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  • 201.
    Petroff, E.
    et al.
    Netherlands Inst Radio Astron, Netherlands.
    Burke-Spolaor, S.
    Natl Radio Astron Observ, USA.
    Keane, E. F.
    Swinburne Univ Technol, Australia.
    McLaughlin, M. A.
    W Virginia Univ, USA.
    Miller, R.
    W Virginia Univ, USA.
    Andreoni, I.
    Swinburne Univ Technol, Australia.
    Bailes, M.
    Swinburne Univ Technol, Australia.
    Barr, E. D.
    Swinburne Univ Technol, Australia.
    Bernard, S. R.
    Swinburne Univ Technol, Australia.
    Bhandari, S.
    Swinburne Univ Technol, Australia.
    Bhat, N. D. R.
    ARC Ctr Excellence All Sky Astrophys CAASTRO, Australia.
    Burgay, M.
    INAF Osservatorio Astron Cagliari, Italy.
    Caleb, M.
    Australia Telescope Natl Facil, Australia.
    Champion, D.
    Max Planck Inst Radioastron, Germany.
    Chandra, P.
    Tata Inst Fundamental Res, India.
    Cooke, J.
    Swinburne Univ Technol, Australia.
    Dhillon, V. S.
    Univ Sheffield, UK.
    Farnes, J. S.
    Radboud Univ Nijmegen, Netherlands.
    Hardy, L. K.
    Univ Sheffield, UK.
    Jaroenjittichai, P.
    Natl Astron Res Inst Thailand, Thailand.
    Johnston, S.
    Australia Telescope Natl Facil, Australia.
    Kasliwal, M.
    CALTECH, USA.
    Kramer, M.
    Max Planck Inst Radioastron, Germany.
    Littlefair, S. P.
    Univ Sheffield, UK.
    Macquart, J. P.
    Curtin Univ, Australia.
    Mickaliger, M.
    Univ Manchester, UK.
    Possenti, A.
    INAF Osservatorio Astron Cagliari, Italy.
    Pritchard, T.
    Swinburne Univ Technol, Australia.
    Ravi, V.
    CALTECH, USA.
    Rest, A.
    Space Telescope Sci Inst, USA.
    Rowlinson, A.
    Netherlands Inst Radio Astron, Netherlands.
    Sawangwit, U.
    Natl Astron Res Inst Thailand, Thailand.
    Stappers, B.
    Univ Manchester, UK.
    Sullivan, M.
    Univ Southampton, UK.
    Tiburzi, C.
    Univ Bielefeld, Germany.
    van Straten, W.
    Swinburne Univ Technol, Australia.
    Albert, A.
    Univ Haute Alsace, France.
    Andre, M.
    Tech Univ Catalonia, Spain.
    Anghinolfi, M.
    Ist Nazl Fis Nucl, Sez Genova, Italy.
    Anton, G.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Ardid, M.
    Univ Politecn Valencia, Spain.
    Aubert, J. -J
    Aix-Marseille Université, France.
    Avgitas, T.
    Univ Paris Diderot, France.
    Baret, B.
    Univ Paris Diderot, France.
    Barrios-Marti, J.
    Univ Valencia, Spain.
    Basa, S.
    Pole Etoile Site Chateau Gombert, France.
    Bertin, V.
    Aix Marseille Univ, France.
    Biagi, S.
    Ist Nazl Fis Nucl, Italy.
    Borrnuth, R.
    Nikhef, Netherlands.
    Bourret, S.
    Univ Paris Diderot, France.
    Bouwhuis, M. C.
    Nikhef, Netherlands.
    Bruijn, R.
    Univ Amsterdam, Netherlands.
    Brunner, J.
    Aix Marseille Univ, France.
    Busto, J.
    Aix Marseille Univ, France.
    Capone, A.
    Ist Nazl Fis Nucl, Italy.
    Caramete, L.
    Inst Space Sci, Romania.
    Carr, J.
    Aix Marseille Univ, France.
    Celli, S.
    Ist Nazl Fis Nucl, Sez Roma, Italy.
    Chiarusi, T.
    Ist Nazl Fis Nucl, Italy.
    Circella, M.
    Ist Nazl Fis Nucl, Italy.
    Coelho, J. A. B.
    Univ Paris Diderot, France.
    Coleiro, A.
    Univ Paris Diderot, France.
    Coniglione, R.
    Ist Nazl Fis Nucl, Italy.
    Costantini, H.
    Aix Marseille Univ, France.
    Coyle, P.
    Aix Marseille Univ, France.
    Creusot, A.
    Univ Paris Diderot, France.
    Deschamps, A.
    UCA, France.
    De Bonis, G.
    Ist Nazl Fis Nucl, Italy.
    Distefano, C.
    Ist Nazl Fis Nucl, Italy.
    Di Palma, I.
    Ist Nazl Fis Nucl, Italy.
    Donzaud, C.
    Univ Paris Diderot, France.
    Dornic, D.
    Aix Marseille Univ, France.
    Drouhin, D.
    Univ Haute Alsace, France.
    Eberl, T.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    El Bojaddaini, I.
    Univ Mohammed 1, Morocco.
    Elsasser, D.
    Univ Wurzburg, Germany.
    Enzenhofer, A.
    Aix Marseille Univ, France.
    Felis, I.
    Univ Politecn Valencia, Spain.
    Fusco, L. A.
    Ist Nazl Fis Nucl, Italy.
    Galata, S.
    Univ Paris Diderot, France.
    Gay, P.
    Univ Paris Diderot, France.
    Geisselsoder, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Geyer, K.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Giordano, V.
    Ist Nazl Fis Nucl, Italy.
    Gleixner, A.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Glotin, H.
    Aix Marseille Univ, France.
    Gregoire, T.
    Univ Paris Diderot, France.
    Gracia-Ruiz, R.
    Univ Paris Diderot, France.
    Graf, K.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Hallmann, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    van Haren, H.
    Royal Netherlands Inst Sea Res NIOZ, Netherlands.
    Heijboer, A. J.
    Nikhef, Netherlands.
    Hello, Y.
    UCA, France.
    Hernandez-Rey, J. J.
    Univ Paris Diderot, France.
    Hossl, J.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Hofestadt, J.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Hugon, C.
    Ist Nazl Fis Nucl, Italy.
    Illuminati, G.
    Univ Valencia, Spain.
    James, C. W. C. W.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    de Jong, M.
    Nikhef, Netherlands.
    Jongen, M.
    Nikhef, Netherlands.
    Kadler, M.
    Univ Wurzburg, Germany.
