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83 results on '"Moiseev, A.A."'

51. The PAMELA experiment on satellite and its capability in cosmic rays measurements

Author

Adriani, O, Ambriola, M, Barbarino, G, Barbier, L.M, Bartalucci, S, Bazilevskaja, G, Bellotti, R, Bertazzoni, S, Bidoli, V, Boezio, M, Bogomolov, E, Bonechi, L, Bonvicini, V, Boscherini, M, Bravar, U, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellano, M, Castellini, G, Christian, E.R, Ciacio, F, Circella, M, D'Alessandro, R, De Marzo, C.N, De Pascale, M.P, Finetti, N, Furano, G, Gabbanini, A, Galper, A.M, Giglietto, N, Grandi, M, Grigorjeva, A, Guarino, F, Hof, M, Koldashov, S.V, Korotkov, M.G, Krizmanic, J.F, Krutkov, S, Lund, J, Marangelli, B, Marino, L, Menn, W, Mikhailov, V.V, Mirizzi, N, Mitchell, J.W, Mocchiutti, E, Moiseev, A.A, Morselli, A, Mukhametshin, R, Ormes, J.F, Osteria, G, Ozerov, J.V, Papini, P, Pearce, M, Perego, A, Piccardi, S, Picozza, P, Ricci, M, Salsano, A, Schiavon, P, Scian, G, Simon, M, Sparvoli, R, Spataro, B, Spillantini, P, Spinelli, P, Stephens, S.A, Stochaj, S.J, Stozhkov, Y, Straulino, S, Streitmatter, R.E, Taccetti, F, Tesi, M, Vacchi, A, Vannuccini, E, Vasiljev, G, Vignoli, V, Voronov, S.A, Yurkin, Y, Zampa, G, and Zampa, N

Published
2002
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53. On Possible Interpretations of the High Energy Electron-Positron Spectrum Measured by the Fermi Large Area Telescope

Author

Grasso, D., primary, Profumo, S., additional, Strong, A.W., additional, Baldini, L., additional, Bellazzini, R., additional, Bloom, E.D., additional, Bregeon, J., additional, Di Bernardo, G., additional, Gaggero, D., additional, Giglietto, N., additional, Kamae, T., additional, Latronico, L., additional, Longo, F., additional, Mazziotta, M.N., additional, Moiseev, A.A., additional, Morselli, A., additional, Ormes, J.F., additional, Pesce-Rollins, M., additional, Pohl, M., additional, Razzano, M., additional, and Sgro, C., additional

Published
2009
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59. Cross-Polarization Optical Coherence Tomography in Comparative in vivo and ex vivo Studies of the Optical Properties of Normal and Tumorous Brain Tissues

Author

Kiseleva, E.B., primary, Yashin, K.S., additional, Moiseev, A.A., additional, Sirotkina, M.A., additional, Timofeeva, L.B., additional, Fedoseeva, V.V., additional, Alekseeva, A.I., additional, Medyanik, I.A., additional, Karyakin, N.N., additional, Kravets, L.Ya., additional, and Gladkova, N.D., additional

Published
2017
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61. Fermi LAT detection of pulsed $\gamma$-rays from the Vela-like pulsars PSR J1048-5832 and PSR J2229+6114

