Zobrazeno 1 - 2
of 2
pro vyhledávání: '"L. G. Balasz"'
Autor:
R. Bellazini, Andreas Zoglauer, M. I. Panasyuk, René Hudec, L. G. Balasz, R. Marcinkowski, V. M. Lipunov, Mark Pearce, Felix Ryde, Andrei M. Bykov, Elena Pian, D. Hartmann, Guido Barbiellini, Andrew W. Strong, A. Majczyna, Zsolt Bagoly, Sandra Savaglio, J. Kiener, István T. Horváth, B. K. Lubsandorgiev, R. V. Poleschuk, Sheila McBreen, Vincent Tatischeff, Karl Mannheim, G. Wrochna, A. M. Chernenko, Martino Marisaldi, G. Bisnovaty-Kogan, A. Pollo, Attila Mészáros, A. F. Iyudin, A. G. Zabrodskij, J. Uvarov, S. Larsson, W. Dröge, S. E. Boggs, A. M. Cherepashuk, Gottfried Kanbach, Andreas von Kienlin, Norbert Langer, S. I. Svertilov, Dmitry Bisikalo, L. M. Zeleny, G. Dicocco, Jochen Greiner, Werner Collmar, Roland Diehl, B. McBreen, Lorraine Hanlon, Claudio Labanti, Cornelia B. Wunderer, Boris Shustov, E. Orlando, Marco Ajello, M. Gierlik, D. A. Varshalovich, Alexei Pozanenko, G. G. Lichti, L. B. Bezrukov
Publikováno v:
Experimental Astronomy
Experimental Astronomy, springer Link, 2009, 23, pp.91-120. ⟨10.1007/S10686-008-9102-0⟩
Experimental Astronomy, springer Link, 2009, 23, pp.91-120. ⟨10.1007/S10686-008-9102-0⟩
The primary scientific goal of the GRIPS mission is to revolutionize our understanding of the early universe using gamma-ray bursts. We propose a new generation gamma-ray observatory capable of unprecedented spectroscopy over a wide range of gamma-ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7535e42c31652532c8f7d03fea256c7d
http://hdl.handle.net/11368/2948586
http://hdl.handle.net/11368/2948586
Autor:
L. G. Balasz, Jürgen Kiener, Wlodek Klamra, Gennady S. Bisnovatij-Kogan, Asaf Pe'er, Friedrich-Karl Thielemann, Grzegorz Wrochna, Suzanne Foley, Wolfgang Rhode, G. DiCocco, Claes Fransson, Claudio Labanti, Andrzej A. Zdziarski, Georg G. Raffelt, Olaf Reimer, Wolfgang Hillebrandt, Attila Mészáros, Boris Shustov, Elena Pian, Omar Tibolla, Jochen Greiner, Stefan Larsson, Matthias Kadler, Joachim Trümper, Lorraine Hanlon, David Tierney, Jordi José, W. Hermsen, Lucien Kuiper, Radoslaw Marcinkowski, Neil Gehrels, Andrej Bykov, Shawn Bishop, Nikos Prantzos, Sheila McBreen, Roland Diehl, Steven E. Boggs, Felix Ryde, Mark Pearce, Keiichi Maeda, A. F. Iyudin, Martino Marisaldi, Jörn Wilms, Ingo Kreykenbohm, Felix Aharonian, Guido Barbiellini, Ronaldo Bellazzini, Uwe Laux, Nikolaos D. Kylafis, Nial R. Tanvir, G. Kanbach, Ken'ichi Nomoto, Norbert Langer, Christian Schmidt, Marco Ajello, Dominik Elsässer, K. Langanke, K. Mannheim, Andrew W. Strong, Bruno Leibundgut, Andreas Zoglauer, Sylvio Klose, D. A. Varshalovich, B. McBreen, René Hudec, Francesco Longo, Joseph Silk, Dieter H. Hartmann
Publikováno v:
Experimental Astronomy
EXPERIMENTAL ASTRONOMY
Experimental Astronomy, springer Link, 2011, à paraître, ⟨10.1007/S10686-011-9255-0⟩
Experimental Astronomy, 34(2), 551-582. Springer Netherlands
EXPERIMENTAL ASTRONOMY
Experimental Astronomy, springer Link, 2011, à paraître, ⟨10.1007/S10686-011-9255-0⟩
Experimental Astronomy, 34(2), 551-582. Springer Netherlands
We propose to perform a continuously scanning all-sky survey from 200 keV to 80 MeV achieving a sensitivity which is better by a factor of 40 or more compared to the previous missions in this energy range. The Gamma-Ray Imaging, Polarimetry and Spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ef906353db48cc489e31936c4f93abf
