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1. High spatial resolution correlation of AGILE TGFs and global lightning activity above the equatorial belt

Author: Fuschino F, Marisaldi M, Labanti C, Barbiellini G, Del Monte E, Bulgarelli A, Trifoglio M, Gianotti F, Galli M, Argan A, Trois A, Tavani M, Moretti E, Giuliani A, Longo F, Costa E, Caraveo P, Cattaneo PW, Chen A, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Lapshov I, Lazzarotto F, Lipari P, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Piano G, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Striani E, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Giommi P, Lucarelli F, Pittori C, Santolamazza P, Verrecchia F, Salotti L., D'AMMANDO, FILIPPO, F., Fuschino, M., Marisaldi, C., Labanti, G., Barbiellini, Monte, E., A., Bulgarelli, M., Trifoglio, F., Gianotti, M., Galli, A., Argan, A., Troi, M., Tavani, E., Moretti, A., Giuliani, Longo, Francesco, E., Costa, P., Caraveo, P. W., Cattaneo, A., Chen, F., D'Ammando, Paris, G., Cocco, G., Persio, G., I., Donnarumma, Y., Evangelista, M., Feroci, A., Ferrari, M., Fiorini, I., Lapshov, F., Lazzarotto, P., Lipari, S., Mereghetti, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, P., Picozza, G., Piano, M., Pilia, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, A., Rubini, S., Sabatini, P., Soffitta, E., Striani, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, L. A., Antonelli, S., Colafrancesco, S., Cutini, P., Giommi, F., Lucarelli, C., Pittori, P., Santolamazza, F., Verrecchia, L., Salotti, Fuschino F, Marisaldi M, Labanti C, Barbiellini G, Del Monte E, Bulgarelli A, Trifoglio M, Gianotti F, Galli M, Argan A, Trois A, Tavani M, Moretti E, Giuliani A, Longo F, Costa E, Caraveo P, Cattaneo PW, Chen A, DAmmando F, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Lapshov I, Lazzarotto F, Lipari P, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Piano G, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Striani E, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Giommi P, Lucarelli F, Pittori C, Santolamazza P, Verrecchia F, and Salotti L
Subjects: AGILE satellite, terrestrial gamma ray flashes, CsI calorimeter, satellite optical observations, global lightning, Atmospheric Processes: Lightning, Lightning [Atmospheric Processes], Atmospheric Processes: Atmospheric electricity, AGILE, TGF, global lightning activity, Atmospheric electricity [Atmospheric Processes]
Abstract: The AGILE satellite detects Terrestrial Gamma-ray Flashes (TGFs) in the 0.35-100 MeV energy range using its Mini-Calorimeter (MCAL) instrument with an average detection rate of 10 TGFs/month. Thanks to its Low Earth Orbit with only 2.5 degree of inclination, AGILE guarantees an unprecedented exposure above the equator, where both lightning activity and TGF detection peak. Here we report the comparison between the AGILE TGFs detected between March 2009 and February 2010 and full climatology lightning worldwide distribution based on satellite optical observations from LIS (Lightning Imaging Sensor) and OTD (Optical Transient Detector) instruments. This approach is complementary to the one-to-one TGF/lightning correlations by ground-based sferics measurements. Based on mono and bi-dimensional Kolmogorov-Smirnov tests, we show that the AGILE TGFs and time-averaged global lightning in the equatorial area are not drawn from the same distribution. However, we find significant regional differences in the degree of correlation as well as in the TGF/lightning ratio. In the case of south east Asia we find a 87% probability for the TGF and lightning being samples of the same distribution. This result supports the idea that the physical conditions at play in TGF generation can have strong geographical and climatological modulation. Based on the assumption that the observed range of TGF/flash ratio holds at all latitudes we can estimate a global rate of (N) over dot similar or equal to 220 divided by 570 TGFs per day. The observed TGF/flash geographical modulation as well as the TGF global rate estimate are in agreement with previous observations. Citation: Fuschino, F., et al. (2011), High spatial resolution correlation of AGILE TGFs and global lightning activity above the equatorial belt, Geophys. Res. Lett., 38, L14806, doi:10.1029/2011GL047817.
Published: 2011

2. The AGILE Mission

Author: Tavani M, Barbiellini G, Argan A, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Frutti M, Galli M, Gianotti F, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Liello F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mastropietro M, Mauri A, Mauri F, Mereghetti S, Morelli E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Pontoni C, Porrovecchio G, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Soffitta P, Traci A, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Preger B, Santolamazza P, Verrecchia F, Giommi P, Colafrancesco S, Antonelli A, Cutini S, Gasparrini D, Stellato S, Fanari G, Primavera R, Tamburelli F, Viola F, Guarrera G, Salotti L, D'Amico F, Marchetti E, Crisconio M, Sabatini P, Annoni G, Alia S, Longoni A, Sanquerin R, Battilana M, Concari P, Dessimone E, Grossi R, Parise A, Monzani F, Artina E, Pavesi R, Marseguerra G, Nicolini L, Scandelli L, Soli L, Vettorello V, Zardetto E, Bonati A, Maltecca L, D'Alba E, Patane M, Babini G, Onorati F, Acquaroli L, Angelucci M, Morelli B, Agostara C, Cerone M, Michetti A, Tempesta P, D'Eramo S, Rocca F, Giannini F, Borghi G, Garavelli B, Conte M, Balasini M, Ferrario I, Vanotti M, Collavo E, Giacomazzo M., D'AMMANDO, FILIPPO, M., Tavani, G., Barbiellini, A., Argan, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, E., Costa, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, G. D., Persio, I., Donnarumma, Y., Evangelista, M., Feroci, A., Ferrari, M., Fiorini, F., Fornari, F., Fuschino, T., Froysland, M., Frutti, M., Galli, F., Gianotti, A., Giuliani, C., Labanti, I., Lapshov, F., Lazzarotto, F., Liello, P., Lipari, Longo, Francesco, E., Mattaini, M., Marisaldi, M., Mastropietro, A., Mauri, F., Mauri, S., Mereghetti, E., Morelli, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, C., Pontoni, G., Porrovecchio, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, E., Rossi, A., Rubini, P., Soffitta, A., Traci, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, C., Pittori, B., Preger, P., Santolamazza, F., Verrecchia, P., Giommi, S., Colafrancesco, A., Antonelli, S., Cutini, D., Gasparrini, S., Stellato, G., Fanari, R., Primavera, F., Tamburelli, F., Viola, G., Guarrera, L., Salotti, F., D'Amico, E., Marchetti, M., Crisconio, P., Sabatini, G., Annoni, S., Alia, A., Longoni, R., Sanquerin, M., Battilana, P., Concari, E., Dessimone, R., Grossi, A., Parise, F., Monzani, E., Artina, R., Pavesi, G., Marseguerra, L., Nicolini, L., Scandelli, L., Soli, V., Vettorello, E., Zardetto, A., Bonati, L., Maltecca, E., D'Alba, M., Patane, G., Babini, F., Onorati, L., Acquaroli, M., Angelucci, B., Morelli, C., Agostara, M., Cerone, A., Michetti, P., Tempesta, S., D'Eramo, F., Rocca, F., Giannini, G., Borghi, B., Garavelli, M., Conte, M., Balasini, I., Ferrario, M., Vanotti, E., Collavo, M., Giacomazzo, Tavani M, Barbiellini G, Argan A, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Frutti M, Galli M, Gianotti F, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Liello F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mastropietro M, Mauri A, Mauri F, Mereghetti S, Morelli E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Pontoni C, Porrovecchio G, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Soffitta P, Traci A, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Preger B, Santolamazza P, Verrecchia F, Giommi P, Colafrancesco S, Antonelli A, Cutini S, Gasparrini D, Stellato S, Fanari G, Primavera R, Tamburelli F, Viola F, Guarrera G, Salotti L, D'Amico F, Marchetti E, Crisconio M, Sabatini P, Annoni G, Alia S, Longoni A, Sanquerin R, Battilana M, Concari P, Dessimone E, Grossi R, Parise A, Monzani F, Artina E, Pavesi R, Marseguerra G, Nicolini L, Scandelli L, Soli L, Vettorello V, Zardetto E, Bonati A, Maltecca L, D'Alba E, Patane M, Babini G, Onorati F, Acquaroli L, Angelucci M, Morelli B, Agostara C, Cerone M, Michetti A, Tempesta P, D'Eramo S, Rocca F, Giannini F, Borghi G, Garavelli B, Conte M, Balasini M, Ferrario I, Vanotti M, Collavo E, and Giacomazzo M
Subjects: Agile, Active galactic nucleus, gamma and X ray detection, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, satellite, FOS: Physical sciences, Astrophysics, High Energy Gamma-ray Astronomy, Pulsar, astro-ph, Angular resolution, media_common, Physics, Calorimeter (particle physics), Astrophysics (astro-ph), Detector, AGILE satellite, Detectors, Astronomy and Astrophysics, Universe, Supernova, Space and Planetary Science, Orbit (dynamics), instrumentation: detectors – techniques: high angular resolution – techniques: image processing – gamma rays: observations – X-rays: general
Abstract: AGILE is an Italian Space Agency mission dedicated to the observation of the gamma-ray Universe. The AGILE very innovative instrumentation combines for the first time a gamma-ray imager (sensitive in the energy range 30 MeV - 50 GeV), a hard X-ray imager (sensitive in the range 18-60 keV) together with a Calorimeter (sensitive in the range 300 keV - 100 MeV) and an anticoincidence system. AGILE was successfully launched on April 23, 2007 from the Indian base of Sriharikota and was inserted in an equatorial orbit with a very low particle background. AGILE provides crucial data for the study of Active Galactic Nuclei, Gamma-Ray Bursts, pulsars, unidentified gamma-ray sources, Galactic compact objects, supernova remnants, TeV sources, and fundamental physics by microsecond timing. An optimal angular resolution (reaching 0.1-0.2 degrees in gamma-rays, 1-2 arcminutes in hard X-rays) and very large fields of view (2.5 sr and 1 sr, respectively) are obtained by the use of Silicon detectors integrated in a very compact instrument. The paper describes the AGILE Mission and its space and ground segments., 20 pages, 26 figures. submitted to Astron. & Astrophys
Published: 2009

3. A precise measurement of the muon neutrino-nucleon inclusive charged current cross section off an isoscalar target in the energy range 2.5 < E-v < 40 GeV by NOMAD RID B-6634-2009

Author: Wu Q, Mishra SR, Godley A, Petti R, Alekhin S, Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Challis R, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Degaudenzi H, Del Prete T, De Santo A, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kent N, Kim JJ, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kulagin S, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Ling J, Linssen L, Ljubicic A, Long J, Lupi A, Lyubushkin V, Marchionni A, Martelli F, Mechian X, Mendiburu JP, Meyer JP, Mezzetto M, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Placci A, Polesello G, Pollmann D, Polyarush A, Poulsen C, Popov B, Rebuffi L, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Samoylov O, Schahmaneche K, Schmidt B, Schmidt T, Sconza A, Seaton M, Sevior M, Sillou D, Soler FJP, Sozzii G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Wu, Q, Mishra, Sr, Godley, A, Petti, R, Alekhin, S, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Challis, R, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Degaudenzi, H, Del Prete, T, De Santo, A, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kent, N, Kim, Jj, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kulagin, S, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Ling, J, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Lyubushkin, V, Marchionni, A, Martelli, F, Mechian, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Poulsen, C, Popov, B, Rebuffi, L, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Samoylov, O, Schahmaneche, K, Schmidt, B, Schmidt, T, Sconza, A, Seaton, M, Sevior, M, Sillou, D, Soler, Fjp, Sozzii, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Experiment, Nuclear Experiment
Abstract: We present a measurement of the muon neutrino-nucleon inclusive charged current cross section, off an isoscalar target, in the neutrino energy range 2.5
Published: 2008

4. Prediction of neutrino fluxes in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDCE, Dumarchez J, Ellis M, Feldman GJ, Ferrari A, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hong TM, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Shih D, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira M, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuberq K., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Edce, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, A, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hong, Tm, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Shih, D, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, M, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, and Zuberq, K.
Subjects: High Energy Physics::Phenomenology, High Energy Physics::Experiment
Abstract: The method developed for the calculation of the flux and composition of the West Area Neutrino Beam used by NOMAD in its search for neutrino oscillations is described. The calculation is based on particle production rates computed using a recent version of FLUKA and modified to take into account the cross-sections measured by the SPY and NA20 experiments. These particles are propagated through the beam line taking into account the material and magnetic fields they traverse. The neutrinos produced through their decays are tracked to the NOMAD detector. The fluxes of the four neutrino flavours at NOMAD,are predicted with an uncertainty of about 8% for v(mu) and v(e), 10% for (v) over bar (mu), and 12% for (v) over bar (e). The energy-dependent uncertainty achieved on the v(e)/v(mu) prediction needed for a v(mu) --> v(e) oscillation search ranges from 4% to 7%, whereas the overall normalization uncertainty on this ratio is 4.2%. (C) 2003 Elsevier B.V. All rights reserved.
Published: 2003

5. New results on a search for a 33.9 MeV/c(2) neutral particle from pi(+) decay in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko SN, Godley A, Gonzalez Garcia MC, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov MM, Klimov O, Kokkonen J, Kovzelev AV, Krasnikov NV, Krasnoperov A, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rathouit P, Rico J, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Sevoir M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin AN, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, Sn, Godley, A, Gonzalez Garcia, Mc, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, Mm, Klimov, O, Kokkonen, J, Kovzelev, Av, Krasnikov, Nv, Krasnoperov, A, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rathouit, P, Rico, J, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Sevoir, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, An, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: We report on a direct search in NOMAD for a new 33.9 MeV/c(2) neutral particle (X) produced in pion decay in flight, pi --> muX followed by the decay X --> nue(+)e(-). Both decays are postulated to occur to explain the time anomaly observed by the KARMEN experiment. From the analysis of the data collected during the 1996-1998 runs with 4.1 x 10(19) protons on target, a single candidate event consistent with background expectations was found. The search is sensitive to a pion branching ratio BR(pi --> muX) > 3.7 x 10(-15), significantly smaller than previous experimental limits. (C) 2002 Elsevier Science B.V. All rights reserved.
Published: 2002

6. A study of strange particle production in nu(mu) charged current interactions in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Challis R, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDCE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kent N, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore FX, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Challis, R, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Edce, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kent, N, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, Fx, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: High Energy Physics::Experiment
Abstract: A study of strange particle production in nu(mu) charged cur-rent interactions has been performed using the data from the NOMAD experiment. Yields of neutral strange particles (K-S(0), Lambda, (&ULambda;) over bar) have been measured. Mean multiplicities are reported as a function of the event kinematic variables E-nu W-2 and Q(2) as well as of the variables describing particle behaviour within a hadronic jet: x(F), z and p(T)(2). Decays of resonances and heavy hyperons with identified K, and A in the final state have been analyzed. Clear signals corresponding to K*+/-, Sigma(*+/-), Xi(-) and Sigma(0) have been observed. (C) 2002 Elsevier Science B.V. All rights reserved.
Published: 2002