Author

A. Abdo, A., Ackermann, Markus, Ajello, Marco, Atwood, William B., Axelsson, Magnus, Baldini, Luca, Ballet, Jean, Barbiellini, Guido, Baring, Matthew G., Bastieri, D., Baughman, B. M., Bechtol, K., Bellazzini, R., Berenji, B., Bloom, E.D., Bonamente, E., Borgland, A.W., Bregeon, J., Brez, A., Brigida, M., Bruel, Pascal, Caliandro, G. A., Cameron, R. A., Camilo, F., Caraveo, P. A., Casandjian, J.M., Cecchi, C., Chekhtman, A., Cheung, C.C., Chiang, J., Ciprini, S., Claus, R., Cognard, Ismaël, Cohen-Tanugi, J., Conrad, J., De Angelis, A., De Palma, F., Dormody, M., Silva, E.D.E., Drell, P.S., Dubois, R., Dumora, D., Farnier, C., Favuzzi, C., Frailis, M., Freire, P.C.C., Fukazawa, Y., Funk, S., Fusco, P., Gargano, F., Gehrels, N., Germani, S., Giebels, B., Giglietto, N., Giordano, F., Glanzman, T., Godfrey, G., Grenier, I.A., Grondin, M.H., Grove, J.E., Guillemot, L., Guiriec, S., Halpern, J. P., Hanabata, Y., Harding, A.K., Hayashida, M., Hays, E., Hobbs, G., Hugues, R.E., Johansson, G., Johnson, A. S., Johnson, R. P., Johnson, T. J., Johnson, W. N., Johnston, S., Kamae, T., Katagiri, H., Kataoka, J., Kawai, N., Kerr, M., Knödlseder, J., Kocian, M. L., Kramer, M., Kuehn, F., Kuss, M., Lande, J., Latronico, L., Lemoine-Goumard, M., Longo, F., Loparco, F., Lott, B., Lovellette, M.N., Lubrano, P., Lyne, A.G., Makeev, A., Manchester, R.N., Marelli, M., Mazziotta, M.N., Mcenery, J.E., Meurer, C., Michelson, P.F., Mitthumsiri, W., Mizuno, T., Moiseev, A.A., Monte, C., Monzani, M.E., Morselli, A., Moskalenko, I.V., Murgia, S., Nolan, P.L., Norris, J. P., Noutsos, A., Nuss, E., Ohsugi, T., Omodei, N., Orlando, E., Ormes, J.F., Ozaki, M., Paneque, D., Panetta, J.H., Parent, D., Pepe, M., Pesce-Rollins, M., Piron, F., Porter, T.A., Rainò, S., Rando, R., Ransom, S.M., Razzano, M., Reimer, A., Reimer, O., Reposeur, T., Rochester, L.S., Rodriguez, A.Y., Romani, R.W., Roth, M., Ryde, F., Sadrosinski, H.F-W., Sanchez, D., Sander, A., Saz Parkinson, P.M., Scargle, J.D., Sgrò, C., Siskind, E.J., Smith, D.A., Smith, P.D., Spandre, G., Spinelli, P., Stappers, B.W., Strickman, M.S., Suson, D.J., Tajima, H., Takahashi, H., Tanaka, T., Thayer, J.B., Thayer, J.G., Theureau, G., Thompson, D. J., Thorsett, S.E., Tibaldo, L., Torres, D.F., Tosti, G., Uchiyama, Y., Usher, T. L., Van Etten, A., Vilchez, N., Vitale, V., Waite, A. P., Wang, P., Wang, N., Watters, K., Weltevrede, P., Winer, B. L., Wood, K.S., Ylinen, T., Ziegler, M., Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de physique et chimie de l'environnement (LPCE), Université d'Orléans (UO)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Laboratoire de Physique Théorique et Astroparticules (LPTA), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Fermi-LAT, Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-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)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), and Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics of Galaxies (astro-ph.GA), pulsars: general, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], FOS: Physical sciences, PSr J222+6114), Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, gamma rays: observations, pulsars: individual (PSR J1048-5832
Abstract

We report the detection of gamma-ray pulsations (> 0.1 GeV) from PSR J2229+6114 and PSR J1048-5832, the latter having been detected as a low-significance pulsar by EGRET. Data in the gamma-ray band were acquired by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope, while the radio rotational ephemerides used to fold the gamma-ray light curves were obtained using the Green Bank Telescope, the Lovell telescope at Jodrell Bank, and the Parkes telescope. The two young radio pulsars, located within the error circles of the previously unidentified EGRET sources 3EG J1048-5840 and 3EG J2227+6122, present spin-down characteristics similar to the Vela pulsar. PSR J1048-5832 shows two sharp peaks at phases 0.15 \pm 0.01 and 0.57 \pm 0.01 relative to the radio pulse confirming the EGRET light curve, while PSR J2229+6114 presents a very broad peak at phase 0.49 \pm 0.01. The gamma-ray spectra above 0.1 GeV of both pulsars are fit with power laws having exponential cutoffs near 3 GeV, leading to integral photon fluxes of (2.19 \pm 0.22 \pm 0.32) x 10^{-7} cm^{-2} ^{-1} for PSR J1048-5832 and (3.77 \pm 0.22 \pm 0.44) x 10^{-7} cm^{-2} s^{-1} for PSR J2229+6114. The first uncertainty is statistical and the second is systematic. PSR J1048-5832 is one of two LAT sources which were entangled together as 3EG J1048-5840. These detections add to the growing number of young gamma-ray pulsars that make up the dominant population of GeV gamma-ray sources in the Galactic plane., 11 pages, 4 figures, 1 table. Accepted for publication in Astrophysical Journal. Contact authors: Alice K. Harding (ahardingx@yahoo.com), Damien Parent (parent@cenbg.in2p3.fr), Massimiliano Razzano (massimiliano.razzano@pi.infn.it)

