Andrea Pastorello
Andrea Pastorello
INAF - Osservatorio Astronomico di Padova
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Citata da
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Multi-messenger observations of a binary neutron star merger
BP Abbott
A kilonova as the electromagnetic counterpart to a gravitational-wave source
SJ Smartt, TW Chen, A Jerkstrand, M Coughlin, E Kankare, SA Sim, ...
Nature 551 (7678), 75-79, 2017
Detection of circumstellar material in a normal type Ia supernova
F Patat, P Chandra, R Chevalier, S Justham, P Podsiadlowski, C Wolf, ...
Science 317 (5840), 924-926, 2007
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
Photometry and spectroscopy of the Type IIP SN 1999em from outburst to dust formation
A Elmhamdi, IJ Danziger, N Chugai, A Pastorello, M Turatto, E Cappellaro, ...
Monthly Notices of the Royal Astronomical Society 338 (4), 939-956, 2003
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
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
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
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
Low-luminosity Type II supernovae: spectroscopic and photometric evolution
A Pastorello, L Zampieri, M Turatto, E Cappellaro, WPS Meikle, S Benetti, ...
Monthly Notices of the Royal Astronomical Society 347 (1), 74-94, 2004
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
Supernova 2002bo: inadequacy of the single parameter description
S Benetti, P Meikle, M Stehle, G Altavilla, S Desidera, G Folatelli, ...
Monthly Notices of the Royal Astronomical Society 348 (1), 261-278, 2004
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
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
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
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
Direct analysis of spectra of type Ib supernovae
D Branch, S Benetti, D Kasen, E Baron, DJ Jeffery, K Hatano, ...
The Astrophysical Journal 566 (2), 1005, 2002
SN 2004aw: confirming diversity of Type Ic supernovae
S Taubenberger, A Pastorello, PA Mazzali, S Valenti, G Pignata, ...
Monthly Notices of the Royal Astronomical Society 371 (3), 1459-1477, 2006
Il sistema al momento non pu eseguire l'operazione. Riprova pi tardi.
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