7. Study of D*(+) production in nu(mu) charged current interactions in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Challis R, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kent N, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Challis, R, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kent, N, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: A search was made among numu charged current events collected in the NOMAD experiment for the reaction: nu(mu) + N --> mu(-) + D*+ + hadrons hooked right arrowD(0) + pi(+) hooked right arrowK(-) + pi(+) A high purity D*+ sample composed of 35 events was extracted. The D*+ yield in nu(mu) charged current interactions was measured to be T = (0.79 +/- 0.17(stat.) +/- 0.10(syst.))%. The mean fraction of the hadronic jet energy taken by the D*+ is 0.67 +/- 0.02(stat.) +/- 0.02(syst.). The distributions of the fragmentation variables z, P-T(2) and x(F) for D*+ are also presented. (C) 2002 Elsevier Science B.V. All rights reserved.
Published: 2002

8. Final NOMAD results on nu(mu) -> nu(tau) and nu(e) -> nu(tau) oscillations including a new search for nu(tau) appearance using hadronic tau decays RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov VE, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sconza A, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sconza, A, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: Results from the v, appearance search in a neutrino beam using the full NOMAD data sample are reported. A new analysis unifies all the hadronic tau decays, significantly improving the overall sensitivity of the experiment to oscillations. The "blind analysis" of all topologies yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% CL allowed region in the sin(2)2 theta (mu tau)-Deltam(2) plane which includes sin(2)2 theta (mu tau) < 3.3 x 10(-4) at large Deltam(2) and Deltam(2) < 0.7 eV(2)/c(4) at sin(2) 2 theta (mu tau) = 1. The corresponding contour in the nu (e) --> nu (tau) oscillation hypothesis results in sin(2) 2 theta (l tau) < 1.5 x 10(-2) at large Deltam(2) and Deltam(2) < 5.9 eV(2)/c(4) at sin(2) 2 theta (l tau) = 1. We also derive limits on effective couplings of the tau lepton to nu (mu) or nu (l). (C) 2001 Elsevier Science B.V. All rights reserved.
Published: 2001

9. Measurement of the (lambda)over-bar polarization in nu(mu) charged current interactions in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: We present a measurement of the polarization of )over bar> hyperons produced in nu (mu) charged current interactions. The full data sample from the NOMAD experiment has been analyzed using the same V-0 identification procedure and analysis method reported in a previous paper [NOMAD Collaboration. Nucl. Phys. B 588 (2000) 3] for the case of Lambda hyperons. The )over bar> polarization has been measured for the first time in a neutrino experiment. The polarization vector is found to be compatible with zero. (C) 2001 Elsevier Science B.V. All rights reserved.
Published: 2001

10. Inclusive production of rho(0)(770), f(0)(980) and f(2)(1270) mesons in nu(mu) charged current interactions RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, LaRotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rathouit P, Rico J, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, Larotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rathouit, P, Rico, J, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: Nuclear Theory, High Energy Physics::Experiment, Nuclear Experiment
Abstract: The inclusive production of the meson resonances p(0)(770), f(0)(980) and f(2)(1270) in neutrino- nucleus charged current interactions has been studied with the NOMAD detector exposed to the wide band neutrino beam generated by 450 GeV protons at the CERN SPS. For the first time the f0(980) meson is observed in neutrino interactions. The statistical significance of its observation is 6 standard deviations. The presence of f(2)(1270) in neutrino interactions is reliably established, The average multiplicity of these three resonances is measured as a function of several kinematic variables, The experimental results are compared to the multiplicities obtained from a simulation based on the Lund model, In addition, the average multiplicity of rho (0)(770) in antineutrino-nucleus interactions is measured. (C) 2001 Elsevier Science B.V. All rights reserved.
Published: 2001

11. A study of backward going p and pi(-) in nu(mu) CC interactions with the NOMAD detector RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vidal Sitjes G, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: Backward proton and pi (-) production has been studied in nu (mu) CC interactions with carbon nuclei. Detailed analyses of the momentum distributions, of the production rates, and of the general features of events with a backward going particle, have been carried out in order to understand the mechanism producing these particles. The backward proton data have been compared with the predictions of the reinteraction and the short range correlation models. (C) 2001 Elsevier Science B.V. All rights reserved.
Published: 2001

12. Neutrino production of opposite sign dimuons in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol GM, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, De Santo A, Del Prete T, Dignan T, Di Lella L, Silva ED, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Ccdeenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Cuglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov V, Lacaprara S, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Manola Poggioli E, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Mossuz L, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Pluquet A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rathouit P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior ME, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko S, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Verkindt D, Vieira JM, Vinogradova T, Vo MK, Weber F, Weisse T, Wilson F, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, Gm, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, De Santo, A, Del Prete, T, Dignan, T, Di Lella, L, Silva, Ed, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Ccdeenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Cuglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, V, Lacaprara, S, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rathouit, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, Me, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, S, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Weber, F, Weisse, T, Wilson, F, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: The NOMAD Collaboration presents a study of opposite sign dimuon events in the framework of Leading Order QCD. A total of 2714 neutrino- and 115 antineutrino-induced opposite sign dimuon events with E-mu 1, E-mu 2 > 4.5 GeV, 15 < E-nu < 300 GeV and Q(2) > 1 (GeV/c)(2) are observed in the Front-Calorimeter of NOMAD during the 1995 and 1996 runs. The analysis yields a value for the charm quark mass of m(c) = 1.3(-0.3-0.3)(+0.3+0.3) GeV/c(2) and fur the average semileptonic branching ratio of B-c = 0.095(-0.007-0.013)(+0.007+0.014). The ratio of the strange to non-strange sea in the nucleon is measured to be kappa = 0.48(-0.07-0.12)(+0.09+0.17). The measured rate of charm-induced dimuon relative to single muon, as a function of neutrino energy, is consistent with the slow rescaling hypothesis of heavy quark production. (C) 2000 Published by Elsevier Science B.V.
Published: 2000

13. Updated results from the nu(tau) appearance search in NOMAD RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov VE, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rebuffi L, Rico J, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rebuffi, L, Rico, J, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: Updated results from the appearance searches for nu(mu) --> nu(tau) and nu(e) --> nu(tau) oscillations in the full NOMAD data sample are reported. The increased data and the use of more refined kinematic schemes for the nu(tau) CC selection allow a significant improvement of the overall sensitivity. The "blind analysis" of both the deep-inelastic and the low multiplicity samples yields no evidence for an oscillation signal. In the two-family oscillation scenario, this sets a 90% C.L. region in the sin(2)2 theta(mu tau) - Delta m(2) plane which includes sin(2)2 theta(mu tau) < 4.4 X 10(-4) at large Delta m(2) and Delta m(2) < 0.8 eV(2)/c(4) at sin(2)2 theta(mu tau) = 1. The corresponding contour in the nu(e) --> nu(tau) oscillation hypothesis results in sin(2)2 theta(e tau) < 2.2 X 10(-2) at large Delta m(2) and Delta m(2) < 6.5 eV(2)/c(4) at sin(2)2 theta(e tau) = 1. (C) 2000 Elsevier Science B.V. All rights reserved.
Published: 2000

14. Limit on nu(e) -> nu(tau) oscillations from the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov VE, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Pluquet A, Polayrush A, Polesello G, Pollmann D, Popov B, Poulsen C, Rathouit P, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polayrush, A, Polesello, G, Pollmann, D, Popov, B, Poulsen, C, Rathouit, P, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Abstract: In the context of a two-flavour approximation we reinterpret the published NOMAD limit on nu(mu) --> nu(tau) oscillations in terms of nu(e) --> nu(tau) oscillations. At 90% C.L. we obtain sin2(2)theta(e tau) < 5.2 X 10(-2) for large Delta m(2), while for sin2(2)theta(e tau) = 1 the confidence region includes Delta m(2) < 11 eV(2)/c(4). (C) 2000 Published by Elsevier Science B.V. All rights reserved.
Published: 2000

15. Measurement of the Lambda polarization in nu(mu) charged current interactions in the NOMAD experiment RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Chukanov A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kustov D, Kuznetsov V, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Naumov D, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pannacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush A, Popov B, Poulsen C, Rathouit P, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Vieira JM, Vinogradova T, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pannacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rathouit, P, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: High Energy Physics::Experiment, Nuclear Experiment
Abstract: The Lambda polarization in upsilon (mu) charged current interactions has been measured in the NOMAD experiment. The event sample (8087 reconstructed Lambda 's) is more than an order of magnitude larger than that of previous bubble chamber experiments, while the quality of event reconstruction is comparable. We observe negative polarization along the W-boson direction which is enhanced in the target fragmentation region: P-x(x(F) < 0) = -0.21 +/- 0.04(stat) +/- 0.02(sys). In the current fragmentation region we find P-x(x(F) > 0) = -0.09 +/- 0.06(stat) +/- 0.03(sys). These results provide a test of different models describing the nucleon spin composition and the spin transfer mechanisms. A significant transverse polarization tin the direction orthogonal to the Lambda production plane! has been observed for the first time in a neutrino experiment: P-y = -0.22 +/- 0.03(stat) +/- 0.01(sys). The dependence of the absolute value of P-y on the Lambda transverse momentum with respect to the hadronic jet direction is in qualitative agreement with the resuits from unpolarized hadron-hadron experiments. (C) 2000 Elsevier Science B.V. All rights reserved.
Published: 2000

16. Search for eV (pseudo) scalar penetrating particles in the SPS neutrino beam RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Bassompiene G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Dumarchez J, Ellis M, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko SN, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov MM, Klimov O, Kokkonen J, Kovzelev AV, Krasnikov NV, Krasnoperov A, Kuznetsov VE, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Mossuz L, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Polesello G, Pollmann D, Polyarush AY, Popov B, Poulsen C, Rico J, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin AN, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Verkindt D, Vieira JM, Vinogradova T, Volkov SA, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zioutas K, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompiene, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, Sn, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, Mm, Klimov, O, Kokkonen, J, Kovzelev, Av, Krasnikov, Nv, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, Ay, Popov, B, Poulsen, C, Rico, J, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, An, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Volkov, Sa, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zioutas, K, Zuber, K, and Zuccon, P.
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Experiment
Abstract: We carried out a model-independent search for light scalar or pseudoscalar particles a's (an example of which is the axion) that couple to two photons by using a photon-regeneration method at high energies allowing a substantial increase in the sensitivity to eV masses. The experimental set-up is based on elements of the CERN West Area Neutrino Facility (WANF) beam Line and the NOMAD neutrino detector. The new particles, if they exist, could be produced through the Primakoff effect in interactions of high energy photons, generated by the 450 GeV protons in the CERN SPS neutrino target, with virtual photons from the WANF horn magnetic field. The particles would penetrate the downstream shielding and would be observed in the NOMAD neutrino detector through their re-conversion into real high energy photons by interacting with the virtual photons from the magnetic field of the NOMAD dipole magnet. From the analysis of the data collected during the 1996 run with 1.08 x 10(19) protons on target, 312 candidate events with energy between 5 and 140 GeV were found. This number is in general agreement with the expectation of 272 +/- 18 background events from standard neutrino processes. A 90 % CL upper limit on the a gamma gamma-coupling g(a gamma gamma) < 1.5 x 10(-4) GeV-1 for a masses up to 40 eV is obtained. (C) 2000 Elsevier Science B.V. All rights reserved.
Published: 2000

17. Parameterization of e and gamma initiated showers in the NOMAD lead-glass calorimeter RID C-6672-2008

Author: Autiero D, Baldo Ceolin M, Bobisut F, Cattaneo PW, Cavasinni V, Collazuol G, Conforto G, Contalbrigo M, Conta C, Del Prete T, De Santo A, Ferrari R, Flaminio V, Fraternali M, Gibin D, Gninenko SN, Graziani G, Guglielmi A, Iacopini E, Lacaprara S, Lupi A, Kirsanov MM, Kovzelev AV, La Rotonda L, Lanza A, Laveder M, Marchionni A, Martelli F, Mezzetto M, Pastore F, Pennacchio E, Petti R, Polesello G, Renzoni G, Roda C, Salvatore F, Sconza A, Toropin AN, Valdata Nappi M, Veltri M, Vercesi V, Volkov SA, ORESTANO, DOMIZIA, Autiero, D, Baldo Ceolin, M, Bobisut, F, Cattaneo, Pw, Cavasinni, V, Collazuol, G, Conforto, G, Contalbrigo, M, Conta, C, Del Prete, T, De Santo, A, Ferrari, R, Flaminio, V, Fraternali, M, Gibin, D, Gninenko, Sn, Graziani, G, Guglielmi, A, Iacopini, E, Lacaprara, S, Lupi, A, Kirsanov, Mm, Kovzelev, Av, La Rotonda, L, Lanza, A, Laveder, M, Marchionni, A, Martelli, F, Mezzetto, M, Orestano, Domizia, Pastore, F, Pennacchio, E, Petti, R, Polesello, G, Renzoni, G, Roda, C, Salvatore, F, Sconza, A, Toropin, An, Valdata Nappi, M, Veltri, M, Vercesi, V, and Volkov, Sa
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Experiment
Abstract: A description of the response of the NOMAD electromagnetic calorimeter to electrons and photons is discussed. In particular, the dependence of the two-dimensional shower shape on the angle and energy of the incident particle is parametrized by analytical functions. Some applications to the neutrino event reconstruction are also reported. (C) 1999 Elsevier Science B.V. All rights reserved.
Published: 1999

18. Precision measurement of scaled momentum, charge multiplicity, and thrust in nu N-mu and (nu)over-bar(mu)N interactions RID B-6634-2009 RID C-6672-2008

Author: Altegoer J, Angelini C, Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Basa S, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, De Santo A, Del Prete T, Dignan T, Di Lella L, Silva EDE, Donnelly IJ, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Galumian P, Gangler E, Geiser A, GEppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov VE, Lacaprara S, Lanza A, La Rotonda L, Laveder M, Lazzeroni C, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Manola Poggioli E, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Mossuz L, Moorhead GF, Nedelec P, Nefedov Y, Nguyen Mau C, Nordmann D, Pastore F, Peak LS, Pennacchio E, Perroud JP, Pessard H, Petti R, Placci A, Pluquet A, Polesello G, Pollmann D, Popov B, Poulsen C, Rathouit P, Renzoni G, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Serrano M, Sevior ME, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko S, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Uros V, Vacavant V, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Verkindt D, Vieira JM, Vinogradova T, Vo MK, Volkov S, Weber F, Weisse T, Werlen M, Wilson F, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Altegoer, J, Angelini, C, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, De Santo, A, Del Prete, T, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Mossuz, L, Moorhead, Gf, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Nordmann, D, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polesello, G, Pollmann, D, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Serrano, M, Sevior, Me, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, S, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Vacavant, V, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, F, Weisse, T, Werlen, M, Wilson, F, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: High Energy Physics::Experiment, Nuclear Experiment
Abstract: We report the first precision measurements of the scaled momentum, the charge multiplicity, and the thrust of hadronic jets in the Breit frame in Deep Inelastic Scattering nu(mu)N and charged cur rent events over the Q(2) range from 1 to 100 GeV2. The neutrino data, obtained in the NOMAD experiment at the CERN SPS, extend the Q(2)-evolution of these parameters by two orders of magnitude, and with commensurate precision, when compared to those reported by the ep and e(+)e(-) experiments. (C) 1999 Elsevier Science B.V. All rights reserved.
Published: 1999