Published
2009
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62. Measurement of the Cosmic Ray e(+)+e(-) Spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

Author

Abdo, A.A., Ackermann, Markus, Ajello, Marco, B. Atwood, W., Axelsson, Magnus, Baldini, Luca, Ballet, Jean, Barbiellini, Guido, Bastieri, D., Battelino, M., Baughmann, B.M., Bechtol, K., Bellazzini, R., Berenji, B., Blandford, R. D., Bloom, E.D., Bogaert, G., Bonamente, E., Borgland, A.W., Bregeon, J., Brez, A., Brigida, M., Bruel, Pascal, Burnett, T.H., A.Caliandro, G., Cameron, R.A., Caraveo, P. A., Carlson, P., Casandjian, J.M., Cecchi, C., Charles, E., Chekhtman, A., Cheung, C.C., Chiang, J., Ciprini, S., Claus, R., Cohen-Tanugi, J., Cominski, L.R., Conrad, J., Cutini, S., D. Dermer, C., De Angelis, A., De Palma, F., Digel, S.W., Di Bernardo, G., Silva, E.D.E., Drell, P.S., Dubois, R., Dumora, D., Edmonds, Y., Farnier, C., Favuzzi, C., Focke, W.B., Frailis, M., Fukazawa, Y., Funk, S., Fusco, P., Gaggero, D., Gargano, F., Gasparrini, D., Gehrels, N., Germani, S., Giebels, B., Giglietto, N., Giordano, F., Glanzman, T., Godfrey, G., Grasso, D., Grenier, I.A., Grondin, M.-H., Grove, J.E., Guillemot, L., Guiriec, S., Hanabata, Y., Harding, A.K., Hartman, R.C., Hayashida, M., Hays, E., Hugues, R.E., Johannesson, G., Johnson, A.S., Johnson, R.P., Johnson, W.N., Kamae, T., Katagiri, H., Kataoka, J., Kerr, M., Knödlseder, Jürgen, Kocevski, D., Kuehn, F., Kuss, M., Lande, J., Latronico, L., Lemoine-Goumard, M., Longo, F., Loparco, F., Lott, B., Lovellette, M.N., Lubrano, P., Madejski, G. M., Makeev, A., Massai, M.M., Mazziotta, M.N., Mcconville, W., Mcenery, J.E., Meurer, C., Michelson, P.F., Mitthumsiri, W., Mizuno, T., Moiseev, A.A., Monte, C., Monzani, M.E., Moretti, E., Morselli, A., Moskalenko, I.V., Murgia, S., Nolan, P.L., Norris, J.P., Nuss, E., Ohsugi, T., Omodei, N., Orlando, E., Ormes, J.F., Ozaki, M., Paneque, D., Panetta, J.H., Parent, D., Pelassa, V., Pepe, M., Pesce-Rollins, M., Piron, F., Pohl, M., Porter, T.A., Profumo, S., Rainò, S., Rando, R., Razzano, M., Reimer, A., Reimer, O., Reposeur, T., Ritz, S., Rochester, L. S., Rodriguez, A. Y., Romani, R.W., Roth, M., Ryde, F., Sadrosinski, H.F-W., Sanchez, D., Sander, A., Saz Parkinson, P.M., Scargle, J. D., Schalk, T. L., Sellerholm, A., Sgro, G., Smith, D. A., Smith, P. D., Spandre, G., Spinelli, P., Starck, Jean-Luc, Stephens, T. E., Strickman, M.S., Strong, A.W., Suson, D. J., Tajima, H., Takahashi, H., Takahashi, T., Tanaka, T., Thayer, J. G., Thompson, D.J., Tibaldo, L., Tibolla, O., Torres, D.F., Tosti, G., Tramacere, A., Uchiyama, Y., Usher, T. L., Van Etten, A., Vasileiou, V., Vilchez, N., Vitale, V., Waite, A. P., Wallace, E., Wang, P., Winer, B. L., Wood, K. S., Ylinen, T., Ziegler, M., Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Théorique et Astroparticules (LPTA), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Fermi-LAT, Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-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)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), and Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], 96.50.sb, 95.35.+d, 95.85.Ry, 98.70.Sa
Abstract

Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2 m2 sr at 300 GeV. Building on the gamma-ray analysis, we have developed an efficient electron detection strategy which provides sufficient background rejection for measurement of the steeply falling electron spectrum up to 1 TeV. Our high precision data show that the electron spectrum falls with energy as E-3.0 and does not exhibit prominent spectral features. Interpretations in terms of a conventional diffusive model as well as a potential local extra component are briefly discussed.

