Home > Publications database > Search for Early Gamma-Ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi Lat > print

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024 7 _ |a 10.1088/0004-637X/807/2/169
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024 7 _ |a 0004-637X
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024 7 _ |a 0004-637x
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024 7 _ |a 1538-4357
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024 7 _ |a WOS:000358967000055
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024 7 _ |a 10.3204/PUBDB-2016-00030
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082 _ _ |a 520
100 1 _ |a Ackermann, Markus
|0 P:(DE-H253)PIP1014130
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245 _ _ |a Search for Early Gamma-Ray Production in Supernovae Located in a Dense Circumstellar Medium with the Fermi Lat
260 _ _ |a Chicago, Ill. [u.a.]
|c 2015
|b Univ.11032
336 7 _ |a article
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336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
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500 _ _ |a (c) The American Astronomical Society
520 _ _ |a Supernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV γ-rays and TeV neutrinos on a timescale of several months. We perform the first systematic search for γ-ray emission in Fermi Large Area Telescope data in the energy range from $100\;\mathrm{MeV}$ to $300\;\mathrm{GeV}$ from the ensemble of 147 SNe Type IIn exploding in a dense CSM. We search for a γ-ray excess at each SNe location in a one-year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months, and 3 months). For the most promising source of the sample, SN 2010jl (PTF 10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in γ-rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases. In addition, we derive limits on the γ-ray luminosity and the ratio of γ-ray-to-optical luminosity ratio as a function of the index of the proton injection spectrum assuming a generic γ-ray production model. Furthermore, we present detailed flux predictions based on multi-wavelength observations and the corresponding flux upper limit at a 95% confidence level (CL) for the source SN 2010jl (PTF 10aaxf).
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
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536 _ _ |a NONTHERMTRANSIENTS - Understanding the variable and transient non-thermal emission of Galactic sources (275861)
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|f FP7-PEOPLE-2010-IOF
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536 _ _ |a COSMICEXPLOSIONS - The nature of cosmic explosions (307260)
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700 1 _ |a Arcavi, I.
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700 1 _ |a Baldini, L.
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700 1 _ |a Ballet, J.
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700 1 _ |a Barbiellini, G.
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700 1 _ |a Bastieri, D.
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700 1 _ |a Bellazzini, R.
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700 1 _ |a Bissaldi, E.
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700 1 _ |a Blandford, R. D.
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700 1 _ |a Bonino, R.
|b 9
700 1 _ |a Bottacini, E.
|b 10
700 1 _ |a Brandt, T. J.
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700 1 _ |a Bregeon, J.
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700 1 _ |a Bruel, P.
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700 1 _ |a Buehler, R.
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700 1 _ |a Buson, S.
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700 1 _ |a Caliandro, G. A.
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700 1 _ |a Cameron, R. A.
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700 1 _ |a Caragiulo, M.
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700 1 _ |a Caraveo, P. A.
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700 1 _ |a Cavazzuti, E.
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700 1 _ |a Cecchi, C.
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700 1 _ |a Charles, E.
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700 1 _ |a Chekhtman, A.
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700 1 _ |a Chiang, J.
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700 1 _ |a Chiaro, G.
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700 1 _ |a Ciprini, S.
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700 1 _ |a Claus, R.
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700 1 _ |a Cohen-Tanugi, J.
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700 1 _ |a Cutini, S.
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700 1 _ |a D’Ammando, F.
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700 1 _ |a Angelis, A. de
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700 1 _ |a Palma, F. de
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700 1 _ |a Desiante, R.
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700 1 _ |a Venere, L. Di
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700 1 _ |a Drell, P. S.
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700 1 _ |a Favuzzi, C.
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700 1 _ |a Fegan, S. J.
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700 1 _ |a Franckowiak, A.
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700 1 _ |a Funk, S.
|b 39
700 1 _ |a Fusco, P.
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700 1 _ |a Gal-Yam, A.
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700 1 _ |a Gargano, F.
|b 42
700 1 _ |a Gasparrini, D.
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700 1 _ |a Giglietto, N.
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700 1 _ |a Giordano, F.
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700 1 _ |a Giroletti, M.
|b 46
700 1 _ |a Glanzman, T.
|b 47
700 1 _ |a Godfrey, G.
|b 48
700 1 _ |a Grenier, I. A.
|b 49
700 1 _ |a Grove, J. E.
|b 50
700 1 _ |a Guiriec, S.
|b 51
700 1 _ |a Harding, A. K.
|b 52
700 1 _ |a Hayashi, K.
|b 53
700 1 _ |a Hewitt, J. W.
|b 54
700 1 _ |a Hill, A. B.
|b 55
700 1 _ |a Horan, D.
|b 56
700 1 _ |a Jogler, T.
|b 57
700 1 _ |a Jóhannesson, G.
|b 58
700 1 _ |a Kocevski, D.
|b 59
700 1 _ |a Kuss, M.
|b 60
700 1 _ |a Larsson, S.
|b 61
700 1 _ |a Lashner, J.
|b 62
700 1 _ |a Latronico, L.
|b 63
700 1 _ |a Li, J.
|b 64
700 1 _ |a Li, L.
|b 65
700 1 _ |a Longo, F.
|b 66
700 1 _ |a Loparco, F.
|b 67
700 1 _ |a Lovellette, M. N.
|b 68
700 1 _ |a Lubrano, P.
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700 1 _ |a Malyshev, D.
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700 1 _ |a Mayer, Michael
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700 1 _ |a Mazziotta, M. N.
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700 1 _ |a McEnery, J. E.
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700 1 _ |a Michelson, P. F.
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700 1 _ |a Mizuno, T.
|b 75
700 1 _ |a Monzani, M. E.
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700 1 _ |a Morselli, A.
|b 77
700 1 _ |a Murase, K.
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700 1 _ |a Nugent, P.
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700 1 _ |a Nuss, E.
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700 1 _ |a Ofek, E.
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700 1 _ |a Ohsugi, T.
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700 1 _ |a Orienti, M.
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700 1 _ |a Orlando, E.
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700 1 _ |a Ormes, J. F.
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700 1 _ |a Paneque, D.
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700 1 _ |a Pesce-Rollins, M.
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700 1 _ |a Piron, F.
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700 1 _ |a Pivato, G.
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700 1 _ |a Rainò, S.
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700 1 _ |a Rando, R.
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700 1 _ |a Razzano, M.
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700 1 _ |a Reimer, A.
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700 1 _ |a Reimer, O.
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700 1 _ |a Schulz, A.
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700 1 _ |a Sgrò, C.
|b 96
700 1 _ |a Siskind, E. J.
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700 1 _ |a Spada, F.
|b 98
700 1 _ |a Spandre, G.
|b 99
700 1 _ |a Spinelli, P.
|b 100
700 1 _ |a Suson, D. J.
|b 101
700 1 _ |a Takahashi, H.
|b 102
700 1 _ |a Thayer, J. B.
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700 1 _ |a Tibaldo, L.
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700 1 _ |a Torres, D. F.
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700 1 _ |a Troja, E.
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700 1 _ |a Vianello, G.
|b 107
700 1 _ |a Werner, M.
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700 1 _ |a Wood, K. S.
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700 1 _ |a Wood, M.
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773 _ _ |a 10.1088/0004-637X/807/2/169
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