    Kalekin, O.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Katz, U.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Kiessling, D.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Kouchner, A.
    Univ Paris Diderot, France.
    Kreter, M.
    Univ Wurzburg, Germany.
    Kreykenbohm, I.
    Univ Erlangen Nurnberg, Germany.
    Kulikovskiy, V.
    Aix Marseille Univ, France.
    Lachaud, C.
    Univ Paris Diderot, France.
    Lahmann, R.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Lefevre, D.
    Aix Marseille Univ, France.
    Leonora, E.
    Ist Nazl Fis Nucl, Italy.
    Lotze, M.
    Univ Valencia, Spain.
    Loucatos, S.
    Univ Paris Diderot, France.
    Marcelin, M.
    Pole Etoile Site Chateau Gombert, France.
    Margiotta, A.
    Ist Nazl Fis Nucl, Italy.
    Marinelli, A.
    Ist Nazl Fis Nucl, Italy.
    Martinez-Mora, J. A.
    Univ Politecn Valencia, Spain.
    Mathieu, A.
    Aix Marseille Univ, France.
    Mele, R.
    Ist Nazl Fis Nucl, Italy.
    Melis, K.
    Univ Amsterdam, Netherlands.
    Michael, T.
    Nikhef, Netherlands.
    Migliozzi, P.
    Ist Nazl Fis Nucl, Italy.
    Moussa, A.
    Univ Mohammed 1, Morocco.
    Mueller, C.
    Univ Wurzburg, Germany.
    Nezri, E.
    Pole Etoile Site Chateau Gombert, France.
    Pavalas, G. E.
    Inst Space Sci, Romania.
    Pellegrino, C.
    Ist Nazl Fis Nucl, Italy.
    Perrina, C.
    Ist Nazl Fis Nucl, Italy.
    Piattelli, P.
    Ist Nazl Fis Nucl, Italy.
    Popa, V.
    Inst Space Sci, Romania.
    Pradier, T.
    Univ Strasbourg, France.
    Quinn, L.
    Aix Marseille Univ, France.
    Racca, C.
    Univ Haute Alsace, France.
    Riccobene, G.
    Ist Nazl Fis Nucl, Italy.
    Roensch, K.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Sanchez-Losa, A.
    Ist Nazl Fis Nucl, Italy.
    Saldana, M.
    Univ Politecn Valencia, Spain.
    Salvadori, I.
    Aix Marseille Univ, France.
    Samtleben, D. F. E.
    Nikhef, Sci Pk, Netherlands.
    Sanguineti, M.
    Ist Nazl Fis Nucl, Italy.
    Sapienza, P.
    Ist Nazl Fis Nucl, Italy.
    Schnabel, J.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Seitz, T.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Sieger, C.
    Friedrich Alexander Univ Erlangen Nurnberg,Germany.
    Spurio, M.
    Ist Nazl Fis Nucl, Italy.
    Stolarczyk, Th.
    CEA Saclay, France.
    Taiuti, M.
    Ist Nazl Fis Nucl, Italy.
    Tayalati, Y.
    Univ Mohammed Rabat, Morocco.
    Trovato, A.
    Ist Nazl Fis Nucl, Italy.
    Tselengidou, M.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Turpin, D.
    Aix Marseille Univ, France.
    Tonnis, C.
    Univ Valencia, Spain.
    Vallage, B.
    Univ Paris Diderot, France.
    Vallee, C.
    Aix Marseille Univ, France.
    Van Elewyck, V.
    Univ Paris Diderot, France.
    Vivolo, D.
    Ist Nazl Fis Nucl, Italy.
    Vizzoca, A.
    Ist Nazl Fis Nucl, Italy.
    Wagner, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Wilms, J.
    Univ Erlangen Nurnberg, Germany.
    Zornoza, J. D.
    Univ Valencia, Spain.
    Zuniga, J.
    Univ Valencia, Spain.
    Abdalla, H.
    North West Univ, South Africa.
    Abramowski, A.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Aharonian, F.
    Max Planck Inst Kernphys, Germany.
    Benkhali, F. Ait
    Max Planck Inst Kernphys, Germany.
    Akhperjanian, A. G.
    Natl Acad Sci Republ Armenia, Armenia.
    Andersson, Tom
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Anguner, E. O.
    Humboldt Univ, Germany.
    Arrieta, M.
    Univ Paris Diderot, France.
    Aubert, P.
    Univ Savoie Mt Blanc, France.
    Backes, M.
    Univ Namibia, Namibia.
    Balzer, A.
    Univ Amsterdam, Netherlands.
    Barnard, M.
    North West Univ, South Africa.
    Becherini, Yvonne
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Tjus, J. Becker
    Ruhr Univ Bochum, Germany.
    Berge, D.
    Univ Amsterdam, Netherlands.
    Bernhard, S.
    Leopold Franzens Univ Innsbruck, Austria.
    Bernlohr, K.
    Max Planck Inst Kernphys, Germany.
    Blackwell, R.
    Univ Adelaide, Australia.
    Bottcher, M.
    North West Univ, South Africa.
    Boisson, C.
    Univ Paris Diderot, France.
    Bolmont, J.
    Univ Paris Diderot, France.
    Bordas, P.
    Max Planck Inst Kernphys, Germany.
    Bregeon, J.
    Univ Montpellier, France.
    Brun, F.
    Univ Bordeaux, France.
    Brun, P.
    CEA Saclay, France.
    Bryan, M.
    Univ Amsterdam, Netherlands.
    Bulik, T.
    Univ Warsaw, Poland.
    Capasso, M.
    Univ Tubingen, Germany.
    Casanova, S.
    Max Planck Inst Kernphys, Germany.
    Cerruti, M.
    Univ Paris Diderot, France.
    Chakraborty, N.
    Max Planck Inst Kernphys, Germany.
    Chalme-Calvet, R.
    Univ Paris Diderot, France.
    Chaves, R. C. G.
    Univ Montpellier, France.
    Chen, A.
    Univ Witwatersrand, South Africa.
    Chevalier, J.
    Univ Savoie Mt Blanc, France.
    Chretien, M.
    Univ Paris Diderot, France.
    Colafrancesco, S.
    Univ Witwatersrand, South Africa.
    Cologna, G.
    Heidelberg Univ, Germany.
    Condon, B.
    Univ Bordeaux, France.
    Conrad, J.
    Stockholm Universiyt, Sweden.
    Cui, Y.
    Univ Tubingen, Germany.
    Davids, I. D.
    North West Univ, South Africa.
    Decock, J.
    CEA Saclay, France.
    Degrange, B.
    Univ Grenoble Alpes, France.
    Deil, C.
    Max Planck Inst Kernphys, Germany.
    Devin, J.
    Univ Montpellier, France.
