize the detector performances. The measurement accuracy dictated by the physics objectives on the velocity and charge resolutions set stringent requirements on the aerogel refractive index determination, namely and for the AMS and CREAM imagers, respectively. The matching of such accuracies for this material turned out to be a metrological challenge, and finally led to a full R&D program, to develop an appropriate characterization procedure. Preliminary studies performed with a standard refractive index measurement technique (laser beam deviation by a prism) have revealed a significant systematic index nonuniformity for the AMS tiles at a level , not acceptable considering the aimed accuracy. These large variations were confirmed in a beam test. A second method, mapping the transverse index gradient by deflection of a laser beam entering normally to the tile has then been developed. It is shown that this procedure is suitable to reach the required accuracy, at the price of using both methods combined. The several hundreds of tiles of the radiator plane of the CREAM and AMS Cherenkov imagers were characterized using a simplified procedure, however, appropriate for each case, compromising between the amount of work and the time available. The experimental procedures and set-ups used are described in the text, and the obtained results are reported. [Copyright &y& Elsevier]

Published
2010
Full Text
View/download PDF

236. Risks management and sanitary vigilances coordination

Author

Steclebout-Derome, L., Poullain, I., and Quaranta, J.-F.

Subjects
*RISK management in business, *SANITATION
Abstract

In application of the statutory texts, health care centres undertook in the implementation of the devices of sanitary attentiveness, which participate in the same objective of security and quality of the care but work according to different modalities. Besides, the reflection turns to a voluntary movement of management of all the risks being able to arise within an establishment of health. It settles for objectives to reduce the frequency of arisen the unwanted events, to prevent of it the incidence and to minimize the harmful consequences. Since 1998, numerous hospitals dashed into a method of coordination of the sanitary attentivenesses and the management of the risks with as main objectives: the correspondence in repository Quality and Prevention of the Risks, Sanitary Attentivenesses and Security Transfusionnelle and Prevention of the Infectious Risk of the manual worker of accreditation of the National Agency of Accreditation and Evaluation in Health, the implementation of a dynamics of continuous improvement of the quality and the prevention of the risks. The coordination of the sanitary attentivenesses and the prevention of the risks participates in the stage of identification of a certain number of risks connected to the products of health and to their use. In partnership with the other structures of the establishment, it represents the driving element of a real coverage of the risks to the hospital and to their prevention. [Copyright &y& Elsevier]

Published
2002
Full Text
View/download PDF

237. Flux of light antimatter nuclei near Earth.

Author

Baret, B., Barrau, A., Boudoul, G., Buénerd, M., Derome, L., Duperray, R., Maurin, D., Protasov, K., and Vratogna, S.

Subjects
INTERSTELLAR medium, GALAXIES, INELASTIC scattering, COSMIC rays, ANTIMATTER
Abstract

The fluxes of light antinuclei A≤ 4 induced near earth by Cosmic Ray (CR) interactions with the interstellar matter (ISM) in the Galaxy are calculated in a phenomenological framework. The hadronic production cross-section for antinucleons is based on a recent parametrization of a wide set of accelerator data. The production of light nuclei is calculated using coalescence models. The non annihilating inelastic scattering process for the antideuterons is discussed and taken into account for the first time via a more realistic procedure than used so far for antiprotons. © 2006 American Institute of Physics [ABSTRACT FROM AUTHOR]

Published
2006
Full Text
View/download PDF

238. Takayasu's disease. A case report with angiographic demonstration

Author

Mignault Jde L, Derome L, Roy P, and Tardif L

Subjects
Adult, medicine.medical_specialty, business.industry, Aortic Arch Syndromes, General surgery, Angiography, 030204 cardiovascular system & hematology, 03 medical and health sciences, 0302 clinical medicine, Medicine, Humans, Takayasu's disease, 030212 general & internal medicine, Cardiology and Cardiovascular Medicine, business
Published
1965

241. The AMS-RICH prototype: Test beam results

Author

Aguayo, P., Arruda, L., Fernando Barao, Barrau, A., Baret, B., Belmont, E., Berdugo, J., Boudoul, G., Borges, J., Buenerd, M., Casadei, D., Casaus, J., Delgado, C., Diaz, C., Derome, L., Eraud, L., Gallin-Martel, L., Giovacchini, F., Goncalves, P., Lanciotti, E., Laurenti, G., Malinine, A., Mana, C., Marin, J., Martinez, G., Menchaca-Rocha, A., Palomares, C., Protasov, K., Sanchez, E., Seo, E. -S, Sevilla, I., Torrento, A., Vargas-Trevino, M., and Veziant, O.