19. A more sensitive search for nu(mu) -> nu(tau) oscillations in NOMAD RID B-6634-2009 RID C-6672-2008

Author: Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol G, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, Degaudenzi H, Del Prete T, De Santo A, Dignan T, Di Lella L, Silva EDE, Donnelly IJ, Dumarchez J, Ellis M, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Gandolfo A, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko S, Godley A, Gomez Cadenas JJ, Gosset J, Gossling C, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Juget F, Kirsanov M, Klimov O, Kokkonen J, Kovzelev A, Krasnoperov A, Kuznetsov VE, Lacaprara S, Lachaud C, Lakic B, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Manola Poggioli E, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Mossuz L, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Pessard H, Petti R, Placci A, Pluquet A, Polesello G, Pollmann D, Popov B, Poulsen C, Rathouit P, Reno R, Renzoni G, Rico J, Riemann P, Roda C, Rubbia A, Salvatore F, Schahmaneche K, Schmidt B, Schmidt T, Segneri G, Sevior M, Sillou D, Soler FJP, Sozzi G, Steele D, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko V, Toropin A, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Vacavant L, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Verkindt D, Vieira JM, Vinogradova T, Vo MK, Volkov S, Weber FV, Weisse T, Wilson FF, Winton LJ, Yabsley BD, Zaccone H, Zuber K, Zuccon P., ORESTANO, DOMIZIA, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gandolfo, A, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polesello, G, Pollmann, D, Popov, B, Poulsen, C, Rathouit, P, Reno, R, Renzoni, G, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Segneri, G, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Subjects: High Energy Physics::Experiment
Abstract: With additional data and improved algorithms, we have enhanced the sensitivity of our appearance search for nu(mu) --> nu(tau) oscillations in the NOMAD detector in the CERN-SPS wide-band neutrino beam. The search uses kinematic criteria to identify nu(tau) charged current interactions followed by decay of the tau(-) to one of several decay modes. Our "blind'' analyses of deep-inelastic scattering data taken in 1996 and 1997, combined with consistent reanalyses of previously reported 1995 data, yield no oscillation signal. For the two-family oscillation scenario, we present the contour outlining a 90% C.L. confidence region in the sin(2)2 theta(mu tau) - Delta m(2) plane. At large Delta m(2) the confidence region includes sin(2)2 theta(mu tau) < 1.2 X 10(-3) (a limit 3.5 times more stringent than in our previous publication), while at sin(2)2 theta(mu tau) = 1 the confidence region includes Delta m(2) < 1.2 eV(2)/c(4). (C) 1999 Published by Elsevier Science B.V. All rights reserved.
Published: 1999

20. A study of the transverse fluctuations of hadronic showers in the NOMAD electromagnetic calorimeter RID C-6672-2008

Author: Autiero D, Baldo Ceolin M, Bobisut F, Camilleri L, Cattaneo PW, Cavasinni V, Collazuol GM, Conforto G, Conta C, Contalbrigo M, Del Prete T, De Santo A, Di Lella L, Ferrari R, Flaminio V, Fraternali M, Gibin D, Gninenko SN, Graziani G, Guglielmi A, Iacopini E, Kirsanov MM, Kovzelev AV, Lacaprara S, La Rotonda L, Lanza A, Laveder M, Lupi A, Marchionni A, Martelli F, Mezzetto M, Pastore F, Pennacchio E, Petti R, Polesello G, Renzoni G, Roda C, Rubbia A, Salvatore F, Sconza A, Toropin AN, Valdata Nappi M, Veltri M, Vercesi V, Volkov SA, ORESTANO, DOMIZIA, Autiero, D, Baldo Ceolin, M, Bobisut, F, Camilleri, L, Cattaneo, Pw, Cavasinni, V, Collazuol, Gm, Conforto, G, Conta, C, Contalbrigo, M, Del Prete, T, De Santo, A, Di Lella, L, Ferrari, R, Flaminio, V, Fraternali, M, Gibin, D, Gninenko, Sn, Graziani, G, Guglielmi, A, Iacopini, E, Kirsanov, Mm, Kovzelev, Av, Lacaprara, S, La Rotonda, L, Lanza, A, Laveder, M, Lupi, A, Marchionni, A, Martelli, F, Mezzetto, M, Orestano, Domizia, Pastore, F, Pennacchio, E, Petti, R, Polesello, G, Renzoni, G, Roda, C, Rubbia, A, Salvatore, F, Sconza, A, Toropin, An, Valdata Nappi, M, Veltri, M, Vercesi, V, and Volkov, Sa
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Experiment, Nuclear Experiment
Abstract: The transverse shower shape of the energy deposition of hadrons in the NOMAD lead glass calorimeter has been studied by exposing a prototype of this calorimeter to pion test beams of various momenta and incident angles. Large event-to-event fluctuations in the shower shape and significant energy depositions far from the incident hadron were observed making it difficult to associate all the deposited energy to the incident hadron that caused it. Since in the NOMAD detector the momenta of charged hadrons are measured by a magnetic spectrometer, such an association is necessary to be able to subtract from the calorimeter ail the energy caused by the observed charged hadrons in order to avoid double counting. Probability functions based on the measurements have been developed to describe fluctuations of the lateral shower shape. Starting from these Functions, an algorithm is developed for identifying the energy deposition associated to a charged hadron. The identification and separation of overlapping showers based on these functions is also discussed. The Monte Carlo simulation of the calorimeter reproduces the test beam data well therefore allowing the application of the algorithm at angles and momenta not studied in the test beam. (C) 1998 Elsevier Science B.V. All rights reserved.
Published: 1998

21. Search for a new gauge boson in pi(0) decays RID B-6634-2009 RID C-6672-2008

Author: Altegoer J, Astier P, Autiero D, Baldisseri A, Baldo Ceolin M, Ballocchi G, Banner M, Basa S, Bassompierre G, Benslama K, Besson N, Bird I, Blumenfeld B, Bobisut F, Bouchez J, Boyd S, Bueno A, Bunyatov S, Camilleri L, Cardini A, Castera A, Cattaneo PW, Cavasinni V, Cervera Villanueva A, Collazuol GM, Conforto G, Conta C, Contalbrigo M, Cousins R, Daniels D, De Santo A, Del Prete T, Dignan T, Di Lella L, Silva EDE, Donnelly IJ, Dumarchez J, Fazio T, Feldman GJ, Ferrari R, Ferrere D, Flaminio V, Fraternali M, Gaillard JM, Galumian P, Gangler E, Geiser A, Geppert D, Gibin D, Gninenko SN, Gomez Cadenas JJ, Gosset J, Gossling CC, Gouanere M, Grant A, Graziani G, Guglielmi A, Hagner C, Hernando J, Hubbard D, Hurst P, Hyett N, Iacopini E, Joseph C, Kekez D, Khomenko B, Kirsanov MM, Klimov O, Kokkonen J, Kovzelev AV, Kuznetsov V, Lacaprara S, Lanza A, La Rotonda L, Laveder M, Letessier Selvon A, Levy JM, Linssen L, Ljubicic A, Long J, Lupi A, Manola Poggioli E, Marchionni A, Martelli F, Mechain X, Mendiburu JP, Meyer JP, Mezzetto M, Mishra SR, Moorhead GF, Mossuz L, Nedelec P, Nefedov Y, Nguyen Mau C, Pastore F, Peak LS, Pennacchio E, Perroud JP, Pessard H, Petti R, Placci A, Plothow Besch H, Pluquet A, Polesello G, Pollmann D, Pope BG, Popov B, Poulsen C, Rathouit P, Roda C, Rubbia A, Salvatore F, Scannicchio D, Schahmaneche K, Schmidt B, Sconza A, Serrano M, Sevior ME, Sillou D, Soler FJP, Sozzi G, Steele D, Steffen P, Steininger M, Stiegler U, Stipcevic M, Stolarczyk T, Tareb Reyes M, Taylor GN, Tereshchenko S, Toropin AN, Touchard AM, Tovey SN, Tran MT, Tsesmelis E, Ulrichs J, Uros V, Valdata Nappi M, Valuev V, Vannucci F, Varvell KE, Veltri M, Vercesi V, Verkindt D, Vieira JM, Vinogradova T, Vo MK, Volkov SA, Weber F, Weisse T, Werlen M, Wilson F, Winton LJ, Yabsley BD, Zaccone H., ORESTANO, DOMIZIA, Altegoer, J, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Castera, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, Gm, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, De Santo, A, Del Prete, T, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, Sn, Gomez Cadenas, Jj, Gosset, J, Gossling, Cc, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Kekez, D, Khomenko, B, Kirsanov, Mm, Klimov, O, Kokkonen, J, Kovzelev, Av, Kuznetsov, V, Lacaprara, S, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Placci, A, Plothow Besch, H, Pluquet, A, Polesello, G, Pollmann, D, Pope, Bg, Popov, B, Poulsen, C, Rathouit, P, Roda, C, Rubbia, A, Salvatore, F, Scannicchio, D, Schahmaneche, K, Schmidt, B, Sconza, A, Serrano, M, Sevior, Me, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steffen, P, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, S, Toropin, An, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, Sa, Weber, F, Weisse, T, Werlen, M, Wilson, F, Winton, Lj, Yabsley, Bd, and Zaccone, H.
Abstract: A search was made for a new light gauge boson X which might be produced in pi(0) -->, gamma + X decay from neutral pions generated by 450 GeV protons in the CERN SPS neutrino target. The X's would penetrate the downstream shielding and be observed in the NOMAD detector via the Primakoff effect, in the process of X --> pi(0) conversion in the external Coulomb field of a nucleus. With 1.45 x 10(18) protons on target, 20 candidate events with energy between 8 and 140 GeV were found from the analysis of neutrino data. This number is in agreement with the expectation of 18.1 +/- 2.8 background events from standard neutrino processes. A new 90% C.L. upper limit on the branching ratio Br(pi(0) --> Y + X)< (3.3 to 1.9)X 10(-5) for X masses ranging from 0 to 120 MeV/c(2) is obtained. (C) 1998 Elsevier Science B.V. All rights reserved.
Published: 1998

22. A search for nu(mu)->nu(tau) oscillations using the NOMAD detector RID B-6634-2009 RID C-6672-2008

Author: Altegoer, J, Angelini, Carlo, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Castera, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Fumagalli, G, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kekez, D, Khomenko, B, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Kuznetsov, Ve, Lacaprara, S, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Placci, A, Plothow Besch, H, Pluquet, A, Polesello, G, Pollmann, D, Pope, Bg, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Scannicchio, D, Schahmaneche, K, Schmidt, B, Sconza, A, Serrano, M, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steffen, P, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, Fv, Weisse, T, Werlen, M, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K., Altegoer, J, Angelini, C, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Castera, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Fumagalli, G, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kekez, D, Khomenko, B, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Kuznetsov, Ve, Lacaprara, S, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Placci, A, Plothow Besch, H, Pluquet, A, Polesello, G, Pollmann, D, Pope, Bg, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, C, Rubbia, A, Salvatore, F, Scannicchio, D, Schahmaneche, K, Schmidt, B, Sconza, A, Serrano, M, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steffen, P, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, Fv, Weisse, T, Werlen, M, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, and Zuber, K.
Subjects: High Energy Physics::Experiment
Abstract: NOMAD is a neutrino oscillation experiment designed to search for v(tau) appearance in the CERN-SPS wide band v(mu) beam. Signal detection relies on the identification of I: charged current interactions using kinematic criteria. The analysis of the 1995 data sample yields no oscillation signal. Combining all studied tau decay modes, a limit of sin(2)2 theta(mu tau) < 4.2 x 10(-3) is obtained for large Delta m(2) at the 90% confidence level. (C) 1998 Elsevier Science B.V. All rights reserved.
Published: 1998

23. The NOMAD experiment at the CERN SPS RID B-6634-2009 RID C-6672-2008

Author: Altegoer, J, Anfreville, M, Angelini, Carlo, Astier, P, Authier, M, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Bunyatov, S, Boyd, S, Bueno, A, Camilleri, L, Cardini, A, Castera, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cavestro, V, Cloue, O, Conforto, G, Conta, C, Cousins, R, De Santo, A, Del Prete, T, Di Lella, L, Dignan, T, Silva, Ede, Donnelly, Lj, Dumarchez, J, Dumps, L, Engster, C, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Fumagalli, G, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Huta, W, Hyett, N, Iacopini, E, Joseph, C, Kirsanov, M, Kekez, D, Khomenko, B, Klimov, O, Kovzelev, A, Kuznetsov, V, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Passerieux, Jp, Pastore, F, Peak, Ls, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Petitpas, P, Placci, A, Plothow Besch, H, Pluquet, A, Poinsignon, J, Polesello, G, Pollmann, D, Pope, Bg, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Shahmaneche, K, Schmidt, B, Sconza, A, Serrano, M, Sevior, Me, Sillou, D, Sobczynski, C, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stipcevic, M, Stolarczyk, T, Taylor, Gn, Tereshchenko, S, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vo, Mk, Volkov, S, Weber, F, Weisse, T, Werlen, M, Wilson, Ff, Wicht, P, Winton, Lj, Yabsley, Bd, Zaccone, H., Altegoer, J, Anfreville, M, Angelini, C, Astier, P, Authier, M, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Bunyatov, S, Boyd, S, Bueno, A, Camilleri, L, Cardini, A, Castera, A, Cattaneo, Pw, Cavasinni, V, Cavestro, V, Cloue, O, Conforto, G, Conta, C, Cousins, R, De Santo, A, Del Prete, T, Di Lella, L, Dignan, T, Silva, Ede, Donnelly, Lj, Dumarchez, J, Dumps, L, Engster, C, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Fumagalli, G, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Huta, W, Hyett, N, Iacopini, E, Joseph, C, Kirsanov, M, Kekez, D, Khomenko, B, Klimov, O, Kovzelev, A, Kuznetsov, V, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Passerieux, Jp, Pastore, F, Peak, L, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Petitpas, P, Placci, A, Plothow Besch, H, Pluquet, A, Poinsignon, J, Polesello, G, Pollmann, D, Pope, Bg, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, C, Rubbia, A, Salvatore, F, Shahmaneche, K, Schmidt, B, Sconza, A, Serrano, M, Sevior, Me, Sillou, D, Sobczynski, C, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stipcevic, M, Stolarczyk, T, Taylor, Gn, Tereshchenko, S, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vo, Mk, Volkov, S, Weber, F, Weisse, T, Werlen, M, Wilson, Ff, Wicht, P, Winton, Lj, Yabsley, Bd, and Zaccone, H.
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology, High Energy Physics::Experiment
Abstract: The NOMAD experiment is a short base-line search for v(mu) - v(tau) oscillations in the CERN neutrino beam. The v(tau)'s are searched for through their charged current interactions followed by the observation of the resulting tau(-) through its electronic, muonic or hadronic decays. These decays are recognized using kinematical criteria necessitating the use of a light target which enables the reconstruction of individual particles produced in the neutrino interactions. This paper describes the various components of the NOMAD detector: the target and muon drift chambers, the electromagnetic and hadronic calorimeters, the preshower and transition radiation detectors and the veto and trigger scintillation counters. The beam and data acquisition system are also described. The quality of the reconstruction and individual particles is demonstrated through the ability of NOMAD to observe K-s(o)'s, Lambda(o)'s and pi(0)s. Finally, the observation of tau(-) through its electronic decay being one of the most promising channels in the search, the identification of electrons in NOMAD is discussed. (C) 1998 Elsevier Science B.V. All rights reserved.
Published: 1998