    de Wilt, P.
    Univ Adelaide, Australia.
    Dirson, L.
    Univ Hamburg, Germany.
    Djannati-Atai, A.
    Univ Paris Diderot, France.
    Domainko, W.
    Max Planck Inst Kernphys, Germany.
    Donath, A.
    Max Planck Inst Kernphys, Germany.
    Drury, L. O 'C.
    Dublin Institute for Advanced Studies, Ireland.
    Dubus, G.
    Univ Grenoble Alpes, France.
    Dutson, K.
    Univ Leicester, UK.
    Dyks, J.
    Nicolaus Copernicus Astron Ctr, Poland.
    Edwards, T.
    Max Planck Inst Kernphys, Germany.
    Egberts, K.
    Univ Potsdam, Germany.
    Eger, P.
    Max Planck Inst Kernphys, Germany.
    Ernenwein, J. -P
    Aix-Marseille Université, France.
    Eschbach, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Farnier, Christian
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Stockholm University, Sweden.
    Fegan, S.
    Ecole Polytech, France.
    Fernandes, M. V.
    Univ Hamburg, Germany.
    Fiasson, A.
    Univ Savoie Mt Blanc, France.
    Fontaine, G.
    Ecole Polytech, France.
    Forster, A.
    Max Planck Inst Kernphys, Germany.
    Funk, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Fussling, M.
    DESY, Germany.
    Gabici, S.
    Univ Paris Diderot, France.
    Gajdus, M.
    Humboldt Univ, Germany.
    Gallant, Y. A.
    Univ Montpellier, France.
    Garrigoux, T.
    North West Univ, South Africa.
    Giavitto, G.
    DESY, Germany.
    Giebels, B.
    Ecole Polytech, France.
    Glicenstein, J. F.
    CEA Saclay, France.
    Gottschall, D.
    Univ Tubingen, Germany.
    Goya, A.
    Uniwersytet Jagiellonski, Poland.
    Grondin, M. -H
    Université Bordeaux, France.
    Hadasch, D.
    Leopold Franzens Univ Innsbruck, Austria.
    Hahn, J.
    Max Planck Inst Kernphys, Germany.
    Haupt, M.
    DESY, Germany.
    Hawkes, J.
    Univ Adelaide, Australia.
    Heinzelmann, G.
    Univ Hamburg, Germany.
    Henri, G.
    Univ Grenoble Alpes, France.
    Hermann, G.
    Max Planck Inst Kernphys, Germany.
    Hervet, O.
    Univ Paris Diderot, France.
    Hinton, J. A.
    Max Planck Inst Kernphys, Germany.
    Hofmann, W.
    Max Planck Inst Kernphys, Germany.
    Hoischen, C.
    Univ Potsdam, Germany.
    Holler, M.
    Ecole Polytech, France.
    Horns, D.
    Univ Hamburg, Germany.
    Ivascenko, A.
    North West Univ, South Africa.
    Jacholkowska, A.
    Univ Paris Diderot, France.
    Jamrozy, M.
    Uniwersytet Jagiellonski, Poland.
    Janiak, M.
    Nicolaus Copernicus Astron Ctr, Poland.
    Jankowsky, D.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Jankowsky, F.
    Heidelberg Univ, Germany.
    Jingo, M.
    Univ Witwatersrand, South Africa.
    Jogler, T.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Jouvin, L.
    Univ Paris Diderot, France.
    Jung-Richardt, I.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Kastendieck, M. A.
    Univ Hamburg, Germany.
    Katarzynski, K.
    Nicolaus Copernicus Univ, Poland.
    Kerszberg, D.
    Univ Paris Diderot, France.
    Khelifi, B.
    Univ Paris Diderot, France.
    Kieffer, M.
    Univ Paris Diderot, France.
    King, J.
    Max Planck Inst Kernphys, Germany.
    Klepser, S.
    Uniwersytet Jagiellonski, Poland.
    Klochkov, D.
    Univ Tubingen, Germany.
    Kluzniak, W.
    Nicolaus Copernicus Astron Ctr, Poland.
    Kolitzus, D.
    Leopold Franzens Univ Innsbruck, Austria.
    Komin, Nu.
    Heidelberg Univ, Germany.
    Kosack, K.
    CEA Saclay, France.
    Krakau, S.
    Ruhr Univ Bochum, Germany.
    Kraus, M.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Krayzel, F.
    Univ Savoie Mt Blanc, France.
    Kruger, P. P.
    North West Univ, South Africa.
    Laffon, H.
    Univ Bordeaux, France.
    Lamanna, G.
    Univ Savoie Mt Blanc, France.
    Lau, J.
    Univ Adelaide, Australia.
    Lees, J. -P
    Université Savoie Mont-Blanc, France.
    Lefaucheur, J.
    Univ Paris Diderot, France.
    Lefranc, V.
    CEA Saclay, France.
    Lemiere, A.
    Univ Paris Diderot, France.
    Lemoine-Goumard, M.
    Univ Bordeaux, France.
    Lenain, J. -P
    Sorbonne Universités, France.
    Leser, E.
    Univ Potsdam, Germany.
    Lohse, T.
    Humboldt Univ, Germany.
    Lorentz, M.
    CEA Saclay, France.
    Liu, R.
    Max Planck Inst Kernphys, Germany.
    Lopez-Coto, R.
    Max Planck Inst Kernphys, Germany.
    Lypova, I.
    DESY, Germany.
    Marandon, V.
    Max Planck Inst Kernphys, Germany.
    Marcowith, A.
    Univ Montpellier, France.
    Mariaud, C.
    Ecole Polytech, France.
    Marx, R.
    Max Planck Inst Kernphys, Germany.
    Maurin, G.
    Univ Savoie Mt Blanc, France.
    Maxted, N.
    Univ Adelaide, Australia.
    Mayer, M.
    Humboldt Univ, Germany.
    Meintjes, P. J.
    Univ Free State, South Africa.
    Meyer, M.
    Stockholm University, Sweden.
    Mitchell, A. M. W.
    Max Planck Inst Kernphys, Germany.
    Moderski, R.
    Nicolaus Copernicus Astron Ctr, Poland.
    Mohamed, M.
    Heidelberg Univ, Germany.
    Mohrmann, L.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Mora, K.
    Stockholm University, Sweden.
    Moulin, E.
    CEA Saclay, France.
    Murach, T.
    Humboldt Univ, Germany.
    de Naurois, M.
    Ecole Polytech, France.
    Niederwanger, F.
    Leopold Franzens Univ Innsbruck, Austria.
    Niemiec, J.
    Inst Fizyki Jadrowej PAN, Poland.
    Oakes, L.
    Humboldt Univ, Germany.
    O'Brien, P.