242. The Ring Imaging Cherenkov detector (RICH) of the AMS experiment

Author

Aguilar Benitez, M., Alcaraz, J., Arruda, L., Barao, F., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Brinet, M., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Delgado, C., Diaz, C., Derome, L., Eraud, L., Garcia-Lopez, R. J., Gallin-Martel, L., Giovacchini, F., Goncalves, P., Lanciotti, E., Laurenti, G., Malinine, A., Mana, C., Marin, J., Martinez, G., Menchaca-Rocha, A., Mercedes Mollá Lorente, Palomares, C., Panniello, M., Pereira, R., Pimenta, M., Protasov, K., Sanchez, E., Seo, E-S, Sevilla, N., Torrento, A., Vargas-Trevino, M., Veziant, O., and Tata Institut Fundamental Res

243. Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer

Author

Aguilar, M., Ali Cavasonza, L., Ambrosi, G., Arruda, L., Attig, N., Bachlechner, A., Barao, F., Barrau, A., Barrin, L., Bartoloni, A., Başeğmez-Du Pree, S., Battiston, R., Becker, U., Behlmann, M., Beischer, B., Berdugo, J., Bertucci, B., Bindi, V., De Boer, W., Bollweg, K., Borgia, B., Boschini, M. J., Bourquin, M., Bueno, E. F., Burger, J., Burger, W. J., Cai, X. D., Capell, M., Caroff, S., Casaus, J., Castellini, G., Cervelli, F., Chang, Y. H., Chen, G. M., Chen, H. S., Chen, Y., Cheng, L., Chou, H. Y., Choutko, V., Chung, C. H., Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., Dai, Y. M., Datta, A., Delgado, C., Della Torre, S., Demirköz, M. B., Derome, L., Di Falco, S., Di Felice, V., Díaz, C., Dimiccoli, F., Von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Galaktionov, Y., Gámez, C., García-López, R. J., Gargiulo, C., Gast, H., Gebauer, I., Gervasi, M., Giovacchini, F., Gómez-Coral, D. M., Gong, J., Goy, C., Grabski, V., Grandi, D., Graziani, M., Guo, K. H., Haino, S., Han, K. C., He, Z. H., Hsieh, T. H., Huang, H., Huang, Z. C., Incagli, M., Jang, W. Y., Jia, Yi, Jinchi, H., Kanishev, K., Khiali, B., Kim, G. N., Kirn, Th., Konyushikhin, M., Kounina, O., Kounine, A., Koutsenko, V., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., Lazzizzera, I., Lebedev, A., Lee, H. T., Lee, S. C., Li, J. Q., Li, Q., Li, T. X., Li, Z. H., Light, C., Lin, C. H., Lippert, T., Liu, Z., Lu, S. Q., Lu, Y. S., Luebelsmeyer, K., Luo, F., Luo, J. Z., Luo, Xi, Lyu, S. S., Machate, F., Mañá, C., Marín, J., Martin, T., Martínez, G., Masi, N., Maurin, D., Menchaca-Rocha, A., Meng, Q., Mo, D. C., Molero, M., Mott, P., Mussolin, L., Nelson, T., Ni, J. Q., Nikonov, N., Nozzoli, F., Oliva, A., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Phan, H. D., Plyaskin, V., Poireau, V., Poluianov, S., Popkow, A., Qi, X. M., Qin, X., Qu, Z. Y., Quadrani, L., Rancoita, P. G., Rapin, D., Reina Conde, A., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, S., Schmidt, S. M., Schulz Von Dratzig, A., Schwering, G., Seo, E. S., Shan, B. S., Shi, J. Y., Siedenburg, T., Solano, C., Song, J. W., Sun, Z. T., Tacconi, M., Tang, X. W., Tang, Z. C., Tian, J., Ting, Samuel C. C., Ting, S. M., Tomassetti, N., Torsti, J., Tüysüz, C., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valente, E., Valtonen, E., Vázquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J. P., Wang, L. Q., Wang, N. H., Wang, Q. L., Wang, X., Wang, X. Q., Wang, Z. X., Wei, J., Weng, Z. L., Wu, H., Xiong, R. Q., Xu, W., Yan, Q., Yang, Y., Yi, H., Yu, Y. J., Yu, Z. Q., Zannoni, M., Zeissler, S., Zhang, C., Zhang, F., Zhang, J. H., Zhang, Z., Zhao, F., Zheng, Z. M., Zhuang, H. L., Zhukov, V., Zichichi, A., Zimmermann, N., and Zuccon, P.