24. Test beam performance of the electromagnetic calorimeter of the NOMAD experiment RID C-6672-2008

Author: Autiero D, BaldoCeolin M, Bobisut F, Cattaneo PW, Camilleri L, Cavasinni V, Collazuol G, Conforto G, Conta C, Contalbrigo M, DelPrete T, DeSanto A, Ferrari R, Fraternali M, Gibin D, Gninenko SN, Graziani G, Guglielmi A, Iacopini E, Kovzelev AV, LaRotonda L, Lacaprara S, Lanza A, Laveder M, Lupi A, Martelli F, Mezzetto M, Pastore F, Pennacchio E, Petti R, Polesello G, Rimoldi A, Salvatore F, Sconza A, ValdataNappi M, Veltri M, Vercesi V, Volkov SA, ORESTANO, DOMIZIA, Autiero, D, Baldoceolin, M, Bobisut, F, Cattaneo, Pw, Camilleri, L, Cavasinni, V, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Delprete, T, Desanto, A, Ferrari, R, Fraternali, M, Gibin, D, Gninenko, Sn, Graziani, G, Guglielmi, A, Iacopini, E, Kovzelev, Av, Larotonda, L, Lacaprara, S, Lanza, A, Laveder, M, Lupi, A, Martelli, F, Mezzetto, M, Orestano, Domizia, Pastore, F, Pennacchio, E, Petti, R, Polesello, G, Rimoldi, A, Salvatore, F, Sconza, A, Valdatanappi, M, Veltri, M, Vercesi, V, and Volkov, Sa
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Experiment
Abstract: Test beam results of the NOMAD electromagnetic calorimeter are presented showing linearity, signal uniformity, energy and position resolution measured in an electron beam. Tests were also performed placing the calorimeter in a magnetic field of 0.4 T. Results on the pi rejection obtained using a combined measurement of preshower/electromagnetic calorimeter are found to be in good agreement with the project expectations. Finally the calorimeter response to the muons is discussed.
Published: 1997

25. The electromagnetic calorimeter of the NOMAD experiment RID C-6672-2008

Author: Autiero D, BaldoCeolin M, Barichello G, BianchiBonaiti V, Bobisut F, Cardini A, Cattaneo PW, Cavasinni V, Conta C, DelPrete T, DeSanto A, DiLella L, Ferrari R, Flaminio V, Fraternali M, Gibin D, Gninenko SN, Guglielmi A, Iacopini E, Kovzelev AV, LaRotonda L, Lanza A, Laveder M, Lazzeroni C, Livan M, Mezzetto M, Pastore F, Pennacchio E, Petti R, Polesello G, Renzoni G, Rimoldi A, Roda C, Sconza A, Sobczynski C, ValdataNappi M, Vascon M, Vercesi V, Visentin L, Volkov SA, ORESTANO, DOMIZIA, Autiero, D, Baldoceolin, M, Barichello, G, Bianchibonaiti, V, Bobisut, F, Cardini, A, Cattaneo, Pw, Cavasinni, V, Conta, C, Delprete, T, Desanto, A, Dilella, L, Ferrari, R, Flaminio, V, Fraternali, M, Gibin, D, Gninenko, Sn, Guglielmi, A, Iacopini, E, Kovzelev, Av, Larotonda, L, Lanza, A, Laveder, M, Lazzeroni, C, Livan, M, Mezzetto, M, Orestano, Domizia, Pastore, F, Pennacchio, E, Petti, R, Polesello, G, Renzoni, G, Rimoldi, A, Roda, C, Sconza, A, Sobczynski, C, Valdatanappi, M, Vascon, M, Vercesi, V, Visentin, L, and Volkov, Sa
Subjects: Physics::Instrumentation and Detectors, High Energy Physics::Experiment
Abstract: A description is given of the NOMAD electromagnetic calorimeter, consisting of 875 lead-glass counters read out by two-stage photomultipliers and a low noise electronic chain. The detector operates in a 0.4 T magnetic field transverse to the counter axis. The paper discusses the design criteria, the lead-glass characteristics, the properties of the read out chain and provides a summary of the calorimeter performance.
Published: 1996

26. Final NOMAD results on nu(mu) -> nu(tau) and nu(e) -> nu(tau) oscillations including a new search for nu(tau) appearance using hadronic tau decays

Author: Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sconza, A, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Published: 2001

27. Measurement of the (lambda)over-bar polarization in nu(mu) charged current interactions in the NOMAD experiment

Author: Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Published: 2001

28. A study of backward going p and pi(-) in nu(mu) CC interactions with the NOMAD detector

Author: Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kustov, D, Kuznetsov, V, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Popov, B, Poulsen, C, Rico, J, Riemann, P, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Published: 2001

29. A more sensitive search for nu(mu) -> nu(tau) oscillations in NOMAD

Author: Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gandolfo, A, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Moorhead, Gf, Mossuz, L, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polesello, G, Pollmann, D, Popov, B, Poulsen, C, Rathouit, P, Reno, R, Renzoni, G, Rico, J, Riemann, P, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Schmidt, T, Segneri, G, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Published: 1999

30. Precision measurement of scaled momentum, charge multiplicity, and thrust in nu N-mu and (nu)over-bar(mu)N interactions

Author: Altegoer, J, Angelini, Carlo, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Ballocchi, G, Banner, M, Basa, S, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, Vincenzo, Cervera Villanueva, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, De Santo, A, Del Prete, T, Dignan, T, Di Lella, L, Silva, Ede, Donnelly, Ij, Dumarchez, J, Ellis, M, Fazio, T, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Galumian, P, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas JJ, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kuznetsov, Ve, Lacaprara, S, Lanza, A, La Rotonda, L, Laveder, M, Lazzeroni, C, Letessier Selvon, A, Levy, Jm, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Manola Poggioli, E, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Mishra, Sr, Mossuz, L, Moorhead, Gf, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Nordmann, D, Orestano, D, Pastore, F, Peak, Ls, Pennacchio, E, Perroud, Jp, Pessard, H, Petti, R, Placci, A, Pluquet, A, Polesello, G, Pollmann, D, Popov, B, Poulsen, C, Rathouit, P, Renzoni, G, Roda, CHIARA MARIA ANGELA, Rubbia, A, Salvatore, F, Schahmaneche, K, Schmidt, B, Serrano, M, Sevior, Me, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Steininger, M, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, S, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Uros, V, Vacavant, V, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Verkindt, D, Vieira, Jm, Vinogradova, T, Vo, Mk, Volkov, S, Weber, F, Weisse, T, Werlen, M, Wilson, F, Winton, Lj, Yabsley, Bd, Zaccone, H, Zuber, K, and Zuccon, P.
Published: 1999

31. THE 2009 DECEMBER GAMMA-RAY FLARE OF 3C 454.3: THE MULTIFREQUENCY CAMPAIGN

Author: L. Salotti, E. Moretti, Mark Gurwell, C. Pittori, M. Tavani, S. Vercellone, V. Vittorini, F. Longo, T. Sakamoto, Martino Marisaldi, A. Morselli, M. Galli, P. Santolamazza, G. Barbiellini P. Caraveo, Elena Pian, C. M. Raiteri, M. Pilia, Francesco Lucarelli, A. Trois, A. Rubini, F. D'Ammando, F. Verrecchia, Michael C. Stroh, M. Prest, F. Perotti, Andrea Tiengo, E. Vallazza, P. W. Cattaneo, M. Feroci, Merja Tornikoski, M. Villata, L. Pacciani, P. Picozza, A. Pellizzoni, E. Costa, E. Del Monte, A. Rappoldi, M. Fiorini, Ryosuke Itoh, P. A. Curran, Masayuki Yamanaka, G. Pucella, F. Lazzarotto, Valeri M. Larionov, C. S. Lin, F. Gianotti, A. C. Sadun, A. Giuliani, V. Cocco, Arnaud Ferrari, P. Lipari, M. Trifoglio, M. Fiocchi, E. Morelli, Andrei Berdyugin, G. Piano, H. A. Krimm, Sandro Mereghetti, L. O. Takalo, A. D. Falcone, S. Colafrancesco, Claudio Labanti, D. Zanello, F. Fuschino, D. Fugazza, G. Di Cocco, M. Rapisarda, A. Argan, Andrea Bulgarelli, Makoto Uemura, P. Giommi, Anne Lähteenmäki, G. De Paris, I. Donnarumma, Y. Evangelista, P. Soffitta, A. W. Chen, Paolo Leto, Hugh D. Aller, E. Striani, Mahito Sasada, I. Lapshov, M. F. Aller, S. Sabatini, Pacciani L, Vittorini V, Tavani M, Fiocchi MT, Vercellone S, DAmmando F, Sakamoto T, Pian E, Raiteri CM, Villata M, Sasada M, Itoh R, Yamanaka M, Uemura M, Striani E, Fugazza D, Tiengo A, Krimm HA, Stroh MC, Falcone AD, Curran PA, Sadun AC, Lahteenmaki A, Tornikoski M, Aller HD, Aller MF, Lin CS, Larionov VM, Leto P, Takalo LO, Berdyugin A, Gurwell MA, Bulgarelli A, Chen AW, Donnarumma I, Giuliani A, Longo F, Pucella G, Argan A, Barbiellini G, Caraveo P, Cattaneo PW, Costa E, De Paris G, Del Monte E, Di Cocco G, Evangelista Y, Ferrari A, Feroci M, Fiorini M, Fuschino F, Galli M, Gianotti F, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Marisaldi M, Mereghetti S, Morelli E, Moretti E, Morselli A, Pellizzoni A, Perotti F, Piano G, Picozza P, Pilia M, Prest M, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Trifoglio M, Trois A, Vallazza E, Zanello D, Colafrancesco S, Pittori C, Verrecchia F, Santolamazza P, Lucarelli F, Giommi P, Salotti L, L., Pacciani, V., Vittorini, M., Tavani, M. T., Fiocchi, S., Vercellone, F., D'Ammando, T., Sakamoto, E., Pian, C. M., Raiteri, M., Villata, M., Sasada, R., Itoh, M., Yamanaka, M., Uemura, E., Striani, D., Fugazza, A., Tiengo, H. A., Krimm, M. C., Stroh, A. D., Falcone, P. A., Curran, A. C., Sadun, A., Lahteenmaki, M., Tornikoski, H. D., Aller, M. F., Aller, C. S., Lin, V. M., Larionov, P., Leto, L. O., Takalo, A., Berdyugin, M. A., Gurwell, A., Bulgarelli, A. W., Chen, I., Donnarumma, A., Giuliani, Longo, Francesco, G., Pucella, A., Argan, G., Barbiellini, P., Caraveo, P. W., Cattaneo, E., Costa, G. D., Pari, E. D., Monte, G. D., Cocco, Y., Evangelista, A., Ferrari, M., Feroci, M., Fiorini, F., Fuschino, M., Galli, F., Gianotti, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, M., Marisaldi, S., Mereghetti, E., Morelli, E., Moretti, A., Morselli, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, M., Pilia, M., Prest, M., Rapisarda, A., Rappoldi, A., Rubini, S., Sabatini, P., Soffitta, M., Trifoglio, A., Troi, E., Vallazza, D., Zanello, S., Colafrancesco, C., Pittori, F., Verrecchia, P., Santolamazza, F., Lucarelli, P., Giommi, and L., Salotti
Subjects: Agile, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, galaxies: active, Flux, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, gamma-ray source, High Energy Gamma-ray Astronomy, AGILE satellite, Active Galactic Nuclei, Spectral line, blazar, law.invention, Accretion disc, multi wavelength observation, law, quasars: general, Blazar, media_common, Physics, galaxies: individual (3C 454.3), Gamma ray, Astronomy and Astrophysics, radiation mechanisms: non-thermal, Wavelength, Space and Planetary Science, Sky, Flare
Abstract: During the month of 2009 December, the blazar 3C 454.3 became the brightest gamma-ray source in the sky, reaching a peak flux F 2000 × 10 -8 photons cm-2 s-1 for E > 100 MeV. Starting in 2009 November intensive multifrequency campaigns monitored the 3C 454 gamma-ray outburst. Here, we report on the results of a two-month campaign involving AGILE, INTEGRAL, Swift/XRT, Swift/BAT, and Rossi XTE for the high-energy observations and Swift/UVOT, KANATA, Goddard Robotic Telescope, and REM for the near-IR/optical/UV data. GASP/WEBT provided radio and additional optical data. We detected a long-term active emission phase lasting 1 month at all wavelengths: in the gamma-ray band, peak emission was reached on 2009 December 2-3. Remarkably, this gamma-ray super-flare was not accompanied by correspondingly intense emission in the optical/UV band that reached a level substantially lower than the previous observations in 2007-2008. The lack of strong simultaneous optical brightening during the super-flare and the determination of the broadband spectral evolution severely constrain the theoretical modeling. We find that the pre- and post-flare broadband behavior can be explained by a one-zone model involving synchrotron self-Compton plus external Compton emission from an accretion disk and a broad-line region. However, the spectra of the 2009 December 2-3 super-flare and of the secondary peak emission on 2009 December 9 cannot be satisfactorily modeled by a simple one-zone model. An additional particle component is most likely active during these states. © 2010. The American Astronomical Society. All rights reserved.
Published: 2010
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32. Long-term AGILE monitoring of the puzzling gamma-ray source 3EG J1835+5918

Author: G. De Paris, A. Zambra, F. D'Ammando, M. Feroci, M. Fiorini, Dario Gasparrini, L. Pacciani, F. Longo, A. Rappoldi, E. Vallazza, F. Boffelli, M. Rapisarda, P. Picozza, A. Argan, F. Perotti, E. Del Monte, G. Pucella, A. Trois, Andrea Bulgarelli, I. Donnarumma, T. Froysland, P. Soffitta, A. Pellizzoni, Guido Barbiellini, Enrico Costa, Y. Evangelista, F. Lazzarotto, V. Vittorini, V. Cocco, P. Santolamazza, M. Trifoglio, A. Giuliani, Paolo Lipari, A. W. Chen, P. Giommi, F. Fuschino, S. Vercellone, C. Pittoril, M. Galli, F. Verrecchia, Martino Marisaldi, Sandro Mereghetti, P. W. Cattaneo, P. A. Caraveo, I. Lapshov, M. Prest, S. Colafrancesco, Marco Tavani, G. Piano, A. Morselli, Claudio Labanti, L. Salotti, D. Zanello, M. Marelli, G. Di Cocco, S. Cutini, Fulvio Gianotti, Bulgarelli A, Tavani M, Caraveo P, Chen AW, Gianotti F, Trifoglio M, Marelli M, Argan A, Barbiellini G, Boffelli F, Cattaneo PW, Cocco V, Costa E, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Donnarumma I, Evangelista Y, Feroci M, Fiorini M, Froysland T, Fuschino F, Galli M, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Prest M, Pucella G, Rapisarda M, Rappoldi A, Soffitta P, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Giommi P, Pittori C, Verrecchia F, Santolamazza P, Gasparrini D, Cutini S, Colafrancesco S, Salotti L, A., Bulgarelli, M., Tavani, P., Caraveo, A. W., Chen, F., Gianotti, M., Trifoglio, M., Marelli, A., Argan, G., Barbiellini, F., Boffelli, P. W., Cattaneo, V., Cocco, E., Costa, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, I., Donnarumma, Y., Evangelista, M., Feroci, M., Fiorini, T., Froysland, F., Fuschino, M., Galli, A., Giuliani, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, S., Mereghetti, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, P., Soffitta, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, P., Giommi, C., Pittori, F., Verrecchia, P., Santolamazza, D., Gasparrini, S., Cutini, S., Colafrancesco, and L., Salotti
Subjects: Photon, Field (physics), FOS: Physical sciences, Flux, Field of view, Astrophysics, Unidentified Gamma-ray Source, Power law, High Energy Gamma-ray Astronomy, AGILE gamma ray satellite, 3EG J1835+5918, Egret, Physics, biology, Astrophysics (astro-ph), Gamma ray, Astronomy and Astrophysics, biology.organism_classification, Term (time), Space and Planetary Science, Unidentified Gamma-ray Sources, AGILE satellite, gamma rays: observations
Abstract: We present the AGILE gamma-ray observations of the field containing the puzzling gamma-ray source 3EG J1835+5918. This source is one of the most remarkable unidentified EGRET sources. An unprecedentedly long AGILE monitoring of this source yields important information on the positional error box, flux evolution, and spectrum. 3EG J1835+5918 has been in the AGILE field of view several times in 2007 and 2008 for a total observing time of 138 days from 2007 Sept 04 to 2008 June 30 encompassing several weeks of continuous coverage. With an exposure time approximately twice that of EGRET, AGILE confirms the existence of a prominent gamma-ray source (AGL J1836+5926) at a position consistent with that of EGRET, although with a remarkably lower average flux value for photon energies greater than 100 MeV. A 5-day bin temporal analysis of the whole data set of AGL J1836+5926 shows some evidence for variability of the gamma-ray flux. The source spectrum between 100 MeV and 1 GeV can be fitted with a power law with photon index in the range 1.6-1.7, fully consistent with the EGRET value. The faint X-ray source RX J1836.2+5925 that has been proposed as a possible counterpart of 3EG J1835+5918 is well within the AGILE error box. Future continuous monitoring (both by AGILE and GLAST) is needed to confirm the gamma-ray flux variability and to unveil the source origin, a subject that is currently being pursued through a multiwavelength search for counterparts., Comment: accepted for publication by Astron. & Astrophys, 4 pages, 2 figures, 2 tables
Published: 2008
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33. Direct Evidence for Hadronic Cosmic-Ray Acceleration in the Supernova Renmant IC 443