Published
2009
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65. Constraints on dark matter annihilation in clusters of galaxies with the Fermi large area telescope

Author

Ackermann, M, primary, Ajello, M, additional, Allafort, A, additional, Baldini, L, additional, Ballet, J, additional, Barbiellini, G, additional, Bastieri, D, additional, Bechtol, K, additional, Bellazzini, R, additional, Blandford, R.D, additional, Bloom, E.D, additional, Bonamente, E, additional, Borgland, A.W, additional, Bouvier, A, additional, Brandt, T.J, additional, Bregeon, J, additional, Brigida, M, additional, Bruel, P, additional, Buehler, R, additional, Buson, S, additional, Caliandro, G.A, additional, Cameron, R.A, additional, Caraveo, P.A, additional, Carrigan, S, additional, Casandjian, J.M, additional, Cecchi, C, additional, Charles, E, additional, Chekhtman, A, additional, Cheung, C.C, additional, Chiang, J, additional, Ciprini, S, additional, Claus, R, additional, Cohen-Tanugi, J, additional, Cominsky, L.R, additional, Conrad, J, additional, Angelis, A. de, additional, Palma, F. de, additional, Silva, E. do Couto e, additional, Drell, P.S, additional, Drlica-Wagner, A, additional, Dubois, R, additional, Dumora, D, additional, Edmonds, Y, additional, Farnier, C, additional, Favuzzi, C, additional, Fegan, S.J, additional, Frailis, M, additional, Fukazawa, Y, additional, Fusco, P, additional, Gargano, F, additional, Gasparrini, D, additional, Gehrels, N, additional, Germani, S, additional, Giglietto, N, additional, Giordano, F, additional, Glanzman, T, additional, Godfrey, G, additional, Grenier, I.A, additional, Guiriec, S, additional, Gustafsson, M, additional, Harding, A.K, additional, Hayashida, M, additional, Horan, D, additional, Hughes, R.E, additional, Jeltema, T.E, additional, Jóhannesson, G, additional, Johnson, A S, additional, Johnson, W.N, additional, Kamae, T, additional, Katagiri, H, additional, Kataoka, J, additional, Knödlseder, J, additional, Kuss, M, additional, Lande, J, additional, Latronico, L, additional, Lee, S.-H, additional, Garde, M. Llena, additional, Longo, F, additional, Loparco, F, additional, Lovellette, M.N, additional, Lubrano, P, additional, Madejski, G.M, additional, Makeev, A, additional, Mazziotta, M.N, additional, Michelson, P.F, additional, Mitthumsiri, W, additional, Mizuno, T, additional, Moiseev, A.A, additional, Monte, C, additional, Monzani, M.E, additional, Morselli, A, additional, Moskalenko, I.V, additional, Murgia, S, additional, Nolan, P.L, additional, Norris, J.P, additional, Nuss, E, additional, Ohno, M, additional, Ohsugi, T, additional, Omodei, N, additional, Orlando, E, additional, Ormes, J.F, additional, Panetta, J.H, additional, Pepe, M, additional, Pesce-Rollins, M, additional, Piron, F, additional, Porter, T.A, additional, Profumo, S, additional, Rainò, S, additional, Razzano, M, additional, Reposeur, T, additional, Ritz, S, additional, Rodriguez, A.Y, additional, Roth, M, additional, Sadrozinski, H.F.-W, additional, Sander, A, additional, Scargle, J.D, additional, Sgrò, C, additional, Siskind, E.J, additional, Smith, P.D, additional, Spandre, G, additional, Spinelli, P, additional, Starck, J.-L, additional, Strickman, M.S, additional, Suson, D.J, additional, Takahashi, H, additional, Tanaka, T, additional, Thayer, J.B, additional, Thayer, J.G, additional, Tibaldo, L, additional, Torres, D.F, additional, Tosti, G, additional, Usher, T.L, additional, Vasileiou, V, additional, Vitale, V, additional, Waite, A.P, additional, Wang, P, additional, Winer, B.L, additional, Wood, K.S, additional, Yang, Z, additional, Ylinen, T, additional, and Ziegler, M, additional

