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93 results on '"TRUMPER J."'

1. Modern compact star observations and the quark matter equation of state

Author

Klahn, T., Blaschke, D., Sandin, F., Fuchs, C., Faessler, A., Grigorian, H., Ropke, G., and Trumper, J.

Subjects
Nuclear Theory
Abstract

We present a hybrid equation of state (EoS) for dense matter that satisfies phenomenological constraints from modern compact star (CS) observations which indicate high maximum masses (M = 2 M_sun) and large radii (R> 12 km). The corresponding isospin symmetric EoS is consistent with flow data analyses of heavy-ion collisions and a deconfinement transition at approx. 0.55 fm^{-3}. The quark matter phase is described by a 3-flavor Nambu--Jona-Lasinio model that accounts for scalar diquark condensation and vector meson interactions while the nuclear matter phase is obtained within the Dirac-Brueckner-Hartree-Fock (DBHF) approach using the Bonn-A potential. We demonstrate that both pure neutron stars and neutron stars with quark matter cores (QCSs) are consistent with modern CS observations. Hybrid star configurations with a CFL quark core are unstable., Comment: 16 pages, 4 figures; published version, important note added in proof

Published
2006
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2. Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions

Author

Klahn, T., Blaschke, D., Typel, S., van Dalen, E. N. E., Faessler, A., Fuchs, C., Gaitanos, T., Grigorian, H., Ho, A., Kolomeitsev, E. E., Miller, M. C., Ropke, G., Trumper, J., Voskresensky, D. N., Weber, F., and Wolter, H. H.

Subjects
Nuclear Theory, Astrophysics, High Energy Physics - Phenomenology
Abstract

A new scheme for testing nuclear matter equations of state (EsoS) at high densities using constraints from neutron star phenomenology and a flow data analysis of heavy-ion collisions is suggested. An acceptable EoS shall not allow the direct Urca process to occur in neutron stars with masses below $1.5~M_{\odot}$, and also shall not contradict flow and kaon production data of heavy-ion collisions. Compact star constraints include the mass measurements of 2.1 +/- 0.2 M_sun (1 sigma level) for PSR J0751+1807, of 2.0 +/- 0.1 M_sun from the innermost stable circular orbit for 4U 1636-536, the baryon mass - gravitational mass relationships from Pulsar B in J0737-3039 and the mass-radius relationships from quasiperiodic brightness oscillations in 4U 0614+09 and from the thermal emission of RX J1856-3754. This scheme is applied to a set of relativistic EsoS constrained otherwise from nuclear matter saturation properties with the result that no EoS can satisfy all constraints simultaneously, but those with density-dependent masses and coupling constants appear most promising., Comment: 15 pages, 8 figures, 5 tables

Published
2006
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3. An XMM-Newton observation of Ton S180: Constraints on the continuum emission in ultrasoft Seyfert galaxies

Author

Vaughan, S., Boller, Th., Fabian, A. C., Ballantyne, D. R., Brandt, W. N., and Trumper, J.

Subjects
Astrophysics
Abstract

We present an XMM-Newton observation of the bright, narrow-line, ultrasoft Seyfert 1 galaxy Ton S180. The 0.3-10 keV X-ray spectrum is steep and curved, showing a steep slope above 2.5 keV (Gamma ~ 2.3) and a smooth, featureless excess of emission at lower energies. The spectrum can be adequately parameterised using a simple double power-law model. The source is strongly variable over the course of the observation but shows only weak spectral variability, with the fractional variability amplitude remaining approximately constant over more than a decade in energy. The curved continuum shape and weak spectral variability are discussed in terms of various physical models for the soft X-ray excess emission, including reflection off the surface of an ionised accretion disc, inverse-Compton scattering of soft disc photons by thermal electrons, and Comptonisation by electrons with a hybrid thermal/non-thermal distribution. We emphasise the possibility that the strong soft excess may be produced by dissipation of accretion energy in the hot, upper atmosphere of the putative accretion disc., Comment: 9 pages, accepted for publication in MNRAS

Published
2002
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4. 1E 1207.4-5209: The puzzling pulsar at the center of the PKS 1209-51/52 supernova remnant

Author

Pavlov, G. G., Zavlin, V. E., Sanwal, D., and Trumper, J.

Subjects
Astrophysics
Abstract

Second Chandra observation of 1E 1207.4-5209, the central source of the supernova remnant PKS 1209-51/52, allowed us to confirm the previously detected period of 424 ms and, assuming a uniform spin-down, estimate the period derivative, Pdot (0.7-3)e-14 s/s. The corresponding characteristic age of the pulsar, P/2Pdot~200-900 kyr, is much larger than the estimated age of the SNR, \~7 kyr. The values of the spin-down luminosity, Edot (0.4-1.6)e34 erg/s, and conventional magnetic field, B (2-4)e12 G, are typical for a middle-aged radio pulsar, although no manifestations of pulsar activity have been observed. If 1E 1207.4-5209 is indeed the neutron star formed in the same supernova explosion that created PKS 1209-51/52, such a discrepancy in ages could be explained either by a long initial period, close to its current value, or, less likely, by a very large braking index of the pulsar. Alternatively, the pulsar could be a foreground object unrelated to the supernova remnant, but the probability of such a coincidence is very low., Comment: 4 pages, 3 figures, to appear in ApJ Letters, v. 569 (April 2002)

Published
2002
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5. The ROSAT deep survey: V. X-rays Sources and Optical Identifications in the Marano Field

Author

Zamorani, G., Mignoli, M., Hasinger, G., Burg, R., Giacconi, R., Schmidt, M., Trumper, J., Ciliegi, P., Gruppioni, C., and Marano, B.

Subjects
Astrophysics
Abstract

We present the X-ray data and the optical identifications for a deep ROSAT PSPC observation in the "Marano field". In the inner region of the ROSAT field (15' radius) we detected 50 X-ray sources with Sx >= 3.7x10^(-15) erg/cm^2/s. When corrected for the different sensitivity over the field, the estimated observed surface density at Sx >= 4x10^(-15) erg/cm^2/s is 272+/-40 sources/sq.deg. Four X-ray sources, corresponding to 8% of the total sample, have been detected in radio images with a flux limit of about 0.2 mJy. Careful statistical analysis of multicolour CCD data in the error boxes of the 50 X-ray sources has led to the identification of 42 sources, corresponding to 84% of the X-ray sample. These 42 reliable identifications are 33 AGNs (including two radio galaxies and one BL Lac candidate; 79% of the identified sources), 2 galaxies, 3 groups or clusters of galaxies and 4 stars. We also show that it is likely that a few of the 8 unidentified sources are such because the derived X-ray positions may be offset with respect to the real ones due to confusion effects. The unidentified sources have a large ratio of X-ray to optical fluxes and most of them have harder than average X-ray spectra. Since most of the identified objects with these characteristics in our field and in the Lockman field are AGNs, we conclude that also most of these sources are likely to be AGNs. Finally, comparing the optically and X-ray selected samples of AGNs in this field, we estimate the ``efficiency'' of AGN selection with deep X-ray exposures and with purely optical criteria., Comment: 24 pages, 13 figures (7 in JPEG format), A&A Latex using psfig and epsf, accepted for publication in Astronomy and Astrophysics Suppl

Published
1999

7. A 36 cm2 monolithic pn-CCD for x-ray detection on the XMM and ABRIXAS satellites

Author

Holl, P., Bihler, E., Brauninger, H., Briel, U., Hartmann, R., Hartner, G., Hauff, D., Kemmer, J., Kendziorra, E., Krause, N., Lechner, P., Maier, B., Meidinger, N., Pfeffermann, E., Pfluger, B., Popp, M., Reppin, C., Richter, R.H., Soltau, H., Stotter, D., Struder, L., Trumper, J., and Zanthier, C.v.

