Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27684| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Levin, L. | en_US |
| dc.contributor.author | Armour, W. | en_US |
| dc.contributor.author | BAFFA, Carlo | en_US |
| dc.contributor.author | Barr, E. | en_US |
| dc.contributor.author | Cooper, S. | en_US |
| dc.contributor.author | Eatough, R. | en_US |
| dc.contributor.author | Ensor, A. | en_US |
| dc.contributor.author | GIANI, Elisabetta | en_US |
| dc.contributor.author | Karastergiou, A. | en_US |
| dc.contributor.author | Karuppusamy, R. | en_US |
| dc.contributor.author | Keith, M. | en_US |
| dc.contributor.author | Kramer, M. | en_US |
| dc.contributor.author | Lyon, R. | en_US |
| dc.contributor.author | Mackintosh, M. | en_US |
| dc.contributor.author | Mickaliger, M. | en_US |
| dc.contributor.author | van Nieuwpoort, R. | en_US |
| dc.contributor.author | Pearson, M. | en_US |
| dc.contributor.author | Prabu, T. | en_US |
| dc.contributor.author | Roy, J. | en_US |
| dc.contributor.author | Sinnen, O. | en_US |
| dc.contributor.author | Spitler, L. | en_US |
| dc.contributor.author | Spreeuw, H. | en_US |
| dc.contributor.author | Stappers, B. W. | en_US |
| dc.contributor.author | van Straten, W. | en_US |
| dc.contributor.author | Williams, C. | en_US |
| dc.contributor.author | Wang, H. | en_US |
| dc.contributor.author | Wiesner, K. | en_US |
| dc.contributor.author | SKA TDT Team | en_US |
| dc.date.accessioned | 2020-10-09T12:32:03Z | - |
| dc.date.available | 2020-10-09T12:32:03Z | - |
| dc.date.issued | 2018 | en_US |
| dc.identifier.issn | 1743-9213 | en_US |
| dc.identifier.uri | http://hdl.handle.net/20.500.12386/27684 | - |
| dc.description.abstract | The Square Kilometre Array will be an amazing instrument for pulsar astronomy. While the full SKA will be sensitive enough to detect all pulsars in the Galaxy visible from Earth, already with SKA1, pulsar searches will discover enough pulsars to increase the currently known population by a factor of four, no doubt including a range of amazing unknown sources. Real time processing is needed to deal with the 60 PB of pulsar search data collected per day, using a signal processing pipeline required to perform more than 10 POps. Here we present the suggested design of the pulsar search engine for the SKA and discuss challenges and solutions to the pulsar search venture. | en_US |
| dc.language.iso | eng | en_US |
| dc.title | Pulsar Searches with the SKA | en_US |
| dc.type | Conference paper | - |
| dc.identifier.doi | 10.1017/S1743921317009528 | en_US |
| dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/pulsar-searches-with-the-ska/4AEEB52DC21A83E013937FE19DB0C2B0 | en_US |
| dc.relation.medium | STAMPA | en_US |
| dc.relation.volume | vol. 13, S337 | en_US |
| dc.relation.firstpage | 171 | en_US |
| dc.relation.lastpage | 174 | en_US |
| dc.relation.numberofpages | 4 | en_US |
| dc.type.referee | REF_1 | en_US |
| dc.description.numberofauthors | 27 | en_US |
| dc.description.international | sì | en_US |
| dc.contributor.country | ITA | en_US |
| dc.contributor.country | GBR | en_US |
| dc.contributor.country | DEU | en_US |
| dc.contributor.country | AUS | en_US |
| dc.contributor.country | GRC | en_US |
| dc.contributor.country | IND | en_US |
| dc.contributor.country | IRL | en_US |
| dc.contributor.country | NZL | en_US |
| dc.contributor.country | ZAF | en_US |
| dc.relation.alleditors | Weltevrede, P.; Perera, B.B.P.;Preston, L.L.; Sanidas, S. | en_US |
| dc.relation.ispartofbook | Pulsar Astrophysics the Next Fifty Years | en_US |
| dc.type.invited | no | en_US |
| dc.relation.conferencename | Pulsar Astrophysics the Next Fifty Years | en_US |
| dc.relation.conferenceplace | Jodrell Bank Observatory, United Kingdom | en_US |
| dc.relation.conferencedate | 4-8 September, 2017 | en_US |
| dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
| dc.type.miur | 273 Contributo in Atti di convegno | - |
| dc.relation.series | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | en_US |
| dc.identifier.adsbibcode | 2018IAUS..337..171L | en_US |
| dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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.fulltext | With Fulltext | - |
| item.languageiso639-1 | en | - |
| crisitem.author.dept | O.A. Arcetri | - |
| crisitem.author.dept | O.A. Arcetri | - |
| crisitem.author.orcid | 0000-0002-4935-100X | - |
| crisitem.author.orcid | 0000-0003-2763-9560 | - |
| Appears in Collections: | 3.01 Contributi in Atti di convegno | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| pulsar_searches_with_the_ska.pdf | Pdf editoriale | 168.13 kB | Adobe PDF | View/Open |
Page view(s)
19
checked on Nov 24, 2020
Download(s)
5
checked on Nov 24, 2020
Google ScholarTM
Check
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.