    Univ Leicester, UK.
    Odaka, H.
    Max Planck Inst Kernphys, Germany.
    Ottl, S.
    Leopold Franzens Univ Innsbruck, Austria.
    Ohm, S.
    DESY, Germany.
    Ostrowski, M.
    Uniwersytet Jagiellonski, Poland.
    Oya, I.
    DESY, Germany.
    Padovani, M.
    Univ Montpellier, France.
    Panter, M.
    Max Planck Inst Kernphys, Germany.
    Parsons, R. D.
    Max Planck Inst Kernphys, Germany.
    Pekeur, N. W.
    North West Univ, South Africa.
    Pelletier, G.
    Univ Grenoble Alpes, France.
    Perennes, C.
    Univ Paris Diderot, France.
    Petrucci, P. -O
    Univ. Grenoble Alpes, France.
    Peyaud, B.
    CEA Saclay, France.
    Piel, Q.
    Univ Savoie Mt Blanc, France.
    Pita, S.
    Univ Paris Diderot, France.
    Poon, H.
    Max Planck Inst Kernphys, Germany.
    Prokhorov, Dmitry
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Prokoph, Heike
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Puhlhofer, G.
    Univ Tubingen, Germany.
    Punch, Michael
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Univ Paris Diderot, France.
    Quirrenbach, A.
    Heidelberg Univ, Germany.
    Raab, S.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Reimer, A.
    Leopold Franzens Univ Innsbruck, Austria.
    Reimer, O.
    Leopold Franzens Univ Innsbruck, Austria.
    Renaud, M.
    Univ Montpellier, France.
    de los Reyes, R.
    Max Planck Inst Kernphys, Germany.
    Rieger, F.
    Max Planck Inst Kernphys, Germany.
    Romoli, C.
    Dublin Inst Adv Studies, Ireland.
    Rosier-Lees, S.
    Univ Savoie Mt Blanc, France.
    Rowell, G.
    Univ Adelaide, Australia.
    Rudak, B.
    Nicolaus Copernicus Astron Ctr, Poland.
    Rulten, C. B.
    Univ Paris Diderot, France.
    Sahakian, V.
    Natl Acad Sci Republ Armenia, Armenia.
    Salek, D.
    Univ Amsterdam, Netherlands.
    Sanchez, D. A.
    Univ Savoie Mt Blanc, France.
    Santangelo, A.
    Univ Tubingen, Germany.
    Sasaki, M.
    Univ Tubingen, Germany.
    Schlickeiser, R.
    Ruhr Univ Bochum, Germany.
    Schulz, A.
    DESY, Germany.
    Schussler, F.
    Ist Nazl Fis Nucl, Italy.
    Schwanke, U.
    Humboldt Univ, Germany.
    Schwemmer, S.
    Heidelberg Univ, Germany.
    Settimo, M.
    Univ Paris Diderot, France.
    Seyffert, A. S.
    North West Univ, South Africa.
    Shafi, N.
    Univ Witwatersrand, South Africa.
    Shilon, I.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Simoni, R.
    Univ Amsterdam, Netherlands.
    Sol, H.
    Univ Paris Diderot, France.
    Spanier, F.
    North West Univ, South Africa.
    Spengler, G.
    Stockholm University, Sweden.
    Spies, F.
    Univ Hamburg, Germany.
    Stawarz, L.
    Uniwersytet Jagiellonski, Poland.
    Steenkamp, R.
    Univ Namibia, Namibia.
    Stegmann, C.
    Univ Potsdam, Germany.
    Stinzing, F.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Stycz, K.
    DESY, Germany.
    Sushch, I.
    North West Univ, South Africa.
    Tavernet, J. -P
    Sorbonne Universités, France.
    Tavernier, T.
    Univ Paris Diderot, France.
    Taylor, A. M.
    Dublin Inst Adv Studies, Ireland.
    Terrier, R.
    Univ Paris Diderot, France.
    Tibaldo, L.
    Max Planck Inst Kernphys, Germany.
    Tiziani, D.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Tluczykont, M.
    Univ Hamburg, Germany.
    Trichard, C.
    Aix Marseille Univ, France.
    Tuffs, R.
    Max Planck Inst Kernphys, Germany.
    Uchiyama, Y.
    Rikkyo Univ, Japan.
    van der Walt, D. J.
    North West Univ, South Africa.
    van Eldik, C.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    van Rensburg, C.
    North West Univ, South Africa.
    van Soelen, B.
    Univ Free State, South Africa.
    Vasileiadis, G.
    Univ Montpellier, France.
    Veh, J.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Venter, C.
    North West Univ, South Africa.
    Viana, A.
    Max Planck Inst Kernphys, Germany.
    Vincent, P.
    Univ Paris Diderot, France.
    Vink, J.
    Univ Amsterdam, Netherlands.
    Voisin, F.
    Univ Adelaide, Australia.
    Volk, H. J.
    Max Planck Inst Kernphys, Germany.
    Vuillaume, T.
    Univ Savoie Mt Blanc, France.
    Wadiasingh, Z.
    North West Univ, South Africa.
    Wagner, S. J.
    Heidelberg Univ, Germany.
    Wagner, P.
    Humboldt Univ, Germany.
    Wagner, R. M.
    Stockholm University, Sweden.
    White, R.
    Max Planck Inst Kernphys, Germany.
    Wierzcholska, A.
    Inst Fizyki Jadrowej PAN, Poland.
    Willmann, P.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Wornlein, A.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Wouters, D.
    CEA Saclay, France.
    Yang, R.
    Max Planck Inst Kernphys, Germany.
    Zabalza, V.
    Univ Leicester, UK.
    Zaborov, D.
    Univ Grenoble Alpes, France.
    Zacharias, M.
    Stockholm University, Sweden.
    Zanin, R.
    Max Planck Inst Kernphys, Germany.
    Zdziarski, A. A.
    Nicolaus Copernicus Astron Ctr, Poland.
    Zech, A.
    Univ Paris Diderot, France.
    Zefi, F.
    Ecole Polytech, France.
    Ziegler, A.
    Friedrich Alexander Univ Erlangen Nurnberg, Germany.
    Zywucka, N.
    Uniwersytet Jagiellonski, Poland.
    A polarized fast radio burst at low Galactic latitude2017Ingår i: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 469, nr 4, s. 4465-4482Artikel i tidskrift (Refereegranskat)
    Abstract [en]