Subjects
Charge coupled devices -- Design and construction, X-ray astronomy -- Equipment and supplies, Business, Electronics, Electronics and electrical industries
Abstract

X-ray sensitive CCDs with outstanding properties have been developed and produced at the MPI Halbleiterlabor. They contribute to the focal plane instrumentation of two space missions: the European XMM and the German ABR, IXAS satellites. These CCDs, presented here, use exclusively ph-junctions on ultra-pure, high-ohmic silicon for all active components, in particular for the transfer electrodes and the on-chip readout circuitry. Full depletion of the detector chip, a homogeneous and thin entrance window and large pixel sizes can be realized by this technological concept. This concept results in low noise performance, spectroscopic energy resolution, high detection efficiency, radiation hardness and fast readout. With these properties the so-called pn-CCDs ideally match the requirements of the satellites, which are given by the specifics of their X-ray imaging optics as well as the intensity, energy range and dynamic behavior of the objects to be observed.

Published
1998

8. A Fully Depleted pn-Junction CCD for Infrared-, UV- and X- ray detection

Author

von Zanthier, C., Brauninger, H., Dennerl, K., Hartmann, R., Hartner, G., Hippmann, H., Kaltenberger, A., Kastelic, E., Kink, W., Krause, N., Meidinger, N., Metzner, G., Pfeffermann, E., Popp, M., Reppin, C., Riedl, J., Stotter, D., Struder, L., Trumper, J., Weber, W., Carathanassis, D., Engelhard, S., Gebhart, Th., Hauff, D., Lutz, G., Richter, R. H., Seitz, H., Solc, P., Biehler, E., Bottcher, H., Kendziorra, E., Kramer, J., Pfluger, B., Staubert, R., Holl, P., Kemmer, J., Lechner, P., Maier, B., Soltau, H., Stotter, R., and Bihler, E.

Subjects
Radiography -- Observations, Charge coupled devices -- Usage, Science and technology
Abstract

Byline: C. von Zanthier (1), H. Brauninger (2), K. Dennerl (2), R. Hartmann (2), G. Hartner (2), H. Hippmann (2), A. Kaltenberger (2), E. Kastelic (2), W. Kink (2), N. Krause (2), N. Meidinger (2), G. Metzner (2), E. Pfeffermann (2), M. Popp (2), C. Reppin (2), J. Riedl (2), D. Stotter (2), L. Struder (2), J. Trumper (2), W. Weber (2), D. Carathanassis (3), S. Engelhard (3), Th. Gebhart (3), D. Hauff (3), G. Lutz (3), R. H. Richter (3), H. Seitz (3), P. Solc (3), E. Biehler (4), H. Bottcher (3,4), E. Kendziorra (4,5), J. Kramer (4,5), B. Pfluger (4,5), R. Staubert (4,5), P. Holl (5), J. Kemmer (3), P. Lechner (5), B. Maier (5), H. Soltau (5), R. Stotter (5), E. Bihler (5) Abstract: This paper describes the performance of the Fully Depleted pn-junction CCD (pn-CCD) system, developed for ESA's XMM-satellite mission for soft x-ray imaging and spectroscopy in the single photon counting mode in the 100 eV to 10 keV photon range. The 58 mm x 60 mm large pn-CCD array, designed and fabricated at the Semiconductor Lab (Halbleiterlabor) of the Max-Planck-Institut, uses pn-junctions for registers and as backside structure. This concept naturally enables full depletion of the detector volume independent of the silicon wafer's resistivity and thickness, and as such make it an efficient detector for the x-ray region and the infrared. For high detection efficiency in the soft x-ray region and UV, an ultrathin pn-CCD backside deadlayer has been realized. Each pn-CCD-channel is equipped with its own on-chip JFET amplifier which, in combination with the CAMEX-amplifier and multiplexing chip, facilitates parallel readout and fast data rate: the cooled pn-CCD system can be read out at a data rate up to 3 MHz with an electronic noise floor of ENC &lt 5 e-. Author Affiliation: (1) KETEK GmbH, Am Isarbach 30, D - 85764, Oberschlei[beta]heim, Germany (2) Max-Planck -, Institut fur extraterrestische Physik, Gie[beta]enbachstr., D-85740, Garching, Germany (3) Max-Planck -Institut fur Physik, Fohringer Ring 6, D - 80805, Munchen, Germany (4) Institut fur Astronomie und, Astrophysik der Universitat Tubingen, Waldhauser Str. 64, D - 72076, Tubingen, Germany (5) Institut fur Astronomie und, Astrophysik der Universitat Tubingen, Waldhauser Stra[beta] 64, D - 72076, Tubingen, Germany Article History: Registration Date: 05/10/2004

Published
1998

9. Discovery of X-ray and extreme ultraviolet emission from Comet C/Hyakutake 1996 B2

Author

Lisse, C.M., Dennerl, K., Englhauser, J., Harden, M., Marshall, F.E., Mumma, M.J., Petre, R., Pye, J.P., Ricketts, M.J., Schmitt, J., Trumper, J., and West, R.G.

Subjects
X-ray astronomy -- Observations -- Spectra, Hyakutake (Comet) -- Observations -- Spectra, Comets -- Spectra, Ultraviolet astronomy -- Observations -- Spectra, Science and technology, Observations, Spectra
Abstract

During its close approach to Earth, comet C/Hyakutake 1996 B2 was observed at extreme ultraviolet and x-ray wavelengths with the Rontgen X-ray Satellite and Rossi X-ray Timing Explorer. The emission morphology was symmetric with respect to a vector from the comet's nucleus toward the sun, but not symmetric around the direction of motion of the comet with respect to interplanetary dust. A slowly varying emission and a large impulsive event that varied on time scales of 1 to 2 hours were observed. An interaction between the comet and the solar wind/solar magnetic field seems to be the most likely mechanism for the observed emission., The close perigee [minimum geocentric distance δ = 0.102 AU (astronomical unit)] of the long-period comet C/Hyakutake 1996 B2 at universal time (UT) 25.3 March 1996 presented a unique opportunity [...]

Published
1996

10. The structure of the Virgo cluster of galaxies from Rosat x-ray images

Author

Bohringer, H., Briel, U.G., Schwarz, R.A., Voges, W., Hartner, G., and Trumper, J.