Author: C. Pittori, Marco Feroci, F. Fuschino, Luigi Pacciani, Paolo Soffitta, G. De Paris, A. Giuliani, E. Scalise, Filippo D'Ammando, V. Cocco, M. Mastropietro, E. Del Monte, V. Vittorini, Arnaud Ferrari, Paolo Lipari, M. Trifoglio, Y. Evangelista, S. Vercellone, F. Perotti, Francesco Lazzarotto, P. Santolamazza, A. Zambra, A. Pellizzoni, G. Di Cocco, E. Striani, I. Lapshov, Fulvio Gianotti, I. Donnarumma, Martino Marisaldi, L. Salotti, Elena Moretti, Alda Rubini, P. W. Cattaneo, A. Rappoldi, A. W. Chen, P. Picozza, P. Giommi, Massimo Rapisarda, G. Pucella, F. Longo, D. Zanello, A. Argan, Andrea Bulgarelli, T. Contessi, Enrico Costa, Claudio Labanti, L. A. Antonelli, G. Piano, P. A. Caraveo, M. Galli, F. Verrecchia, Sandro Mereghetti, A. Morselli, S. Colafrancesco, M. Prest, Alessio Trois, M. Pilia, Marco Tavani, S. Sabatini, Ennio Morelli, G. Barbiellini, E. Vallazza, M., Tavani, A., Giuliani, A. W., Chen, A., Argan, G., Barbiellini, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, V., Cocco, T., Contessi, F., D'Ammando, E., Costa, G. D., Pari, E. D., Monte, G. D., Cocco, I., Donnarumma, Y., Evangelista, A., Ferrari, M., Feroci, F., Fuschino, M., Galli, F., Gianotti, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, M., Mastropietro, S., Mereghetti, E., Morelli, E., Moretti, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, M., Pilia, G., Pucella, M., Prest, M., Rapisarda, A., Rappoldi, E., Scalise, A., Rubini, S., Sabatini, E., Striani, P., Soffitta, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, C., Pittori, F., Verrecchia, P., Santolamazza, P., Giommi, S., Colafrancesco, L. A., Antonelli, L., Salotti, Tavani M, Giuliani A, Chen AW, Argan A, Barbiellini G, Bulgarelli A, Caraveo P, Cattaneo PW, Cocco V, Contessi T, DAmmando F, Costa E, De Paris G, Del Monte E, Di Cocco G, Donnarumma I, Evangelista Y, Ferrari A, Feroci M, Fuschino F, Galli M, Gianotti F, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mastropietro M, Mereghetti S, Morelli E, Moretti E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Pilia M, Pucella G, Prest M, Rapisarda M, Rappoldi A, Scalise E, Rubini A, Sabatini S, Striani E, Soffitta P, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Verrecchia F, Santolamazza P, Giommi P, Colafrancesco S, Antonelli LA, and Salotti L
Subjects: Agile, Photon, Supernova Remnants, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Cosmic ray, Electron, Astrophysics, High Energy Gamma-ray Astronomy, gamma ray production, supernova, Supernova remnant, Astrophysics::Galaxy Astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Molecular cloud, AGILE satellite, Gamma ray, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Supernova, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics - High Energy Astrophysical Phenomena, cosmic rays – gamma rays: general – ISM: supernova remnants – supernovae: general – supernovae: individual (IC 443)
Abstract: The Supernova Remnant (SNR) IC 443 is an intermediate-age remnant well known for its radio, optical, X-ray and gamma-ray energy emissions. In this Letter we study the gamma-ray emission above 100 MeV from IC 443 as obtained by the AGILE satellite. A distinct pattern of diffuse emission in the energy range 100 MeV-3 GeV is detected across the SNR with its prominent maximum (source "A") localized in the Northeastern shell with a flux F = (47 \pm 10) 10^{-8} photons cm^{-2} s^{-1} above 100 MeV. This location is the site of the strongest shock interaction between the SNR blast wave and the dense circumstellar medium. Source "A" is not coincident with the TeV source located 0.4 degree away and associated with a dense molecular cloud complex in the SNR central region. From our observations, and from the lack of detectable diffuse TeV emission from its Northeastern rim, we demonstrate that electrons cannot be the main emitters of gamma-rays in the range 0.1-10 GeV at the site of the strongest SNR shock. The intensity, spectral characteristics, and location of the most prominent gamma-ray emission together with the absence of co-spatial detectable TeV emission are consistent only with a hadronic model of cosmic-ray acceleration in the SNR. A high-density molecular cloud (cloud "E") provides a remarkable "target" for nucleonic interactions of accelerated hadrons: our results show enhanced gamma-ray production near the molecular cloud/shocked shell interaction site. IC 443 provides the first unambiguous evidence of cosmic-ray acceleration by SNRs., Comment: 5 pages, 2 figures; accepted by ApJLetters on Jan 21, 2010
Published: 2010
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34. A year-long AGILE observation of Cygnus X-1 in hard spectral state

Author: A. W. Chen, Francesco Lazzarotto, A. Morselli, Marco Feroci, Luigi Pacciani, E. Striani, S. Vercellone, M. Prest, C. Pittori, I. Lapshov, I. Donnarumma, E. Del Monte, Sandro Mereghetti, A. Argan, M. Galli, P. W. Cattaneo, Piergiorgio Picozza, Massimo Rapisarda, F. Fuschino, Andrea Bulgarelli, F. Perotti, A. Pellizzoni, G. Di Cocco, F. Verrecchia, Enrico Costa, Elena Moretti, Filippo D'Ammando, G. Piano, A. Rappoldi, E. Vallazza, S. Cutini, A. Giuliani, P. A. Caraveo, L. Salotti, Paolo Soffitta, Claudio Labanti, A. Zambra, Francesco Longo, L. A. Antonelli, Guido Barbiellini, Martino Marisaldi, Paolo Lipari, P. Santolamazza, Paolo Giommi, Marco Tavani, S. Sabatini, V. Vittorini, M. Trifoglio, Maura Pilia, Alessio Trois, Fulvio Gianotti, B. Preger, F. Boffelli, Y. Evangelista, G. Pucella, Del Monte E, Feroci M, Evangelista Y, Costa E, Donnarumma I, Lapshov I, Lazzarotto F, Pacciani L, Rapisarda M, Soffitta P, Argan A, Barbiellini G, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen A, DAmmando F, Di Cocco G, Fuschino F, Galli M, Gianotti F, Giuliani A, Labanti C, Lipari P, Longo F, Marisaldi M, Mereghetti S, Moretti E, Morselli A, Pellizzoni A, Perotti F, Piano G, Picozza P, Pilia M, Prest M, Pucella G, Rappoldi A, Sabatini S, Striani E, Tavani M, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Antonelli LA, Cutini S, Pittori C, Preger B, Santolamazza P, Verrecchia F, Giommi P, Salotti L, E. D., Monte, M., Feroci, Y., Evangelista, E., Costa, I., Donnarumma, I., Lapshov, F., Lazzarotto, L., Pacciani, M., Rapisarda, P., Soffitta, A., Argan, G., Barbiellini, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, A., Chen, F., D'Ammando, G. D., Cocco, F., Fuschino, M., Galli, F., Gianotti, A., Giuliani, C., Labanti, P., Lipari, Longo, Francesco, M., Marisaldi, S., Mereghetti, E., Moretti, A., Morselli, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, M., Pilia, M., Prest, G., Pucella, A., Rappoldi, S., Sabatini, E., Striani, M., Tavani, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, L. A., Antonelli, S., Cutini, C., Pittori, B., Preger, P., Santolamazza, F., Verrecchia, P., Giommi, and L., Salotti
Subjects: Agile, Black Holes, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Phase (waves), Flux, FOS: Physical sciences, Astrophysics, cignus, High Energy Gamma-ray Astronomy, X-ray, binaries, silicon detector, Range (statistics), Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Autocorrelation, Gamma ray, Static timing analysis, Astronomy and Astrophysics, stars: individual: Cyg X-1, gamma rays: observations, X-rays: binaries, X-rays: general, Space and Planetary Science, AGILE satellite, Astrophysics - High Energy Astrophysical Phenomena, Energy (signal processing)
Abstract: We present the observation of Cyg X-1 in hard spectral state performed during the AGILE Science Verification Phase and Observing Cycle 1 in hard X-rays (with SuperAGILE) and gamma rays (with the GRID) and lasting for about 160 days with a live time of $\sim 6$ Ms. We investigate the variability of Cyg X-1 in hard X-rays at different timescales, from $\sim 300$ s up to one day, and we apply different tools of timing analysis, such as the autocorrelation function, the first order structure function and the Lomb-Scargle periodogram, to our data (from SuperAGILE) and to the simultaneous data in soft X-rays (from RXTE/ASM). We conclude our investigation with a search for emission in the energy range above 100 MeV with the maximum likelihood technique. In the hard X-ray band the flux of Cyg X-1 shows its typical erratic fluctuations at all timescales with variations of about a factor of two that do not affect significantly the shape of the energy spectrum. From the first order structure function we find that the X-ray emission of Cyg X-1 is characterized by \textit{antipersistence}, indication of a negative feedback mechanism at work. In the gamma ray data a statistically significant point-like source at the position of Cyg X-1 is not found and the upper limit on the flux is $\mathrm{5 \times 10^{-8} \; ph \; cm^{-2} \; s^{-1}}$, over the whole observation (160 days). Finally we compare our upper limit in gamma rays with the expectation of various models of the Cyg X-1 emission, of both hadronic and leptonic origin, in the GeV -- TeV band. The time history of Cyg X-1 in the hard X-ray band over 13 months (not continuous) is shown. Different tools of analysis do not provide fully converging results of the characteristic timescales in the system, suggesting that the timescales found in the structure function are not intrinsic to the physics of the source., Comment: 15 pages and 11 figures (with subfigures). Accepted for publication by A&A.
Published: 2010

35. AGILE detection of intense gamma-ray activity from the blazar PKS 0537-441 in October 2008

Author: Marco Feroci, Luigi Pacciani, F. Boffelli, G. De Paris, E. Vallazza, Martino Marisaldi, Claudio Labanti, C. Pittori, T. Froysland, Domenico Impiombato, Ennio Morelli, A. Zambra, A. Morselli, F. Longo, A. Treves, Fulvio Gianotti, A. W. Chen, P. Caraveo, M. Fiorini, L. Salotti, G. Di Cocco, Francesco Lazzarotto, F. Perotti, E. Del Monte, G. Pucella, M. Perri, Filippo D'Ammando, G. Barbiellini, V. Vittorini, M. Prest, P. Santolamazza, M. Galli, G. Piano, F. Verrecchia, Marco Tavani, P. Giommi, P. W. Cattaneo, A. Argan, I. Donnarumma, Y. Evangelista, Andrea Bulgarelli, A. Pellizzoni, Sandro Mereghetti, Enrico Costa, Maura Pilia, Elena Pian, E. Striani, Alessio Trois, P. Picozza, I. Lapshov, S. Colafrancesco, M. Trifoglio, S. Sabatini, A. Giuliani, D. Zanello, Hans A. Krimm, Massimo Rapisarda, L. A. Antonelli, V. Cocco, A. Rappoldi, Paolo Lipari, F. Fuschino, D. Fugazza, Paolo Soffitta, P. Romano, S. Vercellone, Pucella G, DAmmando F, Romano P, Treves A, Pian E, Vercellone S, Vittorini V, Piano G, Impiombato D, Fugazza D, Verrecchia F, Krimm HA, Donnarumma I, Tavani M, Bulgarelli A, Chen AW, Giuliani A, Longo F, Pacciani L, Argan A, Barbiellini G, Boffelli F, Caraveo P, Cattaneo PW, Cocco V, Costa E, Del Monte E, De Paris G, Di Cocco G, Evangelista Y, Feroci M, Fiorini M, Froysland T, Fuschino F, Galli M, Gianotti F, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Marisaldi M, Mereghetti S, Morelli E, Morselli A, Pellizzoni A, Perotti F, Picozza P, Pilia M, Prest M, Rapisarda M, Rappoldi A, Sabatini S, Soffitta P, Striani E, Trifoglio M, Trois A, Vallazza E, Zambra A, Zanello D, Perri M, Pittori C, Santolamazza P, Giommi P, Antonelli LA, Colafrancesco S, Salotti L, G., Pucella, F., D'Ammando, P., Romano, A., Treve, E., Pian, S., Vercellone, V., Vittorini, G., Piano, D., Impiombato, D., Fugazza, F., Verrecchia, H. A., Krimm, I., Donnarumma, M., Tavani, A., Bulgarelli, A. W., Chen, A., Giuliani, Longo, Francesco, L., Pacciani, A., Argan, G., Barbiellini, F., Boffelli, P., Caraveo, P. W., Cattaneo, V., Cocco, E., Costa, E. D., Monte, G. D., Pari, G. D., Cocco, Y., Evangelista, M., Feroci, M., Fiorini, T., Froysland, F., Fuschino, M., Galli, F., Gianotti, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, M., Marisaldi, S., Mereghetti, E., Morelli, A., Morselli, A., Pellizzoni, F., Perotti, P., Picozza, M., Pilia, M., Prest, M., Rapisarda, A., Rappoldi, S., Sabatini, P., Soffitta, E., Striani, M., Trifoglio, A., Troi, E., Vallazza, A., Zambra, D., Zanello, M., Perri, C., Pittori, P., Santolamazza, P., Giommi, L. A., Antonelli, S., Colafrancesco, and L., Salotti
Subjects: Swift Gamma-Ray Burst Mission, gamma-ray activity, Astrophysics::High Energy Astrophysical Phenomena, Flux, Context (language use), Astrophysics, High Energy Gamma-ray Astronomy, AGILE satellite, Active Galactic Nuclei, law.invention, Luminosity, Telescope, AGILE, X-ray, law, Target of opportunity, gamma rays: general – BL Lacertae objects: individual: PKS 0537-441 – radiation mechanisms: non-thermal, Blazar, Physics, Astronomy, Astronomy and Astrophysics, Gamma-Ray Imaging Detector, Space and Planetary Science, Spectral energy distribution
Abstract: Context. We report the detection by the AGILE satellite of intense gamma-ray activity from the source 1AGL J0538-4424, associated with the low-energy-peaked BL Lac PKS 0537-441, during a target of opportunity (ToO) observation performed on 2008 October 10-17, triggered by a Fermi-LAT alert, together with REM and Swift observations. Aims. The quasi-simultaneous near-infrared, optical, UV, X-ray, and gamma-ray coverage allowed us to investigate the behaviour of the source in different energy bands and study the spectral energy distribution and a theoretical model that can describe the gamma-ray state observed in mid-October. Methods. AGILE observed the source with its two co-aligned imagers: the Gamma-Ray Imaging Detector (GRID) and the hard X-ray imager (SuperAGILE), sensitive in the 30 MeV-30 GeV and 18-60 keV ranges, respectively. During the AGILE observation, the source was monitored simultaneously in the UV and X-ray bands by the Swift satellite through 6 ToO observations carried out between 2008 October 8 and 17. Moreover, the source was observed in the near-infrared and optical bands by the REM telescope on 2008 October 7, 8, and 9. Results. During 2008 October 10-17, AGILE-GRID detected gamma-ray emission from PKS 0537-441 at a significance level of 5.3-sigma with an average flux of (42 +/- 11) x 10(-8) photons cm(-2) s(-1) for energies higher than 100 MeV. A significant increase in the gamma-ray activity was detected between the first and the second halves of the observing period. REM and Swift/XRT detected the source in near-infrared/optical and X-rays during a relatively low and intermediate activity state, respectively, with no signs of evident variability in the different observations. However, Swift/UVOT detected an increase between the first and the second parts of the observing period, smaller than in the gamma-rays. Conclusions. The average gamma-ray flux of PKS 0537-441 detected by AGILE is close to the average flux observed for this source by the EGRET and Fermi-LAT instruments, with an increase of a factor 3 throughout the observation period up to a flux level slightly lower than the highest flux observed by Fermi-LAT during the first 11 months of operation. The spectral energy distribution of PKS 0537-441 in mid-October 2008 seems to require two synchrotron self-Compton components to be modelled, to account for both the near-infrared/optical bump and the X-ray data, together with the information on the gamma-ray flux level observed by AGILE. An alternative model based on the external Compton radiation, which requires an accretion disk with a relatively high luminosity, is also proposed.
Published: 2010

