Search Results - "Strickman, M . S."

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    The calibration and environmental testing of the engineering module of GLAST CsI calorimeter by Ampe, J., Chekhtman, A., Dizon, P., Grove, J.E., Johnson, W.N., Leas, B.E., Sandora, D.P., Strickman, M.S.

    Published in IEEE transactions on nuclear science (01-10-2004)
    “…GLAST is the next generation space-based gamma ray telescope for the energy range 30 MeV-300 GeV, to be launched by NASA in 2007. For photon energy…”
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    Journal Article
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    Search for Compton-backscattered annihilation radiation from the galactic center with the OSSE by Smith, D. M., Leventhal, M., Gehrels, N., Tueller, J., Johnson, W. N., Kinzer, R. L., Kurfess, J. D., Strickman, M . S., Grabelsky, D. A., Purcell, W. R.

    Published in The Astrophysical journal (10-04-1995)
    “…An emission feature near 170 keV, interpreted as Compton-backscattered 511 keV positron-annihilation radiation, has been reported twice by balloon-borne…”
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    Journal Article
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    Observations of a large flare in GX 1+4 with the Compton Gamma Ray Observatory by Staubert, R., Maisack, M., Kendziorra, E., Draxler, T., Finger, M.H., Fishman, G.J., Strickman, M.S., Starr, C.H.

    Published in Advances in space research (01-05-1995)
    “…The pulsating X-ray binary GX 1+4 (4U 1728-24) was observed by OSSE onboard the Compton Gamma Ray Observatory from 9 to 21 September 1993 as a target of…”
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    Journal Article
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    The Radio/Gamma-Ray Connection in Active Galactic Nuclei in the Era of the Fermi Large Area Telescope by Ackermann, M, Ajello, M, Allafort, A, Angelakis, E, Baldini, L, Ballet, J, Barbiellini, G, Bastieri, D, Bellazzini, R, Berenji, B, Blandford, R. D, Bloom, E. D, Borgland, A. W, Bouvier, A, Bregeon, J, Brez, A, Brigida, M, Bruel, P, Caraveo, P. A, Casandjian, J. M, Cecchi, C, Charles, E, Chekhtman, A, Ciprini, S, Claus, R, Cutini, S, de Palma, F, Dubois, R, Dumora, D, Escande, L, Favuzzi, C, Fegan, S. J, Frailis, M, Fukazawa, Y, Fusco, P, Gargano, F, Gasparrini, D, Giglietto, N, Giommi, P, Giordano, F, Grandi, P, Guiriec, S, Hadasch, D, Hayashida, M, Healey, S. E, Johnson, A. S, Kamae, T, Kataoka, J, Kuss, M, Lande, J, Lee, S.-H, Lott, B, Lubrano, P, Makeev, A, Max-Moerbeck, W, McEnery, J. E, Mehault, J, Michelson, P. F, Mizuno, T, Monte, C, Moskalenko, I. V, Murgia, S, Naumann-Godo, M, Nishino, S, Norris, J. P, Nuss, E, Ohsugi, T, Orlando, E, Ormes, J. F, Ozaki, M, Paneque, D, Pavlidou, V, Pelassa, V, Pepe, M, Pesce-Rollins, M, Pierbattista, M, Piron, F, Readhead, A, Reimer, A, Reimer, O, Romani, R. W, Sgrò, C, Siskind, E. J, Smith, P. D, Spandre, G, Suson, D. J, Takahashi, H, Tanaka, T, Thayer, J. G, Thayer, J. B, Thompson, D. J, Torres, D. F, Tosti, G, Tramacere, A, Vianello, G, Waite, A. P, Wang, P, Winer, B. L, Wood, K. S, Ziegler, M

    Published in The Astrophysical journal (01-11-2011)
    “…We present a detailed statistical analysis of the correlation between radio and gamma-ray emission of the active galactic nuclei (AGNs) detected by Fermi…”
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    The soft gamma-ray spectrum of A0535+26: Detection of an absorption feature at 110 keV by OSSE by Grove, J. E., Strickman, M. S., Johnson, W. N., Kurfess, J. D., Kinzer, R. L., Starr, C. H., Jung, G. V., Kendziorra, E., Maisack, M., Staubert, R.

    Published in The Astrophysical journal (01-01-1995)
    “…We present soft gamma-ray observations by the Oriented Scintillation Spectrometer Experiment (OSSE) on the Compton Gamma Ray Observatory (GRO) of the transient…”
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    An advanced Compton telescope based on thick, position-sensitive solid-state detectors by Kurfess, J.D., Johnson, W.N., Kroeger, R.A., Novikova, E.I., Phlips, B.F., Strickman, M.S., Wulf, E.A.

    Published in New astronomy reviews (01-02-2004)
    “…The development of high-resolution, position-sensitive solid-state detectors enables γ-ray instruments with improved sensitivity and imaging capabilities. For…”
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    Gamma-ray line emission from SN1987A by Matz, S. M., Share, G. H., Leising, M. D., Chupp, E. L., Vestrand, W. T.

    Published in Nature (London) (04-02-1988)
    “…The inferred average line flux at about 847 keV in the background-subtracted spectrum of SN1987A from August 1 to October 31, 1987 is about (1.0 + or - 0.25) x…”
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