Subjects
Galaxies -- Clusters, Virgo Cluster -- Research, Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

X-ray observations of Virgo cluster reveal that, while most of the cluster mass is centered on the M87 galaxy, smaller masses are present around M86 and M49. The data reinforces the hypothesis that M86 may belong to a small group of galaxies in the process of merging with the main cluster. Hot luminous gas appear to cover the optically visible regions.

Published
1994

11. X-ray survey of the Large Magellanic Cloud by ROSAT

Author

Trumper, J., Hasinger, G., Aschenbach, B., Brauninger, H., Briel, U.G., Burkert, W., Fink, H., Pfeffermann, E., Pietsch, W., Predehl, P., Schmitt, J.H.M.M., Voges, W., Zimmermann, U., and Beuermann, K.

Subjects
Rosat (Artificial satellite) -- Observations, X-rays -- Spectra, X-ray astronomy -- Research, X-ray telescope -- Observations, Magellanic Clouds -- Observations, Supernova remnants -- Research, Environmental issues, Science and technology, Zoology and wildlife conservation
Published
1991

12. A soft X-ray image of the moon

Author

Schmitt, J.H.M.M., Snowden, S.L., Aschenbach, B., Hasinger, G., Pfeffermann, E., Predehl, P., and Trumper, J.

Subjects
Rosat (Artificial satellite) -- Observations, X-ray astronomy -- Research, Moon -- Observations, Solar wind -- Research, Solar radiation -- Research, Environmental issues, Science and technology, Zoology and wildlife conservation
Published
1991

14. Detection of soft X-rays from supernova 1993J six days after outburst

Author

Zimmermann, H.-U., Lewin, W., Predehl, P., Aschenbach, B., Fabbiano, G., Hasinger, G., Lubin, L., Magnier, E., Paradijs, J. van, Petre, R., Pietsch, W., and Trumper, J.

Subjects
Supernovae -- Spectra, Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

The supernova SN1993J, observed on Mar 28, 1993, emitted X-rays six days after the explosion, and the intrinsic absorption of these emissions and the decay of X-ray luminosity with time were studied. A low intrinsic absorption of X-ray emissions which could be attributed to the radiation intensity during the initial explosion were observed. The decay of the X-ray luminosity with time provided information about the outer layers of the supernova and the circumstellar gas.

Published
1994

16. X-ray detection of Nova Herculis 1991 five days after optical outburst

Author

Lloyd, H.M., O'Brien, T.J., Bode, M.F., Predehl, P., Schmitt, J.H.M.M., Trumper, J., Watson, M.G., and Pounds, K.A.

Subjects
Stars, New -- Observations, X-ray astronomy -- Research, Environmental issues, Science and technology, Zoology and wildlife conservation
Published
1992

17. 'Exigua pars est vitae qua vivimus. Ceterum quidem omne spatium non vita sed tempus est' : divagazioni semantiche (e lessicali) su spatium e sui suoi esiti romanzi

Author

Blumenthal, P, Espinosa Elorza Rosa María, Marello, C, Schapira, C, Becker, M, Bekaert, E, Biermann Fischer, M, Ciama, A, Citraro, C, Crăiniceanu, I, De Cuyper, G, Dragotto, F, Enghels, R, Jansegers, M, Sánchez, Jjg, Gebăilă, A, Gerhard Krait, F, González Manzano, M, Gross, G, Grutschus, A, Fesenmeier, L, Hidalgo Alfageme, Ca, Iliescu, M, Costăchescu, A, Dragoste, R, Khachaturyan, E, Kleiber, G, Lammert, M, Lehmann, S, Loiseau, S, Manole, V, Mattera, M, Mocciaro, E, Gallo, Cm, Piot, M, Piqueras Brunet, M, Rull, X, Plötner, K, Sánchez Jiménez, Su, Sentí i. Pons, A, Soto Andión, X, Soto Nieto, A, Stoichiţoiu Ichim, A, Tanghe, S, Bassett Trumper, J, and Vassiliadou, H

Subjects
tempus, semantica storica, spatium, Settore L-LIN/01 - Glottologia e Linguistica, spatium, tempus, semantica storica
Published
2013

18. The Alpha Magnetic Spectrometer (AMS)

Author

Alcaraz, J., Alpat, B., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Luca Baldini, Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J. D., Burger, W. J., Cai, X. D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y. H., Chen, H. F., Chen, H. S., Chen, Z. G., Chernoplekov, N. A., Chiueh, T. H., Chuang, Y. L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., Da Cunha, J. P., Dai, T. S., Deus, J. D., Dinu, N., Djambazov, L., Antone, I. D., Dong, Z. R., Emonet, P., Engelberg, J., Eppling, F. J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P. H., Fluegge, G., Fouque, N., Yu. Galaktionov, Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W. Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M. A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Giovanni Lamanna, Laurenti, G., Lebedev, A., Lee, S. C., Levi, G., Levtchenko, P., Liu, C. L., Liu, H. T., Lopes, I., Lu, G., Lu, Y. S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., Mcneil, R. R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I. H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P. G., Rapin, D., Raupach, F., Ren, D., Zhuoxiang Ren, Ribordy, M., Richeux, J. P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz Dratzig, A., Schwering, G., Scolieri, G., Seo, E. S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G. S., Suter, H., Tang, X. W., Ting, S. C. C., Ting, S. M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J. P., Viertel, G., Vite, D., Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B. C., Wang, J. Z., Wang, Y. H., Wiik, K., Williams, C., Wu, S. X., Xia, P. C., Yan, J. L., Yan, L. G., Yang, C. G., Yang, M., Ye, S. W., Yeh, P., Xu, Z. Z., Zhang, H. Y., Zhang, Z. P., Zhao, D. X., Zhu, G. Y., Zhu, W. Z., Zhuang, H. L., Zichichi, A., Zimmermann, B., Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), 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), AMS, Alcaraz, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Bene, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Crespo, P, Cristinziani, M, da Cunha, J, Dai, T, Deus, J, Dinu, N, Djambazov, L, Dantone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimm, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, W, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, I, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Roeser, U, Roissin, C, Sagdeev, R, Sartorelli, G, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Usoskin, I, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, and Zimmermann, B

Subjects
Physics, Nuclear and High Energy Physics, Spectrometer, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Dark matter, Cosmic ray, 01 natural sciences, Particle detector, Nuclear physics, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Popular Physics, FIS/05 - ASTRONOMIA E ASTROFISICA, FIS/01 - FISICA SPERIMENTALE, Antimatter, 0103 physical sciences, International Space Station, Alpha Magnetic Spectrometer, Measuring instrument, space-research instrumentation, 010306 general physics, Instrumentation, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract

The Alpha Magnetic Spectrometer (AMS) is a large acceptance (0.65 sr m(2)) detector designed to operate in the International Space Station (ISS) for three years. The purposes of the experiment are to search for cosmic antimatter and dark matter and to study the composition and energy spectrum of the primary cosmic rays. A "scated-down" version has been flown on the Space Shuttle Discovery for 10 days in June 1998. The complete AMS is programmed for installation on the ISS in October 2003 for an operational period of 3 yr. This contribution reports on the experimental configuration that will be installed on the ISS. (C) 2002 Elsevier Science B.V. All rights reserved.