36. Extreme particle acceleration in the microquasar Cygnus X-3

Author: Francesco Longo, Martino Marisaldi, C. Pittori, Paolo Lipari, Arnaud Ferrari, M. Prest, Sandro Mereghetti, P. W. Cattaneo, S. Sabatini, A. Pellizzoni, E. Striani, I. Lapshov, F. Perotti, S. Colafrancesco, Fulvio Gianotti, Francesco Lazzarotto, A. Giuliani, E. Rossi, Ennio Morelli, Karri I. I. Koljonen, Marco Tavani, E. Scalise, Y. Evangelista, Maura Pilia, Guy G. Pooley, M. Galli, F. Fuschino, Alessio Trois, I. Donnarumma, Massimo Rapisarda, F. Verrecchia, N. A. Nizhelskij, P. A. Caraveo, E. Del Monte, D. Zanello, L. Salotti, V. Cocco, M. Trifoglio, G. Pucella, A. Mauri, A. Rappoldi, E. Vallazza, G. De Paris, T. Contessi, G. Piano, A. W. Chen, P. Giommi, A. Argan, Andrea Bulgarelli, Enrico Costa, G. Di Persio, A. Morselli, Filippo D'Ammando, Paolo Soffitta, S. Vercellone, Michael L. McCollough, P. Picozza, P. Santolamazza, Alda Rubini, Sergei A. Trushkin, A. Zambra, M. Mastropietro, Guido Barbiellini, V. Vittorini, Marco Feroci, Luigi Pacciani, Angelo Antonelli, E. Mattaini, G. Di Cocco, Claudio Labanti, M., Tavani, A., Bulgarelli, G., Piano, S., Sabatini, E., Striani, Y., Evangelista, A., Troi, G., Pooley, S., Trushkin, N. A., Nizhelskij, M., Mccollough, K. I. I., Koljonen, G., Pucella, A., Giuliani, A. W., Chen, E., Costa, V., Vittorini, M., Trifoglio, F., Gianotti, A., Argan, G., Barbiellini, P., Caraveo, P. W., Cattaneo, V., Cocco, T., Contessi, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, G. D., Persio, I., Donnarumma, M., Feroci, A., Ferrari, F., Fuschino, M., Galli, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, E., Mattaini, M., Marisaldi, M., Mastropietro, A., Mauri, S., Mereghetti, E., Morelli, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, P., Picozza, M., Pilia, M., Prest, M., Rapisarda, A., Rappoldi, E., Rossi, A., Rubini, E., Scalise, P., Soffitta, E., Vallazza, S., Vercellone, A., Zambra, D., Zanello, C., Pittori, F., Verrecchia, P., Giommi, S., Colafrancesco, P., Santolamazza, A., Antonelli, L., Salotti, Tavani M, Bulgarelli A, Piano G, Sabatini S, Striani E, Evangelista Y, Trois A, Pooley G, Trushkin S, Nizhelskij NA, McCollough M, Koljonen KII, Pucella G, Giuliani A, Chen AW, Costa E, Vittorini V, Trifoglio M, Gianotti F, Argan A, Barbiellini G, Caraveo P, Cattaneo PW, Cocco V, Contessi T, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Feroci M, Ferrari A, Fuschino F, Galli M, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mastropietro M, Mauri A, Mereghetti S, Morelli E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Pilia M, Prest M, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Scalise E, Soffitta P, Vallazza E, Vercellone S, Zambra A, Zanello D, Pittori C, Verrecchia F, Giommi P, Colafrancesco S, Santolamazza P, Antonelli A, and Salotti L
Subjects: Active galactic nucleus, Black Holes, Astrophysics::High Energy Astrophysical Phenomena, super massive black holes, X-ray binary, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, High Energy Gamma-ray Astronomy, Relativistic particle, AGILE, Astrophysical jet, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Galaxy Astrophysics, Physics, Supermassive black hole, Cygnus, Multidisciplinary, particle acceleration, microquasar, Cygnus X-3, Astronomy, X-ray emission, Particle acceleration, Black hole, Neutron star, AGILE satellite
Abstract: Galactic microquasars are binaries with a neutron star or stellar-mass black hole accreting gas from a companion star. They can accelerate particles to relativistic energies and emit radio flares, but the mechanism of jet energization is not known. A survey of the Cygnus region between mid-2007 and mid-2009 has detected four major γ-ray flaring episodes with energies over 100 MeV, each lasting 1 or 2 days, emanating from the microquasar Cygnus X-3. There is a clear pattern of temporal correlation between the γ-ray flares and transitional spectral states of radio and X-ray emission. Particle acceleration occurred a few days before radio jet ejections for two of the flares, suggesting that jet formation involves the production of highly energetic particles. Super-massive black holes in active galaxies can accelerate particles to relativistic energies, producing jets with associated γ-ray emission. Galactic 'microquasars' also produce relativistic jets; however, apart from an isolated event detected in Cygnus X-1, there has hitherto been no systematic evidence for the acceleration of particles to gigaelectronvolt or higher energies in a microquasar. Here, a report of four γ-ray flares with energies above 100 MeV from the microquasar Cygnus X-3 illuminates this important problem. Super-massive black holes in active galaxies can accelerate particles to relativistic energies1, producing jets with associated γ-ray emission. Galactic ‘microquasars’, which are binary systems consisting of a neutron star or stellar-mass black hole accreting gas from a companion star, also produce relativistic jets, generally together with radio flares2. Apart from an isolated event detected3 in Cygnus X-1, there has hitherto been no systematic evidence for the acceleration of particles to gigaelectronvolt or higher energies in a microquasar, with the consequence that we are as yet unsure about the mechanism of jet energization. Here we report four γ-ray flares with energies above 100 MeV from the microquasar Cygnus X-3 (an exceptional X-ray binary4,5,6 that sporadically produces radio jets7,8,9). There is a clear pattern of temporal correlations between the γ-ray flares and transitional spectral states of the radio-frequency and X-ray emission. Particle acceleration occurred a few days before radio-jet ejections for two of the four flares, meaning that the process of jet formation implies the production of very energetic particles. In Cygnus X-3, particle energies during the flares can be thousands of times higher than during quiescent states.
Published: 2009

37. Monitoring the hard X-ray sky with SuperAGILE

Author: S. Cutini, S. Stellato, M. Trifoglio, Ennio Morelli, G. De Paris, Martino Marisaldi, Massimiliano Fiorini, F. Boffelli, G. Fanari, F. Fuschino, F. Fornari, C. Pittori, I. Donnarumma, T. Froysland, A. W. Chen, F. Liello, F. Perotti, A. Pellizzoni, Francesco Longo, Attilio Ferrari, A. Morselli, Guido Barbiellini, V. Vittorini, A. Antonelli, G. Pucella, A. Argan, Alessandro Traci, Marco Tavani, S. Sabatini, Andrea Bulgarelli, Sergio Colafrancesco, Enrico Costa, F. Mauri, Sandro Mereghetti, Francesco Lazzarotto, P. W. Cattaneo, M. Prest, R. Primavera, M. Galli, Piergiorgio Picozza, F. Tamburelli, P. Santolamazza, F. Verrecchia, Paolo Lipari, Elena Moretti, Marco Feroci, Luigi Pacciani, Alda Rubini, I. Lapshov, A. Mauri, Paolo Giommi, F. D'Ammando, A. Rappoldi, E. Vallazza, V. Cocco, A. Giuliani, P. A. Caraveo, Dario Gasparrini, Y. Evangelista, G. Piano, L. Salotti, A. Zambra, C. Pontoni, E. Rossi, Massimo Rapisarda, D. Zanello, Claudio Labanti, E. Del Monte, E. Mattaini, G. Di Cocco, Massimo Frutti, S. Vercellone, G. Di Persio, Paolo Soffitta, B. Preger, Marcello Mastropietro, Maura Pilia, Alessio Trois, Fulvio Gianotti, Geiland Porrovecchio, M., Feroci, E., Costa, E. D., Monte, I., Donnarumma, Y., Evangelista, I., Lapshov, F., Lazzarotto, L., Pacciani, M., Rapisarda, P., Soffitta, G. D., Persio, M., Frutti, M., Mastropietro, E., Morelli, G., Porrovecchio, A., Rubini, A., Antonelli, A., Argan, G., Barbiellini, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, S., Colafrancesco, S., Cutini, F., D'Ammando, G. D., Pari, G. D., Cocco, G., Fanari, A., Ferrari, M., Fiorini, F., Fornari, F., Fuschino, T., Froysland, M., Galli, D., Gasparrini, F., Gianotti, P., Giommi, A., Giuliani, C., Labanti, F., Liello, P., Lipari, Longo, Francesco, E., Mattaini, M., Marisaldi, A., Mauri, F., Mauri, S., Mereghetti, E., Moretti, A., Morselli, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, M., Pilia, C., Pittori, C., Pontoni, B., Preger, M., Prest, R., Primavera, G., Pucella, A., Rappoldi, E., Rossi, S., Sabatini, P., Santolamazza, M., Tavani, S., Stellato, F., Tamburelli, A., Traci, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, F., Verrecchia, V., Vittorini, A., Zambra, D., Zanello, L., Salotti, Feroci M, Costa E, Del Monte E, Donnarumma I, Evangelista Y, Lapshov I, Lazzarotto F, Pacciani L, Rapisarda M, Soffitta P, Di Persio G, Frutti M, Mastropietro M, Morelli E, Porrovecchio G, Rubini A, Antonelli A, Argan A, Barbiellini G, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Colafrancesco S, Cutini S, DAmmando F, De Paris G, Di Cocco G, Fanari G, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Galli M, Gasparrini D, Gianotti F, Giommi P, Giuliani A, Labanti C, Liello F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mauri A, Mauri F, Mereghetti S, Moretti E, Morselli A, Pellizzoni A, Perotti F, Piano G, Picozza P, Pilia M, Pittori C, Pontoni C, Preger B, Prest M, Primavera R, Pucella G, Rappoldi A, Rossi E, Sabatini S, Santolamazza P, Tavani M, Stellato S, Tamburelli F, Traci A, Trifoglio M, Trois A, Vallazza E, Vercellone S, Verrecchia F, Vittorini V, Zambra A, Zanello D, and Salotti L
Subjects: Agile, Photon, High Energy Gamma-ray Astronomy, AGILE satellite, X-ray sources, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Field of view, SuperAgile, x-ray detector, extragalactic and galactic sources, Optics, Angular resolution, Instrumentation and Methods for Astrophysics (astro-ph.IM), media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), COSMIC cancer database, business.industry, Detector, Gamma ray, Astronomy and Astrophysics, instrumentation: detectors – X-rays: binaries – X-rays: general, Space and Planetary Science, Sky, Celestial coordinate system, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: SuperAGILE is the hard X-ray monitor of the AGILE gamma ray mission, in orbit since 23$^{rd}$ April 2007. It is an imaging experiment based on a set of four independent silicon strip detectors, equipped with one-dimensional coded masks, operating in the nominal energy range 18-60 keV. The main goal of SuperAGILE is the observation of cosmic sources simultaneously with the main gamma-ray AGILE experiment, the Gamma Ray Imaging Detector (GRID). Given its $\sim$steradian-wide field of view and its $\sim$15 mCrab day-sensitivity, SuperAGILE is also well suited for the long-term monitoring of Galactic compact objects and the detection of bright transients. The SuperAGILE detector properties and design allow for a 6 arcmin angular resolution in each of the two independent orthogonal projections of the celestial coordinates. Photon by photon data are continuously available by the experiment telemetry, and are used to derive images and fluxes of individual sources, with integration times depending on the source intensity and position in the field of view. In this paper we report on the main scientific results achieved by SuperAGILE over its first two years in orbit, until April 2009., Comment: Accepted for publication on Astronomy & Astrophysics
Published: 2009
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38. Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