Subjects
3. Good health

244. The ring imaging Cerenkov detector (rich) of the ams experiment

Author

Barao, Fernando, Aguilar Benitez, M., Alcaraz, J., Arruda, L., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Brinet, M., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Delgado, C., Diaz, C., Derome, L., Eraud, L., Garcia-Lopez, R. J., Gallin-Martel, L., Giovacchini, F., Goncalves, P., Lanciotti, E., Laurenti, G., Malinine, A., Mana, C., Marin, J., Martinez, G., Menchaca-Rocha, A., Molla, M., Palomares, C., Panniello, M., Rui Pereira, Pimenta, M., Protasov, K., Sanchez, E., Seo, E-S, Sevilla, N., Torrento, A., Vargas-Trevino, M., and Veziant, O.

245. The AMS-RICH velocity and charge reconstruction

Author

Aguilar-Benitez, M., Arruda, L., Barao, F., Baret, B., Barrau, A., Barreira, G., Belmont, E., Berdugo, J., Borges, J., Buenerd, M., Casadei, D., Casaus, J., Cortina, E., Costado, M., Crespo, D., Delgado, C., Diaz, C., Derome, L., Goncalves, P., Garcialopez, R., La Guia, C., Herrero, A., Lanciotti, E., Laurenti, G., Malinin, A., Mana, C., Jesus Marin, Mangin-Brinet, M., Martinez, G., Menchaca-Rocha, A., Palomares, C., Pereira, R., Pimenta, M., Putze, A., Sallaz-Damaz, Y., Se, Es, Sevilla, I., Torrento, A., Vargas-Trevino, M., Veziant, O., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia, AMS, bibliotheque, LPSC, and Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Instrumentation and Detectors, Astrophysics (astro-ph), FOS: Physical sciences, High Energy Physics::Experiment, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], Astrophysics
Abstract

The AMS detector, to be installed on the International Space Station, includes a Ring Imaging Cerenkov detector with two different radiators, silica aerogel (n=1.05) and sodium fluoride (n=1.334). This detector is designed to provide very precise measurements of velocity and electric charge in a wide range of cosmic nuclei energies and atomic numbers. The detector geometry, in particular the presence of a reflector for acceptance purposes, leads to complex Cerenkov patterns detected in a pixelized photomultiplier matrix. The results of different reconstruction methods applied to test beam data as well as to simulated samples are presented. To ensure nominal performances throughout the flight, several detector parameters have to be carefully monitored. The algorithms developed to fulfill these requirements are presented. The velocity and charge measurements provided by the RICH detector endow the AMS spectrometer with precise particle identification capabilities in a wide energy range. The expected performances on light isotope separation are discussed., Contribution to the ICRC07, Merida, Mexico (2007); Presenter: F. Barao

246. Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer

Author

Aguilar, M., Cavasonza, L. A., Allen, M. S., Alpat, B., Ambrosi, G., Arruda, L., Attig, N., Barao, F., Barrin, L., Bartoloni, A., Başeǧmez-Du Pree, S., Battiston, R., Behlmann, M., Beranek, B., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Borgia, B., Boschini, M. J., Bourquin, M., Bueno, E. F., Burger, J., Burger, W. J., Burmeister, S., Cai, X. D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y. H., Chen, G. M., Chen, G. R., Chen, H. S., Chen, Y., Cheng, L., Chou, H. Y., Chouridou, S., Choutko, V., Chung, C. H., Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., Delgado, C., Della Torre, S., Demirköz, M. B., Derome, L., Di Falco, S., Di Felice, V., Díaz, C., Dimiccoli, F., Von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Freeman, C., Galaktionov, Y., Gámez, C., García-López, R. J., Gargiulo, C., Gast, H., Gervasi, M., Giovacchini, F., Gómez-Coral, D. M., Gong, J., Goy, C., Grabski, V., Grandi, D., Graziani, M., Haino, S., Han, K. C., Hashmani, R. K., He, Z. H., Heber, B., Hsieh, T. H., Hu, J. Y., Incagli, M., Jang, W. Y., Jia, Y., Jinchi, H., Kanishev, K., Khiali, B., Kim, G. N., Kirn, T., Konyushikhin, M., Kounina, O., Kounine, A., Koutsenko, V., Kuhlman, A., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., Lazzizzera, I., Lebedev, A., Lee, H. T., Lee, S. C., Li, J. Q., Li, M., Li, Q., Li, S., Li, J. H., Li, Z. H., Liang, J., Light, C., Lin, C. H., Lippert, T., Liu, J. H., Liu, Z., Lu, S. Q., Lu, Y. S., Luebelsmeyer, K., Luo, J. Z., Luo, X., Lyu, S. S., Machate, F., Mañá, C., Marín, J., Marquardt, J., Martin, T., Martínez, G., Masi, N., Maurin, D., Menchaca-Rocha, A., Meng, Q., Mikhailov, V. V., Mo, D. C., Molero, M., Mott, P., Mussolin, L., Negrete, J., Nikonov, N., Nozzoli, F., Oliva, A., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Phan, H. D., Piandani, R., Plyaskin, V., Poluianov, S., Qin, X., Qu, Z. Y., Quadrani, L., Rancoita, P. G., Rapin, D., Conde, A. R., Robyn, E., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, S., Schulz Von Dratzig, A., Schwering, G., Seo, E. S., Shakfa, Z., Shan, B. S., Siedenburg, T., Solano, C., Song, J. W., Song, X. J., Sonnabend, R., Strigari, L., Su, T., Sun, Q., Sun, Z. T., Tacconi, M., Tang, X. W., Tang, Z. C., Tian, J., Ting, S. C. C., Ting, S. M., Tomassetti, N., Torsti, J., Tüysüz, C., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valencia-Otero, M., Valente, E., Valtonen, E., Vázquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J. P., Wang, C. X., Wang, L., Wang, L. Q., Wang, N. H., Wang, Q. L., Wang, S., Wang, X., Wang, Y., Wang, Z. M., Wei, J., Weng, Z. L., Wu, H., Xiong, R. Q., Xu, W., Yan, Q., Yang, Y., Yashin, I. I., Yi, H., Yu, Y. M., Yu, Z. Q., Zannoni, M., Zhang, C., Zhang, F., Zhang, F. Z., Zhang, J. H., Zhang, Z., Zhao, F., Zheng, C., Zheng, Z. M., Zhuang, H. L., Zhukov, V., Zichichi, A., Zuccon, P., and (AMS Collaboration)

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, 3. Good health
Abstract

Precise knowledge of the charge and rigidity dependence of the secondary cosmic ray fluxes and the secondary-to-primary flux ratios is essential in the understanding of cosmic ray propagation. We report the properties of heavy secondary cosmic ray fluorine F in the rigidity R range 2.15 GV to 2.9 TV based on 0.29 million events collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The fluorine spectrum deviates from a single power law above 200 GV. The heavier secondary-to-primary F/Si flux ratio rigidity dependence is distinctly different from the lighter B/O (or B/C) rigidity dependence. In particular, above 10 GV, the F/Si / B/O ratio can be described by a power law R$^{δ}$ with δ=0.052±0.007. This shows that the propagation properties of heavy cosmic rays, from F to Si, are different from those of light cosmic rays, from He to O, and that the secondary cosmic rays have two classes.