Published
2001

20. Relative composition and energy spectra of light nuclei in cosmic rays: Results from AMS-01

Author

Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Arruda, A, Azzarello, P, Basile, M, Barao, F, Barreira, G, Bartoloni, A, Battiston, R, Becker, R, Becker, U, Bellagamba, L:, B, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bindi, V, Boella, G, Boschini, M, Bourquin, M, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cernuda, I, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Choi, Y, Cindolo, F, Commichau, V, Contin, A, Cortina Gil, E, Crespo, D, Cristinziani, M, Dai, T, dela Guia, C, Delgado, C, Di Falco, S, Djambazov, L, D’Antone, I, Dong, Z, Duranti, M, Engelberg, J, Eppling, F, Eronen, T, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Flugge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giovacchini, F, Giusti, P, Grandi, D, Grimm, O, Gu, W, Haino, S, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Hungerford, W, Ionica, M, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kim, D, Kim, G, Kim, K, Kirn, T, Klimentov, A, Kossakowski, R, Kounine, A, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lechanoine Leluc, C, Lee, M, Lee, S, Levi, G, Lin, C, Liu, H, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Menichelli, M, Mihul, A, Mujunen, A, Oliva, A, Palmonari, F, Park, H, Park, W, Pauluzzi, M, Pauss, F, Pereira, R, Perrin, E, Pevsner, A, Pilo, F, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Produit, N, Quadrani, L, Rancoita, P, Rapin, D, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, Schultz von Dratzig, A, Schwering, G, Seo, E, Shin, J, Shoumilov, E, Shoutko, V, Siedenburg, T, Siedling, R, Son, D, Song, T, Spada, F, Spinella, F, Steuer, M, Sun, G, Suter, H, Tang, H, Ting, S, Tomassetti, N, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Vierte, G, Vite, D, Von Gunten, H, Waldmeier Wicki, S, Wallraff, W, Wang, J, Wiik, K, Williams, C, Wu, S, Xia, P, Xu, S, Xu, Z, Yan, J, Yan, L, Yang, C, Yang, J, Yang, M, Ye, S, Zhang, H, Zhang, Z, Zhao, D, Zhou, F, Zhou, Y, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, L: Bene, BOELLA, GIULIANO FILIPPO, Burger, JD, Burger, WJ, Cai, XD, Chang, YH, Chen, HF, Chen, HS, Chen, ZG, Chernoplekov, NA, Chiueh, TH, Choi, YY, Dai, TS, Dong, ZR, Eppling, FJ, Fisher, PH, GERVASI, MASSIMO, Gu, WQ, Kim, DH, Kim, GN, Kim, KS, Lee, MW, Lee, SC, Lin, CH, Liu, HT, Lu, YS, McNeil, RR, Park, HB, Park, WH, Rancoita, PG, Richeux, JP, Seo, ES, Shin, JH, Spada, FR, Sun, GS, Tang, HW, Ting, SCC, Ting, SM, Vialle, JP, Wang, JZ, Xia, PC, Xu, ZZ, Yan, JL, Yan, LG, Yang, CG, Ye, SW, Zhang, HY, Zhang, ZP, Zhao, DX, Zhu, GY, Zhu, WZ, Zhuang, HL, Zuccon, P., Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Arruda, A, Azzarello, P, Basile, M, Barao, F, Barreira, G, Bartoloni, A, Battiston, R, Becker, R, Becker, U, Bellagamba, L:, B, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bindi, V, Boella, G, Boschini, M, Bourquin, M, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cernuda, I, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Choi, Y, Cindolo, F, Commichau, V, Contin, A, Cortina Gil, E, Crespo, D, Cristinziani, M, Dai, T, dela Guia, C, Delgado, C, Di Falco, S, Djambazov, L, D’Antone, I, Dong, Z, Duranti, M, Engelberg, J, Eppling, F, Eronen, T, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Flugge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giovacchini, F, Giusti, P, Grandi, D, Grimm, O, Gu, W, Haino, S, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Hungerford, W, Ionica, M, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kim, D, Kim, G, Kim, K, Kirn, T, Klimentov, A, Kossakowski, R, Kounine, A, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lechanoine Leluc, C, Lee, M, Lee, S, Levi, G, Lin, C, Liu, H, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Menichelli, M, Mihul, A, Mujunen, A, Oliva, A, Palmonari, F, Park, H, Park, W, Pauluzzi, M, Pauss, F, Pereira, R, Perrin, E, Pevsner, A, Pilo, F, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Produit, N, Quadrani, L, Rancoita, P, Rapin, D, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, Schultz von Dratzig, A, Schwering, G, Seo, E, Shin, J, Shoumilov, E, Shoutko, V, Siedenburg, T, Siedling, R, Son, D, Song, T, Spada, F, Spinella, F, Steuer, M, Sun, G, Suter, H, Tang, H, Ting, S, Tomassetti, N, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Vierte, G, Vite, D, Von Gunten, H, Waldmeier Wicki, S, Wallraff, W, Wang, J, Wiik, K, Williams, C, Wu, S, Xia, P, Xu, S, Xu, Z, Yan, J, Yan, L, Yang, C, Yang, J, Yang, M, Ye, S, Zhang, H, Zhang, Z, Zhao, D, Zhou, F, Zhou, Y, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, L: Bene, BOELLA, GIULIANO FILIPPO, Burger, JD, Burger, WJ, Cai, XD, Chang, YH, Chen, HF, Chen, HS, Chen, ZG, Chernoplekov, NA, Chiueh, TH, Choi, YY, Dai, TS, Dong, ZR, Eppling, FJ, Fisher, PH, GERVASI, MASSIMO, Gu, WQ, Kim, DH, Kim, GN, Kim, KS, Lee, MW, Lee, SC, Lin, CH, Liu, HT, Lu, YS, McNeil, RR, Park, HB, Park, WH, Rancoita, PG, Richeux, JP, Seo, ES, Shin, JH, Spada, FR, Sun, GS, Tang, HW, Ting, SCC, Ting, SM, Vialle, JP, Wang, JZ, Xia, PC, Xu, ZZ, Yan, JL, Yan, LG, Yang, CG, Ye, SW, Zhang, HY, Zhang, ZP, Zhao, DX, Zhu, GY, Zhu, WZ, Zhuang, HL, and Zuccon, P.

Abstract

Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. In this paper, the relative abundances of light-nuclei lithium, beryllium, boron, and carbon are presented. The secondary-to-primary ratios Li/C, Be/C, and B/C have been measured in the kinetic energy range 0.35-45 GeV nucleon-1. The isotopic ratio 7Li/6Li is also determined in the magnetic rigidity interval 2.5-6.3 GV. The secondary-to-secondary ratios Li/Be, Li/B, and Be/B are also reported. These measurements are based on the data collected by the Alpha Magnetic Spectrometer AMS-01 during the STS-91 space shuttle flight in 1998 June. Our experimental results are in substantial agreement with other measurements, where they exist. We describe our light-nuclei data with a diffusive-reacceleration model. A 10%-15% overproduction of Be is found in the model predictions and can be attributed to uncertainties in the production cross-section data. © 2010. The American Astronomical Society.