    We report on the discovery of a new fast radio burst (FRB), FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure (DM) of 1105.6 +/- 0.8 pc cm(-3), a pulse duration of 2.8(-0.5)(+1.2) ms, and a measured peak flux density assuming that the burst was at beam centre of 0.7(-0.1)(+0.2) Jy. The FRB originated at a Galactic longitude and latitude of 24.66 degrees, 5.28 degrees and 25 degrees away from the Galactic Center. The burst was found to be 43 +/- 5 per cent linearly polarized with a rotation measure (RM) in the range -9 < RM < 12 rad m(-2) (95 per cent confidence level), consistent with zero. The burst was followed up with 11 telescopes to search for radio, optical, X-ray, gamma-ray and neutrino emission. Neither transient nor variable emission was found to be associated with the burst and no repeat pulses have been observed in 17.25 h of observing. The sightline to the burst is close to the Galactic plane and the observed physical properties of FRB 150215 demonstrate the existence of sight lines of anomalously low RM for a given electron column density. The Galactic RM foreground may approach a null value due to magnetic field reversals along the line of sight, a decreased total electron column density from the Milky Way, or some combination of these effects. A lower Galactic DM contribution might explain why this burst was detectable whereas previous searches at low latitude have had lower detection rates than those out of the plane.

  • 202. Pita, S.
    et al.
    Goldoni, P.
    Boisson, C.
    Becherini, Yvonne
    Gerard, L.
    Lenain, J. -P
    Punch, Michael
    High energy blazars spectroscopy with X-Shooter on the VLT2012Ingår i: High energy gamma-ray astronomy, American Institute of Physics (AIP), 2012, s. 566-569Konferensbidrag (Refereegranskat)
    Abstract [en]