247. Properties of Heavy Secondary Fluorine Cosmic Rays : Results from the Alpha Magnetic Spectrometer

Author

Aguilar, M., Ali Cavasonza, Leila, Allen, M. S., Alpat, B., Ambrosi, G., Arruda, L., Attig, N., Barao, F., Barrin, L., Bartoloni, A., Başeğmez-du Pree, S., Battiston, R., Behlmann, M., Beranek, B., Berdugo, J., Bertucci, B., Bindi, V., Bollweg, K., Borgia, B., Boschini, M. J., Bourquin, M., Bueno, E. F., Burger, J., Burger, W. J., Burmeister, S., Cai, X. D., Capell, M., Casaus, J., Castellini, G., Cervelli, F., Chang, Y. H., Chen, G. M., Chen, G. R., Chen, H. S., Chen, Y., Cheng, L., Chou, H. Y., Chouridou, Sofia, Choutko, V., Chung, Chan Hoon, Clark, C., Coignet, G., Consolandi, C., Contin, A., Corti, C., Cui, Z., Dadzie, K., Delgado, C., Della Torre, S., Demirköz, M. B., Derome, L., Di Falco, S., Di Felice, V., Díaz, C., Dimiccoli, F., von Doetinchem, P., Dong, F., Donnini, F., Duranti, M., Egorov, A., Eline, A., Feng, J., Fiandrini, E., Fisher, P., Formato, V., Freeman, C., Galaktionov, Y., Gámez, C., García-López, R. J., Gargiulo, C., Gast, Henning, Gervasi, M., Giovacchini, F., Gómez-Coral, D. M., Gong, J., Goy, C., Grabski, V., Grandi, D., Graziani, M., Haino, S., Han, K. C., Hashmani, R. K., He, Z. H., Heber, B., Hsieh, T. H., Hu, J. Y., Incagli, M., Jang, W. Y., Jia, Yi, Jinchi, H., Kanishev, K., Khiali, B., Kim, G. N., Kirn, Thomas, Konyushikhin, M., Kounina, O., Kounine, A., Koutsenko, V., Kuhlman, A., Kulemzin, A., La Vacca, G., Laudi, E., Laurenti, G., Lazzizzera, I., Lebedev, A., Lee, H. T., Lee, S. C., Li, J. Q., Li, Manbing, Li, Q., Li, Sichen, Li, J. H., Li, Z. H., Liang, J., Light, C., Lin, C. H., Lippert, T., Liu, J. H., Liu, Z., Lu, S. Q., Lu, Y. S., Lübelsmeyer, Klaus, Luo, J. Z., Luo, Xi, Lyu, S. S., Machate, Fabian, Mañá, C., Marín, J., Marquardt, J., Martin, T., Martínez, G., Masi, N., Maurin, D., Menchaca-Rocha, A., Meng, Q., Mikhailov, V. V., Mo, D. C., Molero, M., Mott, P., Mussolin, L., Negrete, J., Nikonov, Nikolay, Nozzoli, F., Oliva, A., Orcinha, M., Palermo, M., Palmonari, F., Paniccia, M., Pashnin, A., Pauluzzi, M., Pensotti, S., Phan, H. D., Piandani, R., Plyaskin, V., Poluianov, S., Qin, X., Qu, Z. Y., Quadrani, L., Rancoita, P. G., Rapin, D., Conde, A. Reina, Robyn, E., Rosier-Lees, S., Rozhkov, A., Rozza, D., Sagdeev, R., Schael, Stefan, Schulz von Dratzig, A., Schwering, Georg, Seo, E. S., Shakfa, Z., Shan, B. S., Siedenburg, Thorsten, Solano, C., Song, J. W., Song, X. J., Sonnabend, Robin, Strigari, L., Su, T., Sun, Q., Sun, Z. T., Tacconi, M., Tang, X. W., Tang, Z. C., Tian, J., Ting, Samuel C. C., Ting, S. M., Tomassetti, N., Torsti, J., Tüysüz, C., Urban, T., Usoskin, I., Vagelli, V., Vainio, R., Valencia-Otero, M., Valente, E., Valtonen, E., Vázquez Acosta, M., Vecchi, M., Velasco, M., Vialle, J. P., Wang, C. X., Wang, L., Wang, L. Q., Wang, N. H., Wang, Q. L., Wang, S., Wang, X., Wang, Yu, Wang, Z. M., Wei, J., Weng, Z. L., Wu, H., Xiong, R. Q., Xu, W., Yan, Q., Yang, Y., Yashin, I. I., Yi, H., Yu, Y. M., Yu, Z. Q., Zannoni, M., Zhang, C., Zhang, F., Zhang, F. Z., Zhang, J. H., Zhang, Z., Zhao, F., Zheng, C., Zheng, Z. M., Zhuang, H. L., Zhukov, Valery, Zichichi, A., and Zuccon, P.

