Stefano Valenti
Stefano Valenti
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Citata da
Citata da
Multi-messenger observations of a binary neutron star merger
BP Abbott, S Bloemen, P Canizares, H Falcke, RP Fender, S Ghosh, ...
The man behind the curtain: X-rays drive the UV through NIR variability in the 2013 active galactic nucleus outburst in NGC 2617
BJ Shappee, JL Prieto, D Grupe, CS Kochanek, KZ Stanek, G De Rosa, ...
The Astrophysical Journal 788 (1), 48, 2014
A gravitational-wave standard siren measurement of the Hubble constant
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
arXiv preprint arXiv:1710.05835, 2017
Las Cumbres Observatory global telescope network
TM Brown, N Baliber, FB Bianco, M Bowman, B Burleson, P Conway, ...
Publications of the Astronomical Society of the Pacific 125 (931), 1031, 2013
Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
I Arcavi, G Hosseinzadeh, DA Howell, C McCully, D Poznanski, D Kasen, ...
Nature 551 (7678), 64-66, 2017
Super-luminous type Ic supernovae: catching a magnetar by the tail
C Inserra, SJ Smartt, A Jerkstrand, S Valenti, M Fraser, D Wright, K Smith, ...
The Astrophysical Journal 770 (2), 128, 2013
A giant outburst two years before the core-collapse of a massive star
A Pastorello, SJ Smartt, S Mattila, JJ Eldridge, D Young, K Itagaki, ...
Nature 447 (7146), 829-832, 2007
The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
S Valenti, J David, S Yang, E Cappellaro, L Tartaglia, A Corsi, SW Jha, ...
The Astrophysical Journal Letters 848 (2), L24, 2017
Cosmological constraints from measurements of type Ia supernovae discovered during the first 1.5 yr of the Pan-STARRS1 survey
A Rest, D Scolnic, RJ Foley, ME Huber, R Chornock, G Narayan, JL Tonry, ...
The Astrophysical Journal 795 (1), 44, 2014
The broad-lined Type Ic supernova 2003jd
S Valenti, S Benetti, E Cappellaro, F Patat, P Mazzali, M Turatto, K Hurley, ...
Monthly Notices of the Royal Astronomical Society 383 (4), 1485-1500, 2008
Slowly fading super-luminous supernovae that are not pair-instability explosions
M Nicholl, SJ Smartt, A Jerkstrand, C Inserra, M McCrum, R Kotak, ...
Nature 502 (7471), 346-349, 2013
Localization and broadband follow-up of the gravitational-wave transient GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
The Astrophysical journal letters 826 (1), L13, 2016
Ultra-bright optical transients are linked with type Ic supernovae
A Pastorello, SJ Smartt, MT Botticella, K Maguire, M Fraser, K Smith, ...
The Astrophysical Journal Letters 724 (1), L16, 2010
PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects
SJ Smartt, S Valenti, M Fraser, C Inserra, DR Young, M Sullivan, ...
Astronomy & Astrophysics 579, A40, 2015
The metamorphosis of supernova SN 2008D/XRF 080109: a link between supernovae and GRBs/hypernovae
PA Mazzali, S Valenti, M Della Valle, G Chincarini, DN Sauer, S Benetti, ...
Science 321 (5893), 1185-1188, 2008
SN 2005cs in M51–II. Complete evolution in the optical and the near-infrared
A Pastorello, S Valenti, L Zampieri, H Navasardyan, S Taubenberger, ...
Monthly Notices of the Royal Astronomical Society 394 (4), 2266-2282, 2009
Asphericity in supernova explosions from late-time spectroscopy
K Maeda, K Kawabata, PA Mazzali, M Tanaka, S Valenti, K Nomoto, ...
Science 319 (5867), 1220-1223, 2008
The diversity of Type II supernova versus the similarity in their progenitors
S Valenti, DA Howell, MD Stritzinger, ML Graham, G Hosseinzadeh, ...
Monthly Notices of the Royal Astronomical Society 459 (4), 3939-3962, 2016
Interacting supernovae and supernova impostors: SN 2009ip, is this the end?
A Pastorello, E Cappellaro, C Inserra, SJ Smartt, G Pignata, S Benetti, ...
The Astrophysical Journal 767 (1), 1, 2013
High luminosity, slow ejecta and persistent carbon lines: SN 2009dc challenges thermonuclear explosion scenarios
S Taubenberger, S Benetti, M Childress, R Pakmor, S Hachinger, ...
Monthly Notices of the Royal Astronomical Society 412 (4), 2735-2762, 2011
Il sistema al momento non pu eseguire l'operazione. Riprova pi tardi.
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