Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24054
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Jarvis, M. | en_US |
dc.contributor.author | Seymour, N. | en_US |
dc.contributor.author | Afonso, J. | en_US |
dc.contributor.author | Best, P. | en_US |
dc.contributor.author | Beswick, R. | en_US |
dc.contributor.author | Heywood, I. | en_US |
dc.contributor.author | Huynh, M. | en_US |
dc.contributor.author | Murphy, E. | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | Schinnerer, E. | en_US |
dc.contributor.author | Simpson, C. | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.contributor.author | White, S. | en_US |
dc.date.accessioned | 2020-04-15T14:32:04Z | - |
dc.date.available | 2020-04-15T14:32:04Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 978-1-909204-70-6 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24054 | - |
dc.description.abstract | Radio wavelengths offer the unique possibility of tracing the total star-formation rate in galaxies, both obscured and unobscured. As such, they may provide the most robust measurement of the star-formation history of the Universe. In this chapter we highlight the constraints that the SKA can place on the evolution of the star-formation history of the Universe, the survey area required to overcome sample variance, the spatial resolution requirements, along with the multi-wavelength ancillary data that will play a major role in maximising the scientific promise of the SKA. The required combination of depth and resolution means that a survey to trace the star formation in the Universe should be carried out with a facility that has a resolution of at least ~0.5arcsec, with high sensitivity at < 1 GHz. We also suggest a strategy that will enable new parameter space to be explored as the SKA expands over the coming decade. | en_US |
dc.language.iso | eng | en_US |
dc.title | The star-formation history of the Universe with the SKA | en_US |
dc.type | Conference paper | - |
dc.identifier.url | https://pos.sissa.it/215/068/ | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 215 | en_US |
dc.relation.firstpage | 68 | en_US |
dc.type.referee | REF_3 | en_US |
dc.description.numberofauthors | 13 | en_US |
dc.description.international | sì | en_US |
dc.relation.ispartofbook | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
dc.relation.conferenceplace | Giardini Naxos, Italy | en_US |
dc.relation.conferencedate | 9-13 June, 2014 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015aska.confE..68J | 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 | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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AASKA14_068.pdf | 3.47 MB | Adobe PDF | View/Open |
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