Subjects
Automatic Keywords, cosmic radiation: propagation, fluorine, satellite, cosmic radiation: secondary, magnetic spectrometer, Gravitation and Astrophysics, flux: ratio, 3. Good health
Abstract

Physical review letters 126(8), 081102 (2021). doi:10.1103/PhysRevLett.126.081102, Published by APS, College Park, Md.

248. Cosmic ray energetics and mass for the international space station (ISS-Cream)

Author

Seo, E. S., Anderson, T., Angelaszek, D., Baek, S. J., Baylon, J., Buénerd, M., Conklin, N. B., Copley, M., Coutu, S., Derome, L., Eraud, L., Gupta, M., Han, J. H., Huh, H. G., Hwang, Y. S., Hyun, H. J., Jeong, I. S., Kah, D. H., Kang, K. H., Kim, H. J., Kim, K. C., Kim, M. H., Kwashnak, K., Lee, J., Lee, M. H., Link, J., Lutz, L., Malinin, A., Menchaca-Rocha, A., Mitchell, J. W., Nutter, S., Ofoha, O., Park, H., Park, I. H., Park, J. M., Patterson, P., Wu, J., and Young Soo Yoon

249. The USINE cosmic-ray propagation code and recent results from an MCMC analysis

Author

Putze, A., Derome, L., Donato, F., David Maurin, Vernay, Emmanuelle, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [SDU.ASTR.HE] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.HE] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]

250. A Cherenkov imager for charge measurements of Nuclear Cosmic Rays in the CREAM II instrument

Author

Buénerd, M., Barrau, A., Bazer-Bachi, R., Borrel, V., Bourrion, O., Bouvier, J., Boyer, B., Derome, L., Eraud, L., Foglio, R., Gallin-Martel, L., Ganel, O., Moo Hyun Lee, Lutz, L., Malinine, A., Mangin-Brinet, M., Marcowith, A., Menchaca-Rocha, A., Périé, J. N., Protasov, K., Sallaz-Damaz, Y., Seo, E. S., Zinn, S. Y., bibliotheque, LPSC, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), and CREAM

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Physics::Instrumentation and Detectors, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]
Abstract

A proximity focusing Cherenkov imager for the charge measurement of nuclear cosmic rays in the CREAM II instrument, called CHERCAM, is under construction. This imager consists of a silica aerogel radiator plane facing a detector plane equipped with standard photomultipliers. The two planes are separated by a minimal ring expansion gap. The Cherenkov light yield is proportional to the squared charge of the detected particle. The expected relative light collection accuracy is in the few percents range. It should lead to single element separation over the range of nuclear charge Z of main interest 1 $leq$ Z $

Catalog

Books, media, physical & digital resources
See catalog results