Stefano Covino
Stefano Covino
Istituto Nazionale di AstroFisica / Osservatorio Astronomico di Brera
Bestätigte E-Mail-Adresse bei - Startseite
Zitiert von
Zitiert von
Multi-messenger observations of a binary neutron star merger
BP Abbott, S Bloemen, P Canizares, H Falcke, RP Fender, S Ghosh, ...
Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy
M Actis, G Agnetta, F Aharonian, A Akhperjanian, J Aleksić, E Aliu, D Allan, ...
Experimental Astronomy 32 (3), 193-316, 2011
Introducing the CTA concept
BS Acharya, M Actis, T Aghajani, G Agnetta, J Aguilar, F Aharonian, ...
Astroparticle physics 43, 3-18, 2013
Broadband observations of the naked-eye γ-ray burst GRB 080319B
JL Racusin, SV Karpov, M Sokolowski, J Granot, XF Wu, V Pal’Shin, ...
Nature 455 (7210), 183-188, 2008
GRB 090423 at a redshift of z≈ 8.1
R Salvaterra, M Della Valle, S Campana, G Chincarini, S Covino, ...
Nature 461 (7268), 1258-1260, 2009
Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger
E Pian, P D’Avanzo, S Benetti, M Branchesi, E Brocato, S Campana, ...
Nature 551 (7678), 67-70, 2017
SN 2003lw and GRB 031203: A bright supernova for a faint gamma-ray burst
D Malesani, G Tagliaferri, G Chincarini, S Covino, M Della Valle, ...
The Astrophysical Journal Letters 609 (1), L5, 2004
Very-high-energy gamma rays from a distant quasar: how transparent is the universe?
J Albert, E Aliu, H Anderhub, LA Antonelli, P Antoranz, M Backes, ...
Science 320 (5884), 1752-1754, 2008
The X-ray counterpart to the gravitational-wave event GW170817
E Troja, L Piro, H Van Eerten, RT Wollaeger, M Im, OD Fox, NR Butler, ...
Nature 551 (7678), 71-74, 2017
Relativistic jet activity from the tidal disruption of a star by a massive black hole
DN Burrows, JA Kennea, G Ghisellini, V Mangano, B Zhang, KL Page, ...
Nature 476 (7361), 421-424, 2011
An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
M Della Valle, G Chincarini, N Panagia, G Tagliaferri, D Malesani, V Testa, ...
Nature 444 (7122), 1050-1052, 2006
An origin for short γ-ray bursts unassociated with current star formation
SD Barthelmy, G Chincarini, DN Burrows, N Gehrels, S Covino, A Moretti, ...
Nature 438 (7070), 994-996, 2005
The major upgrade of the MAGIC telescopes, Part II: A performance study using observations of the Crab Nebula
J Aleksić, S Ansoldi, LA Antonelli, P Antoranz, A Babic, P Bangale, ...
Astroparticle Physics 72, 76-94, 2016
Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
L Telescope, M Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, ...
Science 361 (6398), 2018
The afterglows of Swift-era gamma-ray bursts. I. Comparing pre-Swift and Swift-era long/soft (type II) GRB optical afterglows
DA Kann, S Klose, B Zhang, D Malesani, E Nakar, A Pozanenko, ...
The Astrophysical Journal 720 (2), 1513, 2010
MAGIC discovery of very high energy emission from the FSRQ PKS 1222+ 21
J Aleksić, LA Antonelli, P Antoranz, M Backes, JA Barrio, D Bastieri, ...
The Astrophysical Journal Letters 730 (1), L8, 2011
Fermi Large Area Telescope observations of Markarian 421: The missing piece of its spectral energy distribution
AA Abdo, M Ackermann, M Ajello, L Baldini, J Ballet, G Barbiellini, ...
The Astrophysical Journal 736 (2), 131, 2011
Performance of the MAGIC stereo system obtained with Crab Nebula data
J Aleksić, EA Alvarez, LA Antonelli, P Antoranz, M Asensio, M Backes, ...
Astroparticle Physics 35 (7), 435-448, 2012
REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination
E Molinari, SD Vergani, D Malesani, S Covino, P d'Avanzo, G Chincarini, ...
Astronomy & Astrophysics 469 (1), L13-L16, 2007
The HARPS search for southern extra-solar planets-VI. A Neptune-mass planet around the nearby M dwarf Gl 581
X Bonfils, T Forveille, X Delfosse, S Udry, M Mayor, C Perrier, F Bouchy, ...
Astronomy & Astrophysics 443 (3), L15-L18, 2005
Das System kann den Vorgang jetzt nicht ausführen. Versuchen Sie es später erneut.
Artikel 1–20