    We present results of observations in the UV to near-IR range for eight blazars, three of which have been recently discovered at Very High Energies (VHE) and five appearing as interesting candidates for VHE gamma-ray detection. We focus in this paper on the search for their redshifts, which are unknown or considered as uncertain.

  • 203.
    Prokoph, Heike
    et al.
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Becherini, Yvonne
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Böttcher, M.
    North-West University, South Africa.
    Boisson, C.
    Université Paris Diderot, France.
    Lenain, J.-P.
    Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, France.
    Sushch, I.
    North-West University, South Africa.
    Collaboration, for the H. E. S. S.
    H.E.S.S. discovery of very-high-energy gamma-ray emission of PKS 1440-3892015Ingår i: Proceedings of Science, SISSA , 2015Konferensbidrag (Övrigt vetenskapligt)
    Abstract [en]

    Blazars are the most abundant class of known extragalactic very-high-energy (VHE, E>100 GeV) gamma-ray sources. However, one of the biggest difficulties in investigating their VHE emission resides in their limited number, since less than 60 of them are known by now. In this contribution we report on H.E.S.S. observations of the BL Lac object PKS 1440-389. This source has been selected as target for H.E.S.S. based on its high-energy gamma-ray properties measured by Fermi-LAT. The extrapolation of this bright, hard-spectrum gamma-ray blazar into the VHE regime made a detection on a relatively short time scale very likely, despite its uncertain redshift. H.E.S.S. observations were carried out with the 4-telescope array from February to May 2012 and resulted in a clear detection of the source. Contemporaneous multi-wavelength data are used to construct the spectral energy distribution of PKS 1440-389 which can be described by a simple one-zone synchrotron-self Compton model

  • 204.
    Punch, M.
    et al.
    Univ Paris Cite, France.
    Senniappan, Mohanraj
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Becherini, Yvonne
    Univ Paris Cite, France.
    Kukec Mezek, Gasper
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Thoudam, S.
    Khalifa Univ, United Arab Emirates.
    Bylund, Tomas
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Ernenwein, J. -P
    Aix Marseille Univ, France.
    Sensitivity to point-like sources of the ALTO atmospheric particle detector array, designed for 200GeV-50TeV gamma-ray astronomy2023Ingår i: Journal of High Energy Astrophysics, ISSN 2214-4048, E-ISSN 2214-4056, Vol. 39, s. 1-13Artikel i tidskrift (Refereegranskat)
    Abstract [en]

    In the context of atmospheric shower arrays designed for gamma-ray astronomy and in the context of the ALTO project, we present: a study of the impact of heavier nuclei in the cosmic-ray background on the estimated gamma-ray detection performance on the basis of dedicated Monte Carlo simulations, a method to calculate the sensitivity to a point-like source, and finally the required observation times to reach a firm detection on a list of known point-like sources.

  • 205. Raue, M.
    et al.
    Lenain, J. -P
    Aharonian, F. A.
    Becherini, Yvonne
    Boisson, C.
    Clapson, A. -C
    Costamante, L.
    Gerard, L.
    Medina, C.
    de Naurois, M.
    Punch, M.
    Univ Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
    Rieger, F.
    So, H.
    Stawarz, L.
    Zech, A.
    Discovery of VHE gamma-rays from Centaurus A2010Ingår i: Accretion and Ejection in AGN: a Global View / [ed] Maraschi, L; Ghisellini, G; DellaCeca, R; Tavecchio, F, Astronomical Society of the Pacific , 2010, Vol. 427, s. 302-303Konferensbidrag (Övrigt vetenskapligt)
    Abstract [en]

    Centaurus A is the closest active radio galaxy. Its proximity enables unique studies of the processes in relativistic jets and near supermassive black holes. Centaurus A has been intensively studied in many wavelength bands and has also been discussed as a possible site for UHECR acceleration. Here, we report the discovery of weak very-high energy gamma-ray emission from Centaurus A with the H.E.S.S. Cherenkov telescope array. The discovery of Centaurus A, together with the detection of M 87, establishes radio galaxies - i.e. AGNs with only weak relativistic beaming - as sources of VHE gamma-rays. The implications of these results on the emission site and on the different models available will be discussed.