Published
2010

21. Modern compact star observations and the quark matter equation of state

Author

Klähn, T., Blaschke, D., Sandin, Fredrik, Fuchs, C., Faessler, A., Grigorian, H., Röpke, G., Trumper, J., Klähn, T., Blaschke, D., Sandin, Fredrik, Fuchs, C., Faessler, A., Grigorian, H., Röpke, G., and Trumper, J.

Abstract

We present a hybrid equation of state (EoS) for dense matter that satisfies phenomenological constraints from modern compact star (CS) observations which indicate high maximum masses (M = 2 Msun) and large radii (R> 12 km). The corresponding isospin symmetric EoS is consistent with flow data analyses of heavy-ion collisions and a deconfinement transition at approx. 0.55 fm-3. The quark matter phase is described by a 3-flavor Nambu--Jona-Lasinio model that accounts for scalar diquark condensation and vector meson interactions while the nuclear matter phase is obtained within the Dirac-Brueckner-Hartree-Fock (DBHF) approach using the Bonn-A potential. We demonstrate that both pure neutron stars and neutron stars with quark matter cores (QCSs) are consistent with modern CS observations. Hybrid star configurations with a CFL quark core are unstable., Validerad; 2007; 20070305 (ysko)

Published
2007
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22. The Alpha Magnetic Spectrometer (AMS)

Author

Alcaraz, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Bene, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Crespo, P, Cristinziani, M, da Cunha, J, Dai, T, Deus, J, Dinu, N, Djambazov, L, Dantone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimm, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, W, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, I, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Roeser, U, Roissin, C, Sagdeev, R, Sartorelli, G, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Usoskin, I, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, BOELLA, GIULIANO FILIPPO, DAntone, I, GERVASI, MASSIMO, McNeil, R, Zimmermann, B., Alcaraz, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Barancourt, D, Barao, F, Barbier, G, Barreira, G, Battiston, R, Becker, R, Becker, U, Bellagamba, L, Bene, P, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Crespo, P, Cristinziani, M, da Cunha, J, Dai, T, Deus, J, Dinu, N, Djambazov, L, Dantone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimm, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, W, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Laurenti, G, Lebedev, A, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, I, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Roeser, U, Roissin, C, Sagdeev, R, Sartorelli, G, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Usoskin, I, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, Vialle, J, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, BOELLA, GIULIANO FILIPPO, DAntone, I, GERVASI, MASSIMO, McNeil, R, and Zimmermann, B.

Abstract

The Alpha Magnetic Spectrometer (AMS) is a large acceptance (0.65 sr m(2)) detector designed to operate in the International Space Station (ISS) for three years. The purposes of the experiment are to search for cosmic antimatter and dark matter and to study the composition and energy spectrum of the primary cosmic rays. A "scated-down" version has been flown on the Space Shuttle Discovery for 10 days in June 1998. The complete AMS is programmed for installation on the ISS in October 2003 for an operational period of 3 yr. This contribution reports on the experimental configuration that will be installed on the ISS. (C) 2002 Elsevier Science B.V. All rights reserved.

Published
2002

23. The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I – results from the test flight on the space shuttle

Author

Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Cho, K, Choi, M, Choi, Y, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Cortina-Gil, E, Cristinziani, M, da Cunha, J, Dai, T, Delgado, C, Deus, J, Dinu, N, Djambazov, L, D'Antone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimms, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, D, Kim, G, Kim, K, Kim, M, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Lanciotti, E, Laurenti, G, Lebedev, A, Lechanoine-Leluc, C, Lee, M, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, H, Park, W, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Rossin, C, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shin, J, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, V, Jp, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, J, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, Burger, JD, Burger, WJ, Cai, XD, Chang, YH, Chen, HF, Chen, HS, Chen, ZG, Chernoplekov, NA, Chiueh, TH, Choi, MJ, Choi, YY, Chuang, YL, da Cunha, JP, Dai, TS, Deus, JD, Dong, ZR, Eppling, FJ, Fisher, PH, Gu, WQ, Huang, MA, Kim, DH, Kim, GN, Kim, KS, Kim, MY, Lee, MW, Lee, SC, Liu, CL, Liu, HT, Lu, YS, McNeil, RR, Park, HB, Park, WH, Rancoita, PG, Richeux, JP, von Dratzig, AS, Seo, ES, Shin, JW, Sun, GS, Tang, XW, Ting, SCC, Ting, SM, F Vialle, JP, Wicki, SW, Wang, BC, Wang, JZ, Wang, YH, Wu, SX, Xia, PC, Yan, JL, Yan, LG, Yang, CG, Ye, SW, Xu, ZZ, Zhang, HY, Zhang, ZP, Zhao, DX, Zhu, GY, Zhu, WZ, Zhuang, HL, Aguilar, M, Alcaraz, J, Allaby, J, Alpat, B, Ambrosi, G, Anderhub, H, Ao, L, Arefiev, A, Azzarello, P, Babucci, E, Baldini, L, Basile, M, Berdugo, J, Berges, P, Bertucci, B, Biland, A, Bizzaglia, S, Blasko, S, Boella, G, Boschini, M, Bourquin, M, Brocco, L, Bruni, G, Buenerd, M, Burger, J, Burger, W, Cai, X, Camps, C, Cannarsa, P, Capell, M, Casadei, D, Casaus, J, Castellini, G, Cecchi, C, Chang, Y, Chen, H, Chen, Z, Chernoplekov, N, Chiueh, T, Cho, K, Choi, M, Choi, Y, Chuang, Y, Cindolo, F, Commichau, V, Contin, A, Cortina-Gil, E, Cristinziani, M, da Cunha, J, Dai, T, Delgado, C, Deus, J, Dinu, N, Djambazov, L, D'Antone, I, Dong, Z, Emonet, P, Engelberg, J, Eppling, F, Eronen, T, Esposito, G, Extermann, P, Favier, J, Fiandrini, E, Fisher, P, Fluegge, G, Fouque, N, Galaktionov, Y, Gervasi, M, Giusti, P, Grandi, D, Grimms, O, Gu, W, Hangarter, K, Hasan, A, Hermel, V, Hofer, H, Huang, M, Hungerford, W, Ionica, M, Ionica, R, Jongmanns, M, Karlamaa, K, Karpinski, W, Kenney, G, Kenny, J, Kim, D, Kim, G, Kim, K, Kim, M, Klimentov, A, Kossakowski, R, Koutsenko, V, Kraeber, M, Laborie, G, Laitinen, T, Lamanna, G, Lanciotti, E, Laurenti, G, Lebedev, A, Lechanoine-Leluc, C, Lee, M, Lee, S, Levi, G, Levtchenko, P, Liu, C, Liu, H, Lopes, I, Lu, G, Lu, Y, Lubelsmeyer, K, Luckey, D, Lustermann, W, Mana, C, Margotti, A, Mayet, F, Mcneil, R, Meillon, B, Menichelli, M, Mihul, A, Mourao, A, Mujunen, A, Palmonari, F, Papi, A, Park, H, Park, W, Pauluzzi, M, Pauss, F, Perrin, E, Pesci, A, Pevsner, A, Pimenta, M, Plyaskin, V, Pojidaev, V, Pohl, M, Postolache, V, Produit, N, Rancoita, P, Rapin, D, Raupach, F, Ren, D, Ren, Z, Ribordy, M, Richeux, J, Riihonen, E, Ritakari, J, Ro, S, Roeser, U, Rossin, C, Sagdeev, R, Santos, D, Sartorelli, G, Sbarra, C, Schael, S, von Dratzig, A, Schwering, G, Scolieri, G, Seo, E, Shin, J, Shoutko, V, Shoumilov, E, Siedling, R, Son, D, Song, T, Steuer, M, Sun, G, Suter, H, Tang, X, Ting, S, Tornikoski, M, Torsti, J, Trumper, J, Ulbricht, J, Urpo, S, Valtonen, E, Vandenhirtz, J, Velcea, F, Velikhov, E, Verlaat, B, Vetlitsky, I, Vezzu, F, V, Jp, Viertel, G, Vite, D, Von Gunten, H, Wicki, S, Wallraff, W, Wang, B, Wang, J, Wang, Y, Wiik, K, Williams, C, Wu, S, Xia, P, Yan, J, Yan, L, Yang, C, Yang, J, Yang, M, Ye, S, Yeh, P, Xu, Z, Zhang, H, Zhang, Z, Zhao, D, Zhu, G, Zhu, W, Zhuang, H, Zichichi, A, Zimmermann, B, Zuccon, P, Burger, JD, Burger, WJ, Cai, XD, Chang, YH, Chen, HF, Chen, HS, Chen, ZG, Chernoplekov, NA, Chiueh, TH, Choi, MJ, Choi, YY, Chuang, YL, da Cunha, JP, Dai, TS, Deus, JD, Dong, ZR, Eppling, FJ, Fisher, PH, Gu, WQ, Huang, MA, Kim, DH, Kim, GN, Kim, KS, Kim, MY, Lee, MW, Lee, SC, Liu, CL, Liu, HT, Lu, YS, McNeil, RR, Park, HB, Park, WH, Rancoita, PG, Richeux, JP, von Dratzig, AS, Seo, ES, Shin, JW, Sun, GS, Tang, XW, Ting, SCC, Ting, SM, F Vialle, JP, Wicki, SW, Wang, BC, Wang, JZ, Wang, YH, Wu, SX, Xia, PC, Yan, JL, Yan, LG, Yang, CG, Ye, SW, Xu, ZZ, Zhang, HY, Zhang, ZP, Zhao, DX, Zhu, GY, Zhu, WZ, and Zhuang, HL

