Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34817
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MASELLI, Alessandro | en_US |
dc.contributor.author | MELANDRI, Andrea | en_US |
dc.contributor.author | Nava, Lara | en_US |
dc.contributor.author | Mundell, C. G. | en_US |
dc.contributor.author | Kawai, N. | en_US |
dc.contributor.author | CAMPANA, Sergio | en_US |
dc.contributor.author | COVINO, Stefano | en_US |
dc.contributor.author | Cummings, J. R. | en_US |
dc.contributor.author | CUSUMANO, GIANCARLO | en_US |
dc.contributor.author | Evans, P. A. | en_US |
dc.contributor.author | GHIRLANDA, Giancarlo | en_US |
dc.contributor.author | GHISELLINI, Gabriele | en_US |
dc.contributor.author | Guidorzi, C. | en_US |
dc.contributor.author | Kobayashi, S. | en_US |
dc.contributor.author | Kuin, P. | en_US |
dc.contributor.author | LA PAROLA, VALENTINA | en_US |
dc.contributor.author | MANGANO, VALERIA | en_US |
dc.contributor.author | Oates, S. | en_US |
dc.contributor.author | Sakamoto, T. | en_US |
dc.contributor.author | Serino, M. | en_US |
dc.contributor.author | Virgili, F. | en_US |
dc.contributor.author | Zhang, B. -B. | en_US |
dc.contributor.author | Barthelmy, S. | en_US |
dc.contributor.author | Beardmore, A. | en_US |
dc.contributor.author | BERNARDINI, Maria Grazia | en_US |
dc.contributor.author | Bersier, D. | en_US |
dc.contributor.author | Burrows, D. | en_US |
dc.contributor.author | CALDERONE, GIORGIO | en_US |
dc.contributor.author | CAPALBI, Milvia | en_US |
dc.contributor.author | Chiang, J. | en_US |
dc.contributor.author | D'AVANZO, Paolo | en_US |
dc.contributor.author | D'Elia, V. | en_US |
dc.contributor.author | De Pasquale, M. | en_US |
dc.contributor.author | FUGAZZA, Dino Pierluigi | en_US |
dc.contributor.author | Gehrels, N. | en_US |
dc.contributor.author | Gomboc, A. | en_US |
dc.contributor.author | Harrison, R. | en_US |
dc.contributor.author | Hanayama, H. | en_US |
dc.contributor.author | Japelj, J. | en_US |
dc.contributor.author | Kennea, J. | en_US |
dc.contributor.author | Kopac, D. | en_US |
dc.contributor.author | Kouveliotou, C. | en_US |
dc.contributor.author | Kuroda, D. | en_US |
dc.contributor.author | Levan, A. | en_US |
dc.contributor.author | Malesani, D. | en_US |
dc.contributor.author | Marshall, F. | en_US |
dc.contributor.author | Nousek, J. | en_US |
dc.contributor.author | O'Brien, P. | en_US |
dc.contributor.author | Osborne, J. P. | en_US |
dc.contributor.author | Pagani, C. | en_US |
dc.contributor.author | Page, K. L. | en_US |
dc.contributor.author | Page, M. | en_US |
dc.contributor.author | PERRI, Matteo | en_US |
dc.contributor.author | Pritchard, T. | en_US |
dc.contributor.author | Romano, P. | en_US |
dc.contributor.author | Saito, Y. | en_US |
dc.contributor.author | Sbarufatti, B. | en_US |
dc.contributor.author | SALVATERRA, Ruben | en_US |
dc.contributor.author | Steele, I. | en_US |
dc.contributor.author | Tanvir, N. | en_US |
dc.contributor.author | Vianello, G. | en_US |
dc.contributor.author | Weigand, B. | en_US |
dc.contributor.author | Wiersema, K. | en_US |
dc.contributor.author | Yatsu, Y. | en_US |
dc.contributor.author | Yoshii, T. | en_US |
dc.contributor.author | TAGLIAFERRI, Gianpiero | en_US |
dc.date.accessioned | 2024-02-22T16:45:21Z | - |
dc.date.available | 2024-02-22T16:45:21Z | - |
dc.date.issued | 2014 | en_US |
dc.identifier.issn | 0036-8075 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34817 | - |
dc.description.abstract | Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ∼ 3 × 10<SUP>53</SUP> ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies. | en_US |
dc.language.iso | eng | en_US |
dc.title | GRB 130427A: A Nearby Ordinary Monster | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1126/science.1242279 | en_US |
dc.identifier.scopus | 2-s2.0-84896711884 | en_US |
dc.identifier.url | http://arxiv.org/abs/1311.5254v3 | en_US |
dc.identifier.url | https://www.science.org/doi/10.1126/science.1242279 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 343 | en_US |
dc.relation.issue | 6166 | en_US |
dc.relation.firstpage | 48 | en_US |
dc.relation.lastpage | 51 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | JPN | en_US |
dc.contributor.country | SVN | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2014Sci...343...48M | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0036-8075 | - |
crisitem.journal.ance | E151981 | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IASF Palermo | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IASF Palermo | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0003-3760-1910 | - |
crisitem.author.orcid | 0000-0002-2810-2143 | - |
crisitem.author.orcid | 0000-0001-5960-0455 | - |
crisitem.author.orcid | 0000-0001-6278-1576 | - |
crisitem.author.orcid | 0000-0001-9078-5507 | - |
crisitem.author.orcid | 0000-0002-8151-1990 | - |
crisitem.author.orcid | 0000-0001-5876-9259 | - |
crisitem.author.orcid | 0000-0002-0037-1974 | - |
crisitem.author.orcid | 0000-0002-8087-6488 | - |
crisitem.author.orcid | 0000-0002-9903-4053 | - |
crisitem.author.orcid | 0000-0001-6106-3046 | - |
crisitem.author.orcid | 0000-0002-7738-5389 | - |
crisitem.author.orcid | 0000-0002-9558-2394 | - |
crisitem.author.orcid | 0000-0001-7164-1508 | - |
crisitem.author.orcid | 0000-0001-9942-277X | - |
crisitem.author.orcid | 0000-0003-3613-4409 | - |
crisitem.author.orcid | 0000-0002-9393-8078 | - |
crisitem.author.orcid | 0000-0003-0121-0723 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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1311.5254.pdf | 4.73 MB | Adobe PDF | View/Open |
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