  • 206.
    Senniappan, Mohanraj
    et al.
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Becherini, Yvonne
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Punch, Michael
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Univ Paris, France.
    Thoudam, Satyendra
    Khalifa University, United Arab Emirates.
    Bylund, Tomas
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Kukec Mezek, Gasper
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Ernenwein, Jean-Pierre
    Aix Marseille Univ, France.
    Expected performance of the ALTO particle detector array designed for 200 GeV - 50 TeV gamma-ray astronomy2022Ingår i: Proceedings of Science: 37th International Cosmic Ray Conference (ICRC 2021), July 12th – 23rd, 2021 Online – Berlin, German, Scuola Internazionale Superiore di Studi Avanzati (SISSA) , 2022, Vol. 395, artikel-id 761Konferensbidrag (Refereegranskat)
    Abstract [en]

    The ALTO project aims to build a particle detector array for very high energy gamma ray observations optimized for soft spectrum sources. The accurate reconstruction of gamma ray events, in particular their energies, using a surface array is an especially challenging problem at the low energies ALTO aims to optimize for. In this contribution, we leverage Convolutional Neural Networks (CNNs) to improve reconstruction performance at lower energies ( smaller 1 TeV ) as compared to the SEMLA analysis procedure, which is a more traditional method using mainly manually derived features.rnWe present performance figures using different network architectures and training settings, both in terms of accuracy and training time, as well as the impact of various data augmentation techniques.

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  • 207.
    Senniappan, Mohanraj
    et al.
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Becherini, Yvonne
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Punch, Michael
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Université de Paris, France.
    Thoudam, Satyendra
    Khalifa University, United Arab Emirates.
    Bylund, Tomas
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Kukec Mezek, Gasper
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Ernenwein, J.-P.
    Aix Marseille Université, France.
    Signal extraction in atmospheric shower arrays designed for 200 GeV–50 TeV γ-ray astronomy2021Ingår i: Journal of Instrumentation, ISSN 1748-0221, E-ISSN 1748-0221, Vol. 16, nr 07, artikel-id P07050Artikel i tidskrift (Refereegranskat)
    Abstract [en]

    We present the SEMLA (Signal Extraction using Machine Learning for ALTO) analysis method, developed for the detection of E>200 GeV γ rays in the context of the ALTO wide-field-of-view atmospheric shower array R&D project. The scientific focus of ALTO is extragalactic γ-ray astronomy, so primarily the detection of soft-spectrum γ-ray sources such as Active Galactic Nuclei and Gamma Ray Bursts. The current phase of the ALTO R&D project is the optimization of sensitivity for such sources and includes a number of ideas which are tested and evaluated through the analysis of dedicated Monte Carlo simulations and hardware testing. In this context, it is important to clarify how data are analysed and how results are being obtained. SEMLA takes advantage of machine learning and comprises four stages: initial event cleaning (stage A), filtering out of poorly reconstructed γ-ray events (stage B), followed by γ-ray signal extraction from proton background events (stage C) and finally reconstructing the energy of the events (stage D). The performance achieved through SEMLA is evaluated in terms of the angular, shower core position, and energy resolution, together with the effective detection area, and background suppression. Our methodology can be easily generalized to any experiment, provided that the signal extraction variables for the specific analysis project are considered.

  • 208. Stamatescu, V.
    et al.
    Becherini, Yvonne
    APC Paris.
    Bernloehr, K.
    Carmona, E.
    Colin, P.
    Farnier, C.
    Gerard, L.
    Hinton, J. A.
    Khelifi, B.
    Komin, N.
    Lamanna, G.
    Lenain, J. -P
    Maier, G.
    Moralejo, A.
    Naumann, C. L.
    Parsons, D.
    Di Pierro, F.
    Prokoph, Heike
    Vorobiov, S.
    Towards an optimized design for the Cherenkov Telescope Array2012Ingår i: HIGH ENERGY GAMMA-RAY ASTRONOMY, American Institute of Physics (AIP), 2012, s. 758-761Konferensbidrag (Refereegranskat)
    Abstract [en]

    The Cherenkov Telescope Array (CTA) is a future instrument for very-high-energy (VHE) gamma-ray astronomy that is expected to deliver an order of magnitude improvement in sensitivity over existing instruments. In order to meet the physics goals of CTA in a cost-effective way, Monte Carlo simulations of the telescope array are used in its design. Specifically, we simulate large arrays comprising numerous large-size, medium-size and small-size telescopes whose configuration parameters are chosen based on current technical design studies and understanding of the costs involved. Subset candidate arrays with various layout configurations are then selected and evaluated in terms of key performance parameters, such as the sensitivity. This is carried out using a number of data analysis methods, some of which were developed within the field and extended to CTA, while others were developed specifically for this purpose. We outline some key results from recent studies that illustrate our approach to the optimization of the CTA design.

