Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32492
DC Field | Value | Language |
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dc.contributor.author | Hardcastle, M. J. | en_US |
dc.contributor.author | Gurkan, G. | en_US |
dc.contributor.author | van Weeren, R. J. | en_US |
dc.contributor.author | Williams, W. L. | en_US |
dc.contributor.author | Best, P. N. | en_US |
dc.contributor.author | de Gasperin, F. | en_US |
dc.contributor.author | Rafferty, D. A. | en_US |
dc.contributor.author | READ, SHAUN CONISBEE | en_US |
dc.contributor.author | Sabater, J. | en_US |
dc.contributor.author | Shimwell, T. W. | en_US |
dc.contributor.author | Smith, D. J. B. | en_US |
dc.contributor.author | Tasse, C. | en_US |
dc.contributor.author | Bourne, N. | en_US |
dc.contributor.author | BRIENZA, MARISA | en_US |
dc.contributor.author | Bruggen, M. | en_US |
dc.contributor.author | BRUNETTI, GIANFRANCO | en_US |
dc.contributor.author | Chyzy, K. T. | en_US |
dc.contributor.author | Conway, J. | en_US |
dc.contributor.author | Dunne, L. | en_US |
dc.contributor.author | Eales, S. A. | en_US |
dc.contributor.author | Maddox, S. J. | en_US |
dc.contributor.author | Jarvis, M. J. | en_US |
dc.contributor.author | Mahony, E. K. | en_US |
dc.contributor.author | Morganti, R. | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | Rottgering, H. J. A. | en_US |
dc.contributor.author | Valiante, E. | en_US |
dc.contributor.author | White, G. J. | en_US |
dc.date.accessioned | 2022-07-14T14:26:15Z | - |
dc.date.available | 2022-07-14T14:26:15Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32492 | - |
dc.description.abstract | The NGP field was observed in four separate pointings, chosen to maximize sky covered, with the LOFAR HBA as part of the Surveys Key Science project. Observations used the HBA<SUB>DUAL</SUB>INNER mode, meaning that the station beams of core and remote stations roughly matched each other and giving the widest possible field of view. The first observation, which was made early on in LOFAR operations, was of slightly longer duration (~10h) than the others (~