Published
2010
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66. Measurement of the cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight

Author

Abe, K., primary, Fuke, H., additional, Haino, S., additional, Hams, T., additional, Itazaki, A., additional, Kim, K.C., additional, Kumazawa, T., additional, Lee, M.H., additional, Makida, Y., additional, Matsuda, S., additional, Matsumoto, K., additional, Mitchell, J.W., additional, Moiseev, A.A., additional, Myers, Z., additional, Nishimura, J., additional, Nozaki, M., additional, Orito, R., additional, Ormes, J.F., additional, Sasaki, M., additional, Seo, E.S., additional, Shikaze, Y., additional, Streitmatter, R.E., additional, Suzuki, J., additional, Takasugi, Y., additional, Takeuchi, K., additional, Tanaka, K., additional, Yamagami, T., additional, Yamamoto, A., additional, Yoshida, T., additional, and Yoshimura, K., additional

Published
2008
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68. Measurements of 0.2–20GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer

Author

Shikaze, Y., primary, Haino, S., additional, Abe, K., additional, Fuke, H., additional, Hams, T., additional, Kim, K.C., additional, Makida, Y., additional, Matsuda, S., additional, Mitchell, J.W., additional, Moiseev, A.A., additional, Nishimura, J., additional, Nozaki, M., additional, Orito, S., additional, Ormes, J.F., additional, Sanuki, T., additional, Sasaki, M., additional, Seo, E.S., additional, Streitmatter, R.E., additional, Suzuki, J., additional, Tanaka, K., additional, Yamagami, T., additional, Yamamoto, A., additional, Yoshida, T., additional, and Yoshimura, K., additional

Published
2007
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69. Erratum to: “Measurements of proton, helium and muon spectra at small atmospheric depths with the BESS spectrometer” [Phys. Lett. B 564 (2003) 8]

Author

Abe, K., primary, Sanuki, T., additional, Anraku, K., additional, Asaoka, Y., additional, Fuke, H., additional, Haino, S., additional, Ikeda, N., additional, Imori, M., additional, Izumi, K., additional, Maeno, T., additional, Makida, Y., additional, Matsuda, S., additional, Matsui, N., additional, Matsukawa, T., additional, Matsumoto, H., additional, Mitchell, J.W., additional, Moiseev, A.A., additional, Nishimura, J., additional, Nozaki, M., additional, Orito, S., additional, Ormes, J.F., additional, Sasaki, M., additional, Seo, E.S., additional, Shikaze, Y., additional, Sonoda, T., additional, Streitmatter, R.E., additional, Suzuki, J., additional, Tanaka, K., additional, Tanizaki, K., additional, Yamagami, T., additional, Yamamoto, A., additional, Yamamoto, Y., additional, Yamato, K., additional, Yoshida, T., additional, and Yoshimura, K., additional

Published
2007
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70. Measurements of atmospheric antiprotons

Author

Yamato, K., primary, Abe, K., additional, Fuke, H., additional, Haino, S., additional, Makida, Y., additional, Matsuda, S., additional, Matsumoto, H., additional, Mitchell, J.W., additional, Moiseev, A.A., additional, Nishimura, J., additional, Nozaki, M., additional, Orito, S., additional, Ormes, J.F., additional, Sanuki, T., additional, Sasaki, M., additional, Seo, E.S., additional, Shikaze, Y., additional, Streitmatter, R.E., additional, Suzuki, J., additional, Tanaka, K., additional, Yamagami, T., additional, Yamamoto, A., additional, Yoshida, T., additional, and Yoshimura, K., additional

Published
2006
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71. Measurements of primary and atmospheric cosmic-ray spectra with the BESS-TeV spectrometer

Author

Haino, S., primary, Sanuki, T., additional, Abe, K., additional, Anraku, K., additional, Asaoka, Y., additional, Fuke, H., additional, Imori, M., additional, Itasaki, A., additional, Maeno, T., additional, Makida, Y., additional, Matsuda, S., additional, Matsui, N., additional, Matsumoto, H., additional, Mitchell, J.W., additional, Moiseev, A.A., additional, Nishimura, J., additional, Nozaki, M., additional, Orito, S., additional, Ormes, J.F., additional, Sasaki, M., additional, Seo, E.S., additional, Shikaze, Y., additional, Streitmatter, R.E., additional, Suzuki, J., additional, Takasugi, Y., additional, Tanaka, K., additional, Tanizaki, K., additional, Yamagami, T., additional, Yamamoto, A., additional, Yamamoto, Y., additional, Yamato, K., additional, Yoshida, T., additional, and Yoshimura, K., additional