  • 209.
    Thoudam, Satyendra
    et al.
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Becherini, Yvonne
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Punch, Michael
    Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE).
    Simulation study for the proposed wide field-of-view gamma-ray detector array ALTO2018Ingår i: Proceedings of Science: 35th International Cosmic Ray Conference, ICRC 2017, 10 -20 July 2017, Bexico, South Korea, Sissa Medialab Srl , 2018Konferensbidrag (Refereegranskat)
    Abstract [en]

    ALTO is a wide field-of-view air shower detector array for very-high-energy (VHE) gamma-ray astronomy, proposed to be installed in the Southern Hemisphere at an altitude of ∼5.1 km above sea level. The array will use water Cherenkov detectors, as in the HAWC observatory, but combined with scintillator detectors, to detect air showers induced by VHE gamma rays in the atmosphere. It is being designed to attain a lower energy threshold, better energy and angular resolution, and improved sensitivity. The array will consist of ∼1250 small-sized (3.6 m diameter) detector units distributed over a circular area of ∼160 m in diameter. Each detector unit will consist of a water Cherenkov detector and a liquid scintillation detector underneath which will preferentially identify muons, facilitating the background (cosmic ray) rejection, thereby improving the sensitivity. The background rejection will be further enhanced by the close-packed arrangement and the small size of the detectors which will allow a fine sampling of air-shower footprints at the ground. In this contribution, we present the Monte-Carlo simulation of the experiment performed using CORSIKA and GEANT4 simulation packages. The expected performance of the array in terms of reconstruction accuracies of the shower core and arrival direction, as well as preliminary estimate of the trigger energy threshold after preliminary selection cuts for a point-like gamma-ray source are presented. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).

  • 210. Togo, V
    et al.
    Ambrosio, M
    Antolini, R
    Auriemma, G
    Bakari, D
    Baldini, A
    Barbarino, G C
    Barish, B C
    Battistoni, G
    Becherini, Yvonne
    Bellotti, R
    Bemporad, C
    Bernardini, P
    Bilokon, H
    Bloise, C
    Bower, C
    Brigida, M
    Bussino, S
    Cafagna, F
    Campana, D
    Carboni, M
    Caruso, R
    Cecchini, S
    Cei, F
    Chiarella, V
    Chiarusi, T
    Choudhary, B C
    Coutu, S
    Cozzi, M
    De Cataldo, G
    Dekhissi, H
    De Marzo, C
    Erriquez, O
    Favuzzi, C
    Forti, C
    Fusco, P
    Giacomelli, G
    Giannini, G
    Giglietto, N
    Giorgini, M
    Grassi, M
    Grillo, A
    Guarino, F
    Gustavino, C
    Habig, A
    Hanson, K
    Heinz, R
    Iarocci, E
    Katsavounidis, E
    Katsavounidis, I
    Kearns, E
    Kim, H
    Kyriazopoulou, S
    Kumar, A
    Lamanna, E
    Lane, C
    Levin, D S
    Lipari, P
    Longo, M J
    Loparco, F
    Maaroufi, F
    Mancarella, G
    Mandrioli, G
    Manzoor, S
    Margiotta, A
    Marini, A
    Martello, D
    Marzari-Chiesa, A
    Matteuzzi, D
    Michael, D G
    Monacelli, P
    Montaruli, T
    Monteno, M
    Mufson, S
    Musser, J
    Nicolo, D
    Nolty, R
    Orth, C
    Osteria, G
    Palamara, O
    Patera, V
    Patrizii, L
    Pazzi, R
    Peck, C W
    Perrone, L
    Petrera, S
    Pistilli, P
    Popa, V
    Raino, A
    Reynoldson, J
    Ronga, F
    Rrhioua, A
    Satriano, C
    Scapparone, E
    Scholberg, K
    Sciubba, A
    Serra, P
    Sioli, M
    Sirri, G
    Sitta, M
    Spinelli, P
    Spinetti, M
    Spurio, M
    Steinberg, R
    Stone, J L
    Sulak, L R
    Surdo, A
    G, Tarle
    Vakili, M
    Walter, C W
    Webb, R
    Calibrations of CR39 and Makrofol nuclear track detectors and search for exotic particles2003Ingår i: Nuclear physics B, Proceedings supplements, ISSN 0920-5632, E-ISSN 1873-3832, Vol. 125, s. 217-221Artikel i tidskrift (Refereegranskat)
    Abstract [en]

    We present the final results of the search for exotic massive particles in the cosmic radiation performed with the MACRO underground experiment. Magnetic monopoles and nuclearites flux upper limits obtained with the CR39 nuclear track subdetector, the scintillation and streamer tube subdetectors are given. Searches at high altitude with the SLIM experiment are in progress.

  • 211. Wouters, Denis
    et al.
    Lenain, Jean-Philippe
    Becherini, Yvonne
    University Paris Diderot.
    Harris, Jon
    Brun, Pierre
    Kaufman, Sarah
    Boisson, Catherine
    Cerruti, Matteo
    Sol, Helene
    Zech, Andreas
    H.E.S.S. Observations of the distant BL Lac PKS 0301-2432012Ingår i: HIGH ENERGY GAMMA-RAY ASTRONOMY, American Institute of Physics (AIP), 2012, s. 498-501Konferensbidrag (Refereegranskat)
    Abstract [en]

    PKS 0301-243 is a distant (z=0.266) high-frequency-peaked BL Lac object, detected both at high and very high energies (VHE) with Fermi/LAT and H. E. S. S., and which experienced a flare in May 2010 in the GeV band. H. E. S. S. observations of PKS 0301-243 carried out between September 2009 and December 2011 result in a strong detection of VHE gamma-rays from the source with a significance of 9.8 standard deviations. Multi-wavelength observations from optical to GeV gamma-rays are also presented. The VHE spectrum is used to derive an upper limit on the opacity of the universe to gamma-rays.

2345 201 - 211 av 211
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