Submitted by Astro-ph Robot on Tue, 02/18/2014 - 20:47
"Detection of bridge emission above 50 GeV from the Crab pulsar with the MAGIC telescopes."J. Aleksić,
S. Ansoldi,
L. A. Antonelli,
P. Antoranz,
A. Babic,
P. Bangale,
U. Barres de Almeida,
J. A. Barrio,
J. Becerra González,
W. Bednarek,
E. Bernardini,
B. Biasuzzi,
A. Biland,
O. Blanch,
S. Bonnefoy,
G. Bonnoli,
F. Borracci,
T. Bretz,
E. Carmona,
A. Carosi,
P. Colin,
E. Colombo,
J. L. Contreras,
J. Cortina,
S. Covino,
P. Da Vela,
F. Dazzi,
A. De Angelis,
G. De Caneva,
B. De Lotto,
C. Delgado Mendez,
M. Doert,
D. Dominis Prester,
D. Dorner,
M. Doro,
S. Einecke,
D. Eisenacher,
D. Elsaesser,
E. Farina,
D. Ferenc,
D. Fidalgo,
M. V. Fonseca,
L. Font,
K. Frantzen,
C. Fruck,
R. J. García López,
M. Garczarczyk,
D. Garrido Terrats,
M. Gaug,
N. Godinović,
A. González Muñoz,
S. R. Gozzini,
D. Hadasch,
M. Hayashida,
J. Herrera,
A. Herrero,
D. Hildebrand.
"The accretion environment in Vela X-1 during a flaring period using XMM-Newton."Silvia Martínez-Núñez,
José Miguel Torrejón,
Matthias Kühnel,
Peter Kretschmar,
Martin Stuhlinger,
José Joaquín Rodes-Roca,
Feliz Fürst,
Ingo Kreykenbohm,
Antonio Martin-Carrillo,
Andy M.T. Pollock,
Joern Wilms.