Abstract

The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7 deg orbit at altitudes between 320 and 390 km. A search for antihelium nuclei in the rigidity range 1–140 GV was performed. No antihelium nuclei were detected at any rigidity. An upper limit on the flux ratio of antihelium to helium of < 1.1×10^−6 was obtained. The high energy proton, electron, positron, helium, antiproton and deuterium spectra were accurately measured. For each particle and nuclei two distinct spectra were observed: a higher energy spectrum and a substantial second spectrum. Positrons in the second spectrum were found to be much more abundant than electrons. Tracing particles from the second spectra shows that most of them travel for an extended period of time in the geomagnetic field, and that the positive particles (p and e+) and negative ones (e−) originate from two complementary geographic regions. The second helium spectrum flux over the energy range 0.1–1.2 GeV/nucleon was measured to be (6.3 ± 0.9) × 10^−3(m^2 s sr)^−1. Over 90 percent of the helium flux was determined to be 3He at the 90% confidence level

Published
2002

26. The Northern ROSAT All‐Sky (NORAS) Galaxy Cluster Survey. I. X‐Ray Properties of Clusters Detected as Extended X‐Ray Sources

Author

Bohringer, H., primary, Voges, W., additional, Huchra, J. P., additional, McLean, B., additional, Giacconi, R., additional, Rosati, P., additional, Burg, R., additional, Mader, J., additional, Schuecker, P., additional, Simic, D., additional, Komossa, S., additional, Reiprich, T. H., additional, Retzlaff, J., additional, and Trumper, J., additional

Published
2000
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28. A 36 cm/sup 2/ monolithic pn-CCD for X-ray detection on the XMM and ABRIXAS satellites

Author

Holl, P., primary, Bihler, E., additional, Brauninger, H., additional, Briel, U., additional, Hartmann, R., additional, Hartner, G., additional, Hauff, D., additional, Kemmer, J., additional, Kendziorra, E., additional, Krause, N., additional, Lechner, P., additional, Maier, B., additional, Meidinger, N., additional, Pfeffermann, E., additional, Pfluger, B., additional, Popp, M., additional, Reppin, C., additional, Richter, R.H., additional, Soltau, H., additional, Stotter, D., additional, Struder, L., additional, Trumper, J., additional, and van Zanthier, C., additional

Published
1998
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29. ROSATSurvey Diffuse X‐Ray Background Maps. II.

Author

Snowden, S. L., primary, Egger, R., additional, Freyberg, M. J., additional, McCammon, D., additional, Plucinsky, P. P., additional, Sanders, W. T., additional, Schmitt, J. H. M. M., additional, Trumper, J., additional, and Voges, W., additional

Published
1997
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32. JET-X A Joint European X-ray Telescope for SPECTRUM-X

Author

Wells, A., primary, Lumb, D.H., additional, Pounds, K.A., additional, Stewart, G.C., additional, Aschenbach, B., additional, Brauninger, H., additional, Hasinger, G., additional, Trumper, J., additional, Citterio, O., additional, Scarsi, L., additional, Peacock, A., additional, and Taylor, B., additional

Published
1990
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33. X-ray spectral variability of 3C273.

Author

Turner, M., Courvoisier, T., Staubert, R., Molteni, D., and Trumper, J.

Abstract

3C273 has been monitored by EXOSAT over the period December 1983 to June 1984 in 4 observations. In the December observation the flux was high and the spectrum showed a power law index of 1.5 changing to 0.9 at∼8 keV. In subsequent observations the flux dropped to∼40% of its original value and the hard tail disappeared. In the last observation the LE flux increased by a factor of 2 with no accompanying ME flux increase. [ABSTRACT FROM AUTHOR]

Published
1985
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34. A 36 cm[sup 2] large monolythic pn-charge coupled device x-ray detector for the European XMM...

Author

Struder, L., Brauninger, H., Briel, U., Hartmann, R., Hartner, G., Hauff, D., Krause, N., Maier, B., Meidinger, N., Pfeffermann, E., Popp, M., Reppin, C., Richter, R., Stotter, D., Trumper, J., Weber, U., Holl, P., Kemmer, J., and Soltau, H.

Subjects
CHARGE coupled devices, ARTIFICIAL satellites
Abstract

Focuses on monolythic arrays of pn-charge coupled devices that have been developed and produced for the focal plane instrumentation of the high throughput European Photon Imaging Camera. XMM and the German ABRIXAS x-ray satellite mission; Layout topology; Operating conditions guaranteeing ten years operation in space without performance degradation.

