Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27915
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BOTTICELLA, MARIA TERESA | en_US |
dc.contributor.author | CAPPELLARO, Enrico | en_US |
dc.contributor.author | Pignata, G. | en_US |
dc.contributor.author | GRADO, ANIELLO | en_US |
dc.contributor.author | Limatola, L. | en_US |
dc.contributor.author | DELLA VALLE, Massimo | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.contributor.author | GREGGIO, Laura | en_US |
dc.contributor.author | Spiro, S. | en_US |
dc.contributor.author | BUFANO, FILOMENA | en_US |
dc.contributor.author | TOMASELLA, Lina | en_US |
dc.contributor.author | Covone, G. | en_US |
dc.contributor.author | Capaccioli, M. | en_US |
dc.contributor.author | NAPOLITANO, NICOLA ROSARIO | en_US |
dc.contributor.author | Marchetti, L. | en_US |
dc.contributor.author | Gonzales-Solares, E. | en_US |
dc.contributor.author | Jarvis, M. | en_US |
dc.contributor.author | RADOVICH, MARIO | en_US |
dc.contributor.author | BENETTI, Stefano | en_US |
dc.contributor.author | PASTORELLO, Andrea | en_US |
dc.contributor.author | TURATTO, Massimo | en_US |
dc.contributor.author | Paolillo, Maurizio | en_US |
dc.contributor.author | SCHIPANI, Pietro | en_US |
dc.contributor.author | BARUFFOLO, Andrea | en_US |
dc.contributor.author | CASCONE, Enrico | en_US |
dc.date.accessioned | 2020-10-22T10:19:52Z | - |
dc.date.available | 2020-10-22T10:19:52Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 978-3-319-19329-8 | en_US |
dc.identifier.isbn | 978-3-319-19330-4 | en_US |
dc.identifier.issn | 1570-6591 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27915 | - |
dc.description.abstract | Despite the key role played by Supernovae (SNe) in discovering the accelerating expansion of the Universe, there are still fundamental questions to answer about their progenitor systems and explosion mechanisms. Furthermore the discovery of a significant number of both exceptionally bright and extremely faint SNe, as well as peculiar events, suggests the existence of an unexpected diversity. Important clues on the SN progenitors can be derived by examining the rate of type Ia and core collapse SNe. With this goal in mind we started the SUpernova Diversity And Rate Evolution (SUDARE) programme currently running at the VLT Survey Telescope (VST). We present a measurement of the volumetric SN rates as a function of redshift for the first 2 years of data from SUDARE. | en_US |
dc.language.iso | eng | en_US |
dc.title | First Results from Supernova Diversity and Rate Evolution (SUDARE) Survey at VST | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1007/978-3-319-19330-4_31 | en_US |
dc.identifier.scopus | 2-s2.0-84978993722 | en_US |
dc.identifier.isi | 000389802600032 | en_US |
dc.identifier.url | https://link.springer.com/chapter/10.1007%2F978-3-319-19330-4_31 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 42 | en_US |
dc.relation.firstpage | 197 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.alleditors | Napolitano, Nicola R.; Longo, Giuseppe; Marconi, Marcella; Paolillo, Maurizio; Iodice, Enrichetta | en_US |
dc.relation.ispartofbook | The Universe of Digital Sky Surveys: a Meeting to Honour the 70th Birthday of Massimo Capaccioli | en_US |
dc.relation.conferencename | The Universe of Digital Sky Surveys: a Meeting to Honour the 70th Birthday of Massimo Capaccioli | en_US |
dc.relation.conferenceplace | Napoli, Italy | en_US |
dc.relation.conferencedate | 25-28 November, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | ASTROPHYSICS AND SPACE SCIENCE PROCEEDINGS | en_US |
dc.identifier.adsbibcode | 2016ASSP...42..197B | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0002-3938-692X | - |
crisitem.author.orcid | 0000-0001-5008-8619 | - |
crisitem.author.orcid | 0000-0002-0501-8256 | - |
crisitem.author.orcid | 0000-0003-3142-5020 | - |
crisitem.author.orcid | 0000-0003-2634-4875 | - |
crisitem.author.orcid | 0000-0002-3429-2481 | - |
crisitem.author.orcid | 0000-0002-3697-2616 | - |
crisitem.author.orcid | 0000-0003-0911-8884 | - |
crisitem.author.orcid | 0000-0002-3585-866X | - |
crisitem.author.orcid | 0000-0002-3256-0016 | - |
crisitem.author.orcid | 0000-0002-7259-4624 | - |
crisitem.author.orcid | 0000-0002-9719-3157 | - |
crisitem.author.orcid | 0000-0003-4210-7693 | - |
crisitem.author.orcid | 0000-0003-0197-589X | - |
crisitem.author.orcid | 0000-0002-1114-4355 | - |
crisitem.author.orcid | 0000-0002-7425-7517 | - |
crisitem.journal.journalissn | 1570-6591 | - |
crisitem.journal.ance | E210911 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
Botticella2016_Chapter_FirstResultsFromSupernovaDiver.pdf | Pdf editoriale | 123.09 kB | Adobe PDF |
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