Author: A. Pellizzoni, M. Galli, A. Giuliani, F. Verrecchia, Francesco Lazzarotto, E. Vallazza, C. Pittori, T. Contessi, N. D'Amico, G. Piano, G. De Paris, A. Argan, Sandro Mereghetti, E. Rossi, E. Scalise, A. Morselli, Arnaud Ferrari, E. Striani, P. Santolamazza, Andrea Bulgarelli, F. Fuschino, I. Lapshov, S. Colafrancesco, L. Salotti, I. Donnarumma, Y. Evangelista, Massimo Rapisarda, G. Di Cocco, A. Possenti, Enrico Costa, S. Sabatini, Alda Rubini, P. W. Cattaneo, G. Pucella, P. Picozza, Marco Tavani, G. Barbiellini, Elena Moretti, Martino Marisaldi, A. Rappoldi, D. Zanello, M. Prest, V. Cocco, M. Mastropietro, F. Perotti, M. Burgay, V. Vittorini, A. W. Chen, Claudio Labanti, A. Zambra, Paolo Lipari, P. Giommi, J. Palfreyman, Giovanni F. Bignami, P. A. Caraveo, M. Trifoglio, M. Fiorini, E. Del Monte, Aidan Hotan, F. Longo, Angelo Antonelli, Marco Feroci, Luigi Pacciani, Maura Pilia, Alessio Trois, Paolo Esposito, Fulvio Gianotti, G. Di Persio, Filippo D'Ammando, Paolo Soffitta, S. Vercellone, Pellizzoni A, Trois A, Tavani M, Pilia M, Giuliani A, Pucella G, Esposito P, Sabatini S, Piano G, Argan A, Barbiellini G, Bulgarelli A, Burgay M, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Contessi T, Costa E, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fuschino F, Galli M, Gianotti F, Hotan A, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mastropietro M, Mereghetti S, Moretti E, Morselli A, Pacciani L, Palfreyman J, Perotti F, Picozza P, Pittori C, Possenti A, Prest M, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Santolamazza P, Scalise E, Soffitta P, Striani E, Trifoglio M, Vallazza E, Vercellone S, Verrecchia F, Vittorini V, Zambra A, Zanello D, Giommi P, Colafrancesco S, Antonelli A, Salotti L, D'Amico N, Bignami GF, A., Pellizzoni, A., Troi, M., Tavani, M., Pilia, A., Giuliani, G., Pucella, P., Esposito, S., Sabatini, G., Piano, A., Argan, G., Barbiellini, A., Bulgarelli, M., Burgay, P., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, T., Contessi, E., Costa, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, G. D., Persio, I., Donnarumma, Y., Evangelista, M., Feroci, A., Ferrari, M., Fiorini, F., Fuschino, M., Galli, F., Gianotti, A., Hotan, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, M., Mastropietro, S., Mereghetti, E., Moretti, A., Morselli, L., Pacciani, J., Palfreyman, F., Perotti, P., Picozza, C., Pittori, A., Possenti, M., Prest, M., Rapisarda, A., Rappoldi, E., Rossi, A., Rubini, P., Santolamazza, E., Scalise, P., Soffitta, E., Striani, M., Trifoglio, E., Vallazza, S., Vercellone, F., Verrecchia, V., Vittorini, A., Zambra, D., Zanello, P., Giommi, S., Colafrancesco, A., Antonelli, L., Salotti, N., D'Amico, and G. F., Bignami
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Population, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Vela, Pulsar wind nebula, High Energy Gamma-ray Astronomy, gamma detection, Relativistic particle, AGILE, Pulsar Wind Nebulae, Pulsar, Astrophysics::Solar and Stellar Astrophysics, AGILE satellite, education, Astrophysics::Galaxy Astrophysics, pulsar, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), education.field_of_study, Multidisciplinary, Vela Pulsar Wind Nebula, AGILE, gamma-rays, Gamma ray, Astronomy, Physics::Space Physics, Astrophysics - High Energy Astrophysical Phenomena, Phenomenology (particle physics), X-ray pulsar
Abstract: Pulsars are known to power winds of relativistic particles that can produce bright nebulae by interacting with the surrounding medium. These pulsar wind nebulae (PWNe) are observed in the radio, optical, x-rays and, in some cases, also at TeV energies, but the lack of information in the gamma-ray band prevents from drawing a comprehensive multiwavelength picture of their phenomenology and emission mechanisms. Using data from the AGILE satellite, we detected the Vela pulsar wind nebula in the energy range from 100 MeV to 3 GeV. This result constrains the particle population responsible for the GeV emission, probing multivavelength PWN models, and establishes a class of gamma-ray emitters that could account for a fraction of the unidentified Galactic gamma-ray sources., Comment: Accepted by Science; first published online on December 31, 2009 in Science Express. Science article and Supporting Online Material are available at http://www.sciencemag.org
Published: 2009
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39. A measurement of coherent neutral pion production in neutrino neutral current interactions in the NOMAD experiment

Author: Marco Fraternali, A. Placci, J. A. Hernando, M. Mezzetto, A. De Santo, Alexander Toropin, Kai Zuber, G. Bassompierre, S. Boyd, B. Lakić, G. N. Taylor, L. S. Peak, O.L. Klimov, V. Flaminio, F. J. P. Soler, J. Long, K. Benslama, T. Vinogradova, F. Bobisut, Antonio Bueno, A.-M. Touchard, A. Cervera-Villanueva, Kevin Varvell, L. Camilleri, Vyacheslav Valuev, J.M. Gaillard, C. Lachaud, Giacomo Graziani, V. V. Lyubushkin, M. T. Tran, D. Steele, Nathalie Besson, E. Gangler, Mikhail Kirsanov, R. Cousins, Barry Blumenfeld, A.M. Scott, A. Grant, H. Pessard, P. Nedelec, T. Weisse, J. Kokkonen, Malcolm Ellis, R. Challis, J.-P. Mendiburu, Q. Wu, S.A. Bunyatov, A. Marchionni, J.-M. Vieira, U. Stiegler, E. Pennacchio, I. Bird, D. Geppert, J. Rico, P.W. Cattaneo, Ante Ljubičić, F. Vannucci, E. do Couto e Silva, N. Hyett, R. Petti, D. Pollmann, P. Astier, J. Bouchez, L. Linssen, J.J. Gómez-Cadenas, André Rubbia, O. Samoylov, Alessandro Cardini, X.C. Tian, A. Baldisseri, Sergey Alekhin, Roberto Ferrari, V. Tereshchenko, F. Salvatore, B. A. Popov, Alexey Krasnoperov, D. Autiero, D. Sillou, Yu. Nefedov, L. Vacavant, F.V. Weber, Frédéric Juget, Chiara Roda, P. Zuccon, J. Gosset, A. Lupi, E. Iacopini, Caroline Poulsen, H. Zaccone, Luca Rebuffi, Artem Chukanov, Bruce Yabsley, Claus Gößling, X. Méchain, A. Guglielmi, D. Gibin, C. Joseph, Vincenzo Cavasinni, G. Vidal-Sitjes, M. Baldo-Ceolin, A. Polyarush, C. Conta, B. Schmidt, H. Degaudenzi, G. J. Feldman, Achim Geiser, G. F. Moorhead, G. Conforto, J. Dumarchez, Marco Laveder, Didier Ferrere, Th. Stolarczyk, M. Banner, Valerio Vercesi, Dmitry V. Naumov, M. E. Sevior, K. Schahmaneche, Sergei Gninenko, C.T. Kullenberg, P. Hurst, L. Di Lella, M. Valdata-Nappi, E. Tsesmelis, Caren Hagner, Domizia Orestano, J.J. Kim, T. Schmidt, A. Kovzelev, A. Godley, M. Contalbrigo, J. M. Levy, Sergey A. Kulagin, G. Collazuol, Mario Stipčević, M. Veltri, J-P. Meyer, L.J. Winton, A. Sconza, J. Ulrichs, M.B. Seaton, L. La Rotonda, S. R. Mishra, A. Lanza, G. Sozzi, P. Riemann, Stefano Lacaprara, Fergus Wilson, A. Letessier-Selvon, Giacomo Polesello, M. Tareb-Reyes, Michel Gouanère, F. Martelli, N. Kent, C. Nguyen-Mau, T. Del Prete, S.N. Tovey, Fr Pastore, Kullenberg, Ct, Mishra, Sr, Seaton, Mb, Kim, Jj, Tian, Xc, Scott, Am, Kirsanov, M, Petti, R, Alekhin, S, Astier, P, Autiero, D, Baldisseri, A, Baldo Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Camilleri, L, Cardini, A, Cattaneo, Pw, Cavasinni, V, Cervera Villanueva, A, Challis, R, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Degaudenzi, H, De Santo, A, Del Prete, T, Di Lella, L, Silva, Ede, Dumarchez, J, Ellis, M, Feldman, Gj, Ferrari, R, Ferrere, D, Flaminio, V, Fraternali, M, Gaillard, Jm, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez Cadenas, Jj, Gosset, J, Gossling, C, Gouanere, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kent, N, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kulagin, S, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier Selvon, A, Levy, Jm, Ling, J, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Lyubushkin, V, Marchionni, A, Martelli, F, Mechain, X, Mendiburu, Jp, Meyer, Jp, Mezzetto, M, Moorhead, Gf, Naumov, D, Nedelec, P, Nefedov, Y, Nguyen Mau, C, Orestano, Domizia, Pastore, F, Peak, L, Pennacchio, E, Pessard, H, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Poulsen, C, Popov, B, Rebuffi, L, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Samoylov, O, Schahmaneche, K, Schmidt, B, Schmidt, T, Sconza, A, Sevior, M, Sillou, D, Soler, Fjp, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, T, Tareb Reyes, M, Taylor, Gn, Tereshchenko, V, Toropin, A, Touchard, Am, Tovey, Sn, Tran, Mt, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata Nappi, M, Valuev, V, Vannucci, F, Varvell, Ke, Veltri, M, Vercesi, V, Vidal Sitjes, G, Vieira, Jm, Vinogradova, T, Weber, Fv, Weisse, T, Wilson, Ff, Winton, Lj, Wu, Q, Yabsley, Bd, Zaccone, H, Zuber, K, Zuccon, P., Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Neutrinos, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), NOMAD, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire d'Annecy de Physique des Particules (LAPP), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Particle physics, Nuclear and High Energy Physics, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Pion, Coherent pion neutrino neutral current, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Nuclear Experiment, Charged current, Physics, Range (particle radiation), Large Hadron Collider, Neutral current, 010308 nuclear & particles physics, Scattering, Física, Deep inelastic scattering, coherent pion, neutrino, neutral current, High Energy Physics::Experiment, Neutrino, Particle Physics - Experiment
Abstract: We present a study of exclusive neutral pion production in neutrino-nucleus Neutral Current interactions using data from the NOMAD experiment at the CERN SPS. The data correspond to $1.44 \times 10^6$ muon-neutrino Charged Current interactions in the energy range $2.5 \leq E_{\nu} \leq 300$ GeV. Neutrino events with only one visible $\pi^0$ in the final state are expected to result from two Neutral Current processes: coherent $\pi^0$ production, {\boldmath $\nu + {\cal A} \to \nu + {\cal A} + \pi^0$} and single $\pi^0$ production in neutrino-nucleon scattering. The signature of coherent $\pi^0$ production is an emergent $\pi^0$ almost collinear with the incident neutrino while $\pi^0$'s produced in neutrino-nucleon deep inelastic scattering have larger transverse momenta. In this analysis all relevant backgrounds to the coherent $\pi^0$ production signal are measured using data themselves. Having determined the backgrounds, and using the Rein-Sehgal model for the coherent $\pi^0$ production to compute the detection efficiency, we obtain {\boldmath $4630 \pm 522 (stat) \pm 426 (syst)$} corrected coherent-$\pi^0$ events with $E_{\pi^0} \geq 0.5$ GeV. We measure {\boldmath $\sigma (\nu {\cal A} \to \nu {\cal A} \pi^0) = [ 72.6 \pm 8.1(stat) \pm 6.9(syst) ] \times 10^{-40} cm^2/nucleus$}. This is the most precise measurement of the coherent $\pi^0$ production to date., Comment: 23 pages, 9 figures, accepted for publication in Phys. Lett. B
Published: 2009
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40. AGILE detection of intense gamma-ray emission from the blazar PKS 1510-089

Author: C. Pittori, T. Froysland, A. Pellizzoni, Alessio Trois, Margo F. Aller, H. D. Aller, F. Boffelli, Filippo D'Ammando, Marco Feroci, D. Zanello, Luigi Pacciani, G. Pucella, F. Perotti, Fulvio Gianotti, C. M. Raiteri, A. Rappoldi, E. Vallazza, E. Del Monte, Francesco Longo, A. W. Chen, G. De Paris, V. Cocco, Francesco Lazzarotto, Y. Evangelista, Marco Tavani, S. Cutini, G. Di Cocco, M. Prest, Sergio Colafrancesco, M. Villata, L. A. Antonelli, Sandro Mereghetti, P. W. Cattaneo, I. Donnarumma, A. Argan, M. Fiorini, Massimo Rapisarda, D. Carosati, P. Lipari, Andrea Bulgarelli, Dario Gasparrini, F. Fuschino, Enrico Costa, Martino Marisaldi, V. Vittorini, Valeri M. Larionov, M. Trifoglio, A. Giuliani, I. Lapshov, A. Morselli, P. A. Caraveo, Claudio Labanti, M. Galli, Piergiorgio Picozza, F. Verrecchia, L. Salotti, A. Zambra, Guido Barbiellini, R. Ligustri, Paolo Giommi, S. Vercellone, Paolo Soffitta, G., Pucella, V., Vittorini, F., D'Ammando, M., Tavani, C. M., Raiteri, M., Villata, A., Argan, G., Barbiellini, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, E., Costa, E., Delmonte, G. D., Pari, G. D., Cocco, I., Donnarumma, Y., Evangelista, M., Feroci, M., Fiorini, T., Froysland, F., Fuschino, M., Galli, F., Gianotti, A., Giuliani, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, S., Mereghetti, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, P., Picozza, M., Prest, M., Rapisarda, A., Rappoldi, P., Soffitta, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, A., Zambra, D., Zanello, L. A., Antonelli, S., Colafrancesco, S., Cutini, D., Gasparrini, P., Giommi, C., Pittori, F., Verrecchia, L., Salotti, M. F., Aller, H. D., Aller, D., Carosati, V. M., Larionov, R., Ligustri, Pucella G, Vittorini V, DAmmando F, Tavani M, Raiteri CM, Villata M, Argan A, Barbiellini G, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, DelMonte E, De Paris G, Di Cocco G, Donnarumma I, Evangelista Y, Feroci M, Fiorini M, Froysland T, Fuschino F, Galli M, Gianotti F, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Prest M, Rapisarda M, Rappoldi A, Soffitta P, Trifoglio M, Trois A, Vallazza E, Vercellone S, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Gasparrini D, Giommi P, Pittori C, Verrecchia F, Salotti L, Aller MF, Aller HD, Carosati D, Larionov VM, and Ligustri R
Subjects: High Energy Gamma-ray Astronomy, Active Galactic Nuclei, AGILE satellite, Photon, Astrophysics::High Energy Astrophysical Phenomena, satellite, FOS: Physical sciences, Astrophysics, Photon energy, law.invention, Telescope, AGILE, law, gamma ray satellite, quasar, Blazar, Physics, Astrophysics (astro-ph), Gamma ray, Astronomy and Astrophysics, Quasar, gamma rays: observations -- radiation mechanisms: non-thermal -- quasars: individual: PKS 1510-089, Space and Planetary Science, Spectral energy distribution, Flare
Abstract: We report the detection by the AGILE (Astro-rivelatore Gamma a Immagini LEggero) satellite of an intense gamma-ray flare from the source AGL J1511-0909, associated with the powerful quasar PKS 1510-089, during ten days of observations from 23 August to 1 September 2007. During the observation period, the source was in optical decrease following a flaring event monitored by the GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT). The simultaneous gamma-ray, optical, and radio coverage allows us to study the spectral energy distribution and the theoretical models based on the synchrotron and inverse Compton (IC) emission mechanisms. AGILE observed the source with its two co-aligned imagers, the Gamma-Ray Imaging Detector and the hard X-ray imager Super-AGILE sensitive in the 30 MeV - 50 GeV and 18 - 60 keV bands, respectively. Between 23 and 27 August 2007, AGILE detected gamma-ray emission from PKS 1510-089 when this source was located about 50 degrees off-axis, with an average flux of (270 +/- 65) x 10^{-8} photons cm^{-2} s^{-1} for photon energy above 100 MeV. In the following period, 28 August - 1 September, after a satellite re-pointing, AGILE detected the source at about 35 degrees off-axis, with an average flux (E > 100 MeV) of (195 +/- 30) x 10^{-8} photons cm^{-2} s^{-1}. No emission was detected by Super-AGILE, with a 3-sigma upper limit of 45 mCrab in 200 ksec. The spectral energy distribution is modelled with a homogeneous one-zone synchrotron self Compton (SSC) emission plus contributions by external photons: the SSC emission contributes primarily to the X-ray band, whereas the contribution of the IC from the external disc and the broad line region match the hard gamma-ray spectrum observed., 5 pages, 5 figures, accepted for publication in A&A
Published: 2008
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41. Multiwavelength observations of 3C 454.3. I. The AGILE 2007 November campaign on the 'Crazy Diamond'