Published
1997

36. Observations on sociolinguistics behavior in two Italian regions.

Author

Trumper, J.

Subjects
SOCIOLINGUISTICS, VERBAL behavior, LANGUAGE & culture, LANGUAGE & languages, SOCIOLOGY methodology
Abstract

This article presents observations on sociolinguistic behavior in two Italian regions. A. A. Sobrero states that what is socially relevant in Italian verbal behavior is the choice of code and the factors determine code switching rather than variability in the codes used. The problem remains: how to characterize a continuum of varieties with at one extreme dialect defined as patois, limited in use, at the other hypothetical standard pronunciation, and in between a vast varietal range that compromises the majority of real verbal production by Italian speakers. This continuum might be considered as a series of compartments in which the upper limits of each compartment are at the same time the lower limits of the next and so on. Conversion analysis and direction observation led the author to conclude that most inter-group working class interaction is carried out in dialect, except perhaps in the youngest group analyzed.

Published
1989
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39. GX 3+1

Author

Lewin, W.H.G., van Paradijs, J., Hasinger, G., Penninx, W., van der Klis, M., Jansen, F., Langmeier, A., Sztajno, M., Trumper, J., and API (FNWI)

Published
1986

41. GX 5-1 (4U 1758-250)

Author

van der Klis, M., Jansen, F., van Paradijs, J., Lewin, W.H.G., Trumper, J., Sztajno, M., and API (FNWI)

Published
1985

43. GX 5-1

Author

van der Klis, M., Jansen, F., van Paradijs, J., Lewin, W.H.G., Trumper, J., Sztajno, M., and API (FNWI)

Published
1985

44. Detection of Hard X-Rays from Supernova 1987A - Preliminary Mir-Kvant Results

Author

Syunyaev, Ra, Kaniovskii, A., Efremov, V., Gilfanov, M., Eugene Churazov, Grebenev, Sa, Kuznetsov, Av, Melioranskii, As, Yamburenko, Ns, Yunin, S., Stepanov, D., Chulkov, I., Pappe, N., Boyarskii, Mn, Gavrilova, Ea, Loznikov, Vm, Prudkoglyad, A., Rodin, Vg, Reppin, C., Pietsch, W., Engelhauser, J., Trumper, J., Voges, W., Kendziorra, E., Bezler, M., Staubert, R., Brinkman, Ac, Skinner, Gk, Alemam, O., Patterson, Tg, Willmore, Ap, Heise, J., Mels, Wa, and Jager, R.

45. The results of Alpha Magnetic Spectrometer (AMS) experiment in space

Author

Alpat, B., Alcaraz, J., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Luca Baldini, Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J. D., Burger, W. J., Cai, X. D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y. H., Chen, H. F., Chen, H. S., Chen, Z. G., Chernoplekov, N. A., Chiueh, T. H., Chuang, Y. L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., Da Cunha, J. P., Dai, T. S., Deus, J. D., Dinu, N., Djambazov, L., Antone, I. D., Dong, Z. R., Emonet, P., Engelberg, J., Eppling, F. J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P. H., Fluegge, G., Fouque, N., Yu. Galaktionov, Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W. Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M. A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Giovanni Lamanna, Laurenti, G., Lebedev, A., Lee, S. C., Levi, G., Levtchenko, P., Liu, C. L., Liu, H. T., Lopes, I., Lu, G., Lu, Y. S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., Mcneil, R. R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I. H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P. G., Rapin, D., Raupach, F., Ren, D., Zhuoxiang Ren, Ribordy, M., Richeux, J. P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz Dratzig, A., Schwering, G., Scolieri, G., Seo, E. S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G. S., Suter, H., Tang, X. W., Ting, S. C. C., Ting, S. M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J. P., Viertel, G., Vite, D., Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B. C., Wang, J. Z., Wang, Y. H., Wiik, K., Williams, C., Wu, S. X., Xia, P. C., Yan, J. L., Yan, L. G., Yang, C. G., Yang, M., Ye, S. W., Yeh, P., Xu, Z. Z., Zhang, H. Y., Zhang, Z. P., Zhao, D. X., Zhu, G. Y., Zhu, W. Z., Zhuang, H. L., Zichichi, A., Zimmermann, B., bibliotheque, LPSC, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), 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), and AMS

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]

46. Detection of a Hard Component in the Spectrum of the Vulpecula X-Ray Nova - Preliminary KVANT Results

Author

Syunyaev, R. A., Lapshov, I. Y., Grebenev, S. A., Efremov, V. V., Kaniovskii, A. S., Stepanov, D. K., Yunin, S. N., Gavrilova, E. A., Loznikov, V. M., Prudkoglyad, A. V., Rodin, V. G., Babushkina, O. P., Kiselev, S. V., Kuznetsov, A. V., Melioranskii, A. S., Smith, A., Arvind Parmar, Pietsch, W., Dobereiner, S., Engelhauser, J., Reppin, C., Trumper, J., Voges, W., Kendziorra, E., Maisack, M., Mony, B., and Staubert, R.

47. The results of Alpha Magnetic Spectrometer (AMS) experiment in space

Author

Laboratoire de Physique Subatomique et de Cosmologie (LPSC) ; CNRS - IN2P3 - Université Joseph Fourier - Grenoble I - Institut Polytechnique de Grenoble - Grenoble Institute of Technology, Laboratoire d'Annecy le Vieux de Physique des Particules (LAPP) ; CNRS - IN2P3 - Université de Savoie, AMS, Alpat, B., Alcaraz, J., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y.H., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiueh, T.H., Chuang, Y.L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., Da Cunha, J.P., Dai, T.S., Deus, J.D., Dinu, N., Djambazov, L., D'Antone, I., Dong, Z.R., Emonet, P., Engelberg, J., Eppling, F.J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P.H., Fluegge, G., Fouque, N., Galaktionov, Yu., Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W.Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M.A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Lamanna, G., Laurenti, G., Lebedev, A., Lee, S.C., Levi, G., Levtchenko, P., Liu, C.L., Liu, H.T., Lopes, I., Lu, G., Lu, Y.S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., McNeil, R.R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I.H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P.G., Rapin, D., Raupach, F., Ren, D., Ren, Z., Ribordy, M., Richeux, J.P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz Von Dratzig, A., Schwering, G., Scolieri, G., Seo, E.S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G.S., Suter, H., Tang, X.W., Ting, S.C.C., Ting, S.M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Viertel, G., Vite, D., Von Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B.C., Wang, J.Z., Wang, Y.H., Wiik, K., Williams, C., Wu, S.X., Xia, P.C., Yan, J.L., Yan, L.G., Yang, C.G., Yang, M., Ye, S.W., Yeh, P., Xu, Z.Z., Zhang, H.Y., Zhang, Z.P., Zhao, D.X., Zhu, G.Y., Zhu, W.Z., Zhuang, H.L., Zichichi, A., Zimmermann, B., Laboratoire de Physique Subatomique et de Cosmologie (LPSC) ; CNRS - IN2P3 - Université Joseph Fourier - Grenoble I - Institut Polytechnique de Grenoble - Grenoble Institute of Technology, Laboratoire d'Annecy le Vieux de Physique des Particules (LAPP) ; CNRS - IN2P3 - Université de Savoie, AMS, Alpat, B., Alcaraz, J., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, R., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y.H., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiueh, T.H., Chuang, Y.L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., Da Cunha, J.P., Dai, T.S., Deus, J.D., Dinu, N., Djambazov, L., D'Antone, I., Dong, Z.R., Emonet, P., Engelberg, J., Eppling, F.J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P.H., Fluegge, G., Fouque, N., Galaktionov, Yu., Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W.Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M.A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Lamanna, G., Laurenti, G., Lebedev, A., Lee, S.C., Levi, G., Levtchenko, P., Liu, C.L., Liu, H.T., Lopes, I., Lu, G., Lu, Y.S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., McNeil, R.R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I.H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P.G., Rapin, D., Raupach, F., Ren, D., Ren, Z., Ribordy, M., Richeux, J.P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz Von Dratzig, A., Schwering, G., Scolieri, G., Seo, E.S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G.S., Suter, H., Tang, X.W., Ting, S.C.C., Ting, S.M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Viertel, G., Vite, D., Von Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B.C., Wang, J.Z., Wang, Y.H., Wiik, K., Williams, C., Wu, S.X., Xia, P.C., Yan, J.L., Yan, L.G., Yang, C.G., Yang, M., Ye, S.W., Yeh, P., Xu, Z.Z., Zhang, H.Y., Zhang, Z.P., Zhao, D.X., Zhu, G.Y., Zhu, W.Z., Zhuang, H.L., Zichichi, A., and Zimmermann, B.