Published
2004
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72. Measurements of proton, helium and muon spectra at small atmospheric depths with the BESS spectrometer

Author

Abe, K, primary, Sanuki, T, additional, Anraku, K, additional, Asaoka, Y, additional, Fuke, H, additional, Haino, S, additional, Ikeda, N, additional, Imori, M, additional, Izumi, K, additional, Maeno, T, additional, Makida, Y, additional, Matsuda, S, additional, Matsui, N, additional, Matsukawa, T, additional, Matsumoto, H, additional, Mitchell, J.W, additional, Moiseev, A.A, additional, Nishimura, J, additional, Nozaki, M, additional, Orito, S, additional, Ormes, J.F, additional, Sasaki, M, additional, Seo, E.S, additional, Shikaze, Y, additional, Sonoda, T, additional, Streitmatter, R.E, additional, Suzuki, J, additional, Tanaka, K, additional, Tanizaki, K, additional, Yamagami, T, additional, Yamamoto, A, additional, Yamamoto, Y, additional, Yamato, K, additional, Yoshida, T, additional, and Yoshimura, K, additional

Published
2003
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80. Bimodal imaging of functional changes in blood flow using optoacoustic and optical coherent angiography

Author

Orlova, A.G., Subochev, P.V., Moiseev, A.A., Smolina, E.O., Ksenofontov, S.Yu., Kirillin, M.Yu., and Shakhova, N.M.

Abstract

The results of a complementary study of functional changes of the blood flow in human superficial tissues using optoacoustic (OA) microscopy and angiographic optical coherent tomography (OCT-A) during an occlusive test are demonstrated for the first time. OA microscopy data allow one to estimate the increase in blood content during the occlusive test, while OCT-A data demonstrate a decrease in the number of vessels with a functioning blood flow in the area of interest. The combined approach reported in the paper can be employed in experimental and clinical medicine to study the functional changes of microcirculation in diagnostics of vascular pathologies of superficial tissues and to evaluate the microcirculation response to treatment.

Published
2019
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82. Improvement of lateral resolution of spectral domain optical coherence tomography images in out-of-focus regions with holographic data processing techniques

Author

Moiseev, A.A., Gelikonov, G.V., Terpelov, D.A., Shilyagin, P.A., and Gelikonov, V.M.

Abstract

An analogy between spectral-domain optical coherence tomography (SD OCT) data and broadband digital holography data is considered. Based on this analogy, a method for processing SD OCT data, which makes it possible to construct images with a lateral resolution in the whole investigated volume equal to the resolution in the in-focus region, is developed. Several issues concerning practical application of the proposed method are discussed.

Published
2014
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83. Achromatic registration of quadrature components of the optical spectrum in spectral domain optical coherence tomography

Author

Shilyagin, P.A., Gelikonov, G.V., Gelikonov, V.M., Moiseev, A.A., and Terpelov, D.A.

Abstract

We have thoroughly investigated the method of simultaneous reception of spectral components with the achromatised quadrature phase shift between two portions of a reference wave, designed for the effective suppression of the ‘mirror’ artefact in the resulting image obtained by means of spectral domain optical coherence tomography (SD OCT). We have developed and experimentally tested a phase-shifting element consisting of a beam divider, which splits the reference optical beam into the two beams, and of delay lines being individual for each beam, which create a mutual phase difference of in the double pass of the reference beam. The phase shift achromatism over a wide spectral range is achieved by using in the delay lines the individual elements with different dispersion characteristics. The ranges of admissible adjustment parameters of the achromatised delay line are estimated for exact and inexact conformity of the geometric characteristics of its components to those calculated. A possibility of simultaneous recording of the close-to-quadrature spectral components with a single linear photodetector element is experimentally confirmed. The suppression of the artefact mirror peak in the OCT-signal by an additional relative to the level of its suppression is experimentally achieved when the air delay line is used. Two-dimensional images of the surface positioned at an angle to the axis of the probe beam are obtained with the correction of the ‘mirror’ artefact while maintaining the dynamic range of the image.

Published
2014
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