Author: P. Santolamazza, I. Donnarumma, Francesco Longo, M. Galli, A. Argan, P. Romano, Piergiorgio Picozza, F. Verrecchia, S. Vercellone, L. Salotti, A. Zambra, Andrea Bulgarelli, G. De Paris, Paolo Giommi, Francesco Lazzarotto, V. Cocco, Sandro Mereghetti, Enrico Costa, P. W. Cattaneo, Paolo Soffitta, Filippo D'Ammando, G. Barbiellini, G. Novara, C. M. Raiteri, F. Fornari, Attilio Ferrari, Massimo Rapisarda, G. Di Cocco, A. Morselli, F. Senziani, Angela Bazzano, Y. Evangelista, Claudio Labanti, Mariateresa Fiocchi, F. Fuschino, C. Pittori, A. Rappoldi, T. Froysland, Gino Tosti, S. Cutini, Andrea Belfiore, Marco Tavani, Wen Ping Chen, A. W. Chen, A. Pellizzoni, Sergio Colafrancesco, P. Lipari, E. Del Monte, A. Giuliani, Massimiliano Fiorini, Dario Gasparrini, I. Lapshov, F. Boffelli, Alessio Trois, Marco Feroci, Luigi Pacciani, D. Impiombato, Pietro Ubertini, V. Vittorini, M. Trifoglio, D. Zanello, B. Preger, Fulvio Gianotti, E. Vallazza, G. Pucella, F. Perotti, A. De Luca, P. A. Caraveo, M. Prest, M. Villata, Martino Marisaldi, S., Vercellone, A. W., Chen, V., Vittorini, A., Giuliani, F., D'Ammando, M., Tavani, I., Donnarumma, G., Pucella, C. M., Raiteri, M., Villata, W. P., Chen, G., Tosti, D., Impiombato, P., Romano, A., Belfiore, A. D., Luca, G., Novara, F., Senziani, A., Bazzano, M. T., Fiocchi, P., Ubertini, A., Ferrari, A., Argan, G., Barbiellini, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, V., Cocco, E., Costa, E. D., Monte, G. D., Pari, G. D., Cocco, Y., Evangelista, M., Feroci, M., Fiorini, F., Fornari, T., Froysland, F., Fuschino, M., Galli, F., Gianotti, C., Labanti, I., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, S., Mereghetti, A., Morselli, A., Pellizzoni, L., Pacciani, F., Perotti, P., Picozza, M., Prest, M., Rapisarda, A., Rappoldi, P., Soffitta, M., Trifoglio, A., Troi, E., Vallazza, A., Zambra, D., Zanello, C., Pittori, F., Verrecchia, P., Santolamazza, B., Preger, D., Gasparrini, S., Cutini, P., Giommi, S., Colafrancesco, L., Salotti, Vercellone S, Chen AW, Vittorini V, Giuliani A, DAmmando F, Tavani M, Donnarumma I, Pucella G, Raiteri CM, Villata M, Chen WP, Tosti G, Impiombato D, Romano P, Belfiore A, De Luca A, Novara G, Senziani F, Bazzano A, Fiocchi MT, Ubertini P, Ferrari A, Argan A, Barbiellini G, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Cocco V, Costa E, Del Monte E, De Paris G, Di Cocco G, Evangelista Y, Feroci M, Fiorini M, Fornari F, Froysland T, Fuschino F, Galli M, Gianotti F, Labanti C, Lapshov I, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mereghetti S, Morselli A, Pellizzoni A, Pacciani L, Perotti F, Picozza P, Prest M, Rapisarda M, Rappoldi A, Soffitta P, Trifoglio M, Trois A, Vallazza E, Zambra A, Zanello D, Pittori C, Verrecchia F, Santolamazza P, Preger B, Gasparrini D, Cutini S, Giommi P, Colafrancesco S, and Salotti L
Subjects: High Energy Gamma-ray Astronomy, Active Galactic Nuclei, AGILE satellite, Agile, Photon, Astrophysics::High Energy Astrophysical Phenomena, Inverse, FOS: Physical sciences, Astrophysics, Electron, blazar, law.invention, Telescope, law, Blazar, Electronic band structure, galaxies: active – galaxies: jets – quasars: general – quasars: individual (3C 454.3) – radiation mechanisms: non-thermal, Line (formation), Physics, Astrophysics (astro-ph), Compton scattering, multiwavelength observation, Astronomy and Astrophysics, galaxies: active, galaxies: jets, quasars: general, quasars: individual: 3C 454.3, radiation mechanisms: non-thermal, Space and Planetary Science
Abstract: [Abridged] We report on a multiwavelength observation of the blazar 3C 454.3 (which we dubbed "crazy diamond") carried out on November 2007 by means of the astrophysical satellites AGILE, INTEGRAL, Swift, the WEBT Consortium, and the optical-NIR telescope REM. 3C 454.3 is detected at a $\sim 19-\sigma$ level during the 3-week observing period, with an average flux above 100 MeV of $F_{\rm E>100MeV} = (170 \pm 13) \times 10^{-8}$ \phcmsec. The gamma-ray spectrum can be fit with a single power-law with photon index $\Gamma_{\rm GRID} = 1.73 \pm 0.16$ between 100 MeV and 1 GeV. We detect significant day-by-day variability of the gamma-ray emission during our observations, and we can exclude that the fluxes are constant at the 99.6% ($\sim 2.9 \sigma$) level. The source was detected typically around 40 degrees off-axis, and it was substantially off--axis in the field of view of the AGILE hard X-ray imager. However, a 5-day long ToO observation by INTEGRAL detected 3C 454.3 at an average flux of about $F_{\rm 20-200 keV} = 1.49 \times 10^{-3}$ \phcmsec with an average photon index of $\Gamma_{\rm IBIS} = 1.75 \pm 0.24$ between 20--200 keV. Swift also detected 3C 454.3 with a flux in the 0.3--10 keV energy band in the range $(1.23-1.40) \times 10^{-2}$ \phcmsec{} and a photon index in the range $\Gamma_{\rm XRT} = 1.56-1.73$. In the optical band, both WEBT and REM show an extremely variable behavior in the $R$ band. A correlation analysis based on the entire data set is consistent with no time-lags between the gamma-ray and the optical flux variations. Our simultaneous multifrequency observations strongly indicate that the dominant emission mechanism between 30 MeV and 30 GeV is dominated by inverse Compton scattering of relativistic electrons in the jet on the external photons from the broad line region., Comment: Accepted for publication in ApJ. Abridged Abstract. 37 pages, 14 Figures, 3 Tables
Published: 2008
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42. AGILE detection of GeV $\sf$γ-ray emission from the SNR W28

Author: A. Giuliani, M. Tavani, A. Bulgarelli, E. Striani, S. Sabatini, M. Cardillo, Y. Fukui, A. Kawamura, A. Ohama, N. Furukawa, K. Torii, H. Sano, F. A. Aharonian, F. Verrecchia, A. Argan, G. Barbiellini, P. A. Caraveo, P. W. Cattaneo, A. W. Chen, V. Cocco, E. Costa, F. D'Ammando, E. Del Monte, G. De Paris, G. Di Cocco, I. Donnarumma, Y. Evangelista, M. Feroci, M. Fiorini, T. Froysland, F. Fuschino, M. Galli, F. Gianotti, C. Labanti, Y. Lapshov, F. Lazzarotto, P. Lipari, F. Longo, M. Marisaldi, S. Mereghetti, A. Morselli, E. Moretti, L. Pacciani, A. Pellizzoni, F. Perotti, P. Picozza, M. Pilia, M. Prest, G. Pucella, M. Rapisarda, A. Rappoldi, P. Soffitta, M. Trifoglio, A. Trois, E. Vallazza, S. Vercellone, V. Vittorini, A. Zambra, D. Zanello, C. Pittori, P. Santolamazza, P. Giommi, S. Colafrancesco, L. Salotti, A., Giuliani, M., Tavani, A., Bulgarelli, E., Striani, S., Sabatini, M., Cardillo, Y., Fukui, A., Kawamura, A., Ohama, N., Furukawa, K., Torii, H., Sano, F. A., Aharonian, F., Verrecchia, A., Argan, G., Barbiellini, P. A., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, E., Costa, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, I., Donnarumma, Y., Evangelista, M., Feroci, M., Fiorini, T., Froysland, F., Fuschino, M., Galli, F., Gianotti, C., Labanti, Y., Lapshov, F., Lazzarotto, P., Lipari, Longo, Francesco, M., Marisaldi, S., Mereghetti, A., Morselli, E., Moretti, L., Pacciani, A., Pellizzoni, F., Perotti, P., Picozza, M., Pilia, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, P., Soffitta, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, C., Pittori, P., Santolamazza, P., Giommi, S., Colafrancesco, L., Salotti, Giuliani A, Tavani M, Bulgarelli A, Striani E, Sabatini S, Cardillo M, Fukui Y, Kawamura A, Ohama A, Furukawa N, Torii K, Sano H, Aharonian FA, Verrecchia F, Argan A, Barbiellini G, Caraveo PA, Cattaneo PW, Chen AW, Cocco V, Costa E, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Donnarumma I, Evangelista Y, Feroci M, Fiorini M, Froysland T, Fuschino F, Galli M, Gianotti F, Labanti C, Lapshov Y, Lazzarotto F, Lipari P, Longo F, Marisaldi M, Mereghetti S, Morselli A, Moretti E, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Soffitta P, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Santolamazza P, Giommi P, Colafrancesco S, and Salotti L
Subjects: Supernova Remnants, Supernova, Astrophysics::High Energy Astrophysical Phenomena, Hadron, acceleration of particles – diffusion – ISM: supernova remnants – gamma rays: ISM, FOS: Physical sciences, Flux, Cosmic ray, Astrophysics, AGILE, galactic cosmic rays, High Energy Gamma-ray Astronomy, Spectral line, law.invention, Telescope, law, Astrophysics::Galaxy Astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Molecular cloud, AGILE satellite, Gamma ray, Astronomy and Astrophysics, Space and Planetary Science, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Supernova remnants (SNRs) are believed to be the main sources of Galactic cosmic rays. Molecular clouds associated with SNRs can produce gamma-ray emission through the interaction of accelerated particles with the concentrated gas. The middle aged SNR W28, for its associated system of dense molecular clouds, provides an excellent opportunity to test this hypothesis. We present the AGILE/GRID observations of SNR W28, and compare them with observations at other wavelengths (TeV and 12CO J=1-->0 molecular line emission). The gamma-ray flux detected by AGILE from the dominant source associated with W28 is (14 +- 5) 10^-8 ph cm^-2 s^-1 for E > 400 MeV. This source is positionally well correlated with the TeV emission observed by the HESS telescope. The local variations of the GeV to TeV flux ratio suggest a difference between the CR spectra of the north-west and south molecular cloud complexes. A model based on a hadronic-induced interaction and diffusion with two molecular clouds at different distances from the W28 shell can explain both the morphological and spectral features observed by AGILE in the MeV-GeV energy range and by the HESS telescope in the TeV energy range. The combined set of AGILE and H.E.S.S. data strongly support a hadronic model for the gamma-ray production in W28., Accepted for publication in Astronomy & Astrophysics Letters
Published: 2010
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43. Gamma-ray localization of terrestrial gamma-ray flashes

Author: M. Rapisarda, E. Del Monte, A. Argan, G. Pucella, I. Donnarumma, M. Pilia, Andrea Bulgarelli, Y. Evangelista, A. Rubini, Enrico Costa, S. Vercellone, P. Soffitta, A. Zambra, F. D'Ammando, Fulvio Gianotti, M. Feroci, Marco Tavani, M. Fiorini, F. Longo, Sandro Mereghetti, Claudio Labanti, E. Moretti, G. De Paris, A. W. Chen, A. Morselli, P. Giommi, S. Colafrancesco, Martino Marisaldi, D. Zanello, G. Di Persio, L. Pacciani, V. Vittorini, E. Vallazza, P. Santolamazza, F. Fuschino, G. Piano, P. A. Caraveo, Arnaud Ferrari, P. Lipari, G. Di Cocco, P. W. Cattaneo, S. Cutini, E. Striani, M. Prest, S. Sabatini, I. Lapshov, G. Barbiellini, A. Pellizzoni, A. Giuliani, A. Trois, Fabrizio Lucarelli, P. Picozza, M. Galli, F. Verrecchia, L. Salotti, M. Trifoglio, F. Perotti, F. Lazzarotto, C. Pittori, T. Froysland, L. A. Antonelli, A. Rappoldi, Marisaldi M, Argan A, Trois A, Giuliani A, Tavani M, Labanti C, Fuschino F, Bulgarelli A, Longo F, Barbiellini G, Del Monte E, Moretti E, Trifoglio M, Costa E, Caraveo P, Cattaneo PW, Chen A, DAmmando F, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Froysland T, Galli M, Gianotti F, Lapshov I, Lazzarotto F, Lipari P, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Piano G, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Striani E, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Giommi P, Lucarelli F, Pittori C, Santolamazza P, Verrecchia F, and Salotti L
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), Physics, Agile, Photon, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Attenuation, Gamma ray, FOS: Physical sciences, General Physics and Astronomy, minicalorimeter, terrestrial gamma-ray flashes, Astrophysics, Electromagnetic radiation, Particle detector, Semiconductor detector, Physics - Atmospheric and Oceanic Physics, Atmosphere of Earth, Optics, Terrestrial Gamma-Ray Flashes, Atmospheric and Oceanic Physics (physics.ao-ph), Satellite, business, Astrophysics - Earth and Planetary Astrophysics
Abstract: Terrestrial Gamma-Ray Flashes (TGFs) are very short bursts of high energy photons and electrons originating in Earth's atmosphere. We present here a localization study of TGFs carried out at gamma-ray energies above 20 MeV based on an innovative event selection method. We use the AGILE satellite Silicon Tracker data that for the first time have been correlated with TGFs detected by the AGILE Mini-Calorimeter. We detect 8 TGFs with gamma-ray photons of energies above 20 MeV localized by the AGILE gamma-ray imager with an accuracy of 5-10 degrees at 50 MeV. Remarkably, all TGF-associated gamma rays are compatible with a terrestrial production site closer to the sub-satellite point than 400 km. Considering that our gamma rays reach the AGILE satellite at 540 km altitude with limited scattering or attenuation, our measurements provide the first precise direct localization of TGFs from space., Comment: 5 pages, 4 figures, 1 table, available at http://prl.aps.org/abstract/PRL/v105/i12/e128501

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