48. The results of Alpha Magnetic Spectrometer (AMS) experiment in space

Author

Alpat, B., Alcaraz, J., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, r., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y.H., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiueh, T.H., Chuang, Y.L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., da Cunha, J.P., Dai, T.S., Deus, J.D., Dinu, N., Djambazov, L., D'Antone, I., Dong, Z.R., Emonet, P., Engelberg, J., Eppling, F.J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P.H., Fluegge, G., Fouque, N., Galaktionov, Yu., Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W.Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M.A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Lamanna, G., Laurenti, G., Lebedev, A., Lee, S.C., Levi, G., Levtchenko, P., Liu, C.L., Liu, H.T., Lopes, I., Lu, G., Lu, Y.S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., McNeil, R.R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I.H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P.G., Rapin, D., Raupach, F., Ren, D., Ren, Z., Ribordy, M., Richeux, J.P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz von Dratzig, A., Schwering, G., Scolieri, G., Seo, E.S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G.S., Suter, H., Tang, X.W., Ting, S.C.C., Ting, S.M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Viertel, G., Vite, D., Von Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B.C., Wang, J.Z., Wang, Y.H., Wiik, K., Williams, C., Wu, S.X., Xia, P.C., Yan, J.L., Yan, L.G., Yang, C.G., Yang, M., Ye, S.W., Yeh, P., Xu, Z.Z., Zhang, H.Y., Zhang, Z.P., Zhao, D.X., Zhu, G.Y., Zhu, W.Z., Zhuang, H.L., Zichichi, A., Zimmermann, B., Alpat, B., Alcaraz, J., Ambrosi, G., Anderhub, H., Ao, L., Arefiev, A., Azzarello, P., Babucci, E., Baldini, L., Basile, M., Barancourt, D., Barao, F., Barbier, G., Barreira, G., Battiston, R., Becker, r., Becker, U., Bellagamba, L., Bene, P., Berdugo, J., Berges, P., Bertucci, B., Biland, A., Bizzaglia, S., Blasko, S., Boella, G., Boschini, M., Bourquin, M., Brocco, L., Bruni, G., Buenerd, M., Burger, J.D., Burger, W.J., Cai, X.D., Camps, C., Cannarsa, P., Capell, M., Casadei, D., Casaus, J., Castellini, G., Cecchi, C., Chang, Y.H., Chen, H.F., Chen, H.S., Chen, Z.G., Chernoplekov, N.A., Chiueh, T.H., Chuang, Y.L., Cindolo, F., Commichau, V., Contin, A., Crespo, P., Cristinziani, M., da Cunha, J.P., Dai, T.S., Deus, J.D., Dinu, N., Djambazov, L., D'Antone, I., Dong, Z.R., Emonet, P., Engelberg, J., Eppling, F.J., Eronen, T., Esposito, G., Extermann, P., Favier, J., Fiandrini, E., Fisher, P.H., Fluegge, G., Fouque, N., Galaktionov, Yu., Gervasi, M., Giusti, P., Grandi, D., Grimm, O., Gu, W.Q., Hangarter, K., Hasan, A., Hermel, V., Hofer, H., Huang, M.A., Hungerford, W., Ionica, M., Ionica, R., Jongmanns, M., Karlamaa, K., Karpinski, W., Kenney, G., Kenny, J., Kim, W., Klimentov, A., Kossakowski, R., Koutsenko, V., Kraber, M., Laborie, G., Laitinen, T., Lamanna, G., Laurenti, G., Lebedev, A., Lee, S.C., Levi, G., Levtchenko, P., Liu, C.L., Liu, H.T., Lopes, I., Lu, G., Lu, Y.S., Luebelsmeyer, K., Luckey, D., Lustermann, W., Mana, C., Margotti, A., Mayet, F., McNeil, R.R., Meillon, B., Menichelli, M., Mihul, A., Mourao, A., Mujunen, A., Palmonari, F., Papi, A., Park, I.H., Pauluzzi, M., Pauss, F., Perrin, E., Pesci, A., Pevsner, A., Pimenta, M., Plyaskin, V., Pozhidaev, V., Postolache, V., Produit, N., Rancoita, P.G., Rapin, D., Raupach, F., Ren, D., Ren, Z., Ribordy, M., Richeux, J.P., Riihonen, E., Ritakari, J., Roser, U., Rossin, C., Sagdeev, R., Sartorelli, G., Schultz von Dratzig, A., Schwering, G., Scolieri, G., Seo, E.S., Shoutko, V., Shumilov, E., Siedling, R., Son, D., Song, T., Steuer, M., Sun, G.S., Suter, H., Tang, X.W., Ting, S.C.C., Ting, S.M., Tornikoski, M., Torsti, J., Trumper, J., Ulbricht, J., Urpo, S., Usoskin, I., Valtonen, E., Vandenhirtz, J., Velcea, F., Velikhov, E., Verlaat, B., Vetlitsky, I., Vezzu, F., Vialle, J.P., Viertel, G., Vite, D., Von Gunten, H., Waldmeier Wicki, S., Wallraff, W., Wang, B.C., Wang, J.Z., Wang, Y.H., Wiik, K., Williams, C., Wu, S.X., Xia, P.C., Yan, J.L., Yan, L.G., Yang, C.G., Yang, M., Ye, S.W., Yeh, P., Xu, Z.Z., Zhang, H.Y., Zhang, Z.P., Zhao, D.X., Zhu, G.Y., Zhu, W.Z., Zhuang, H.L., Zichichi, A., and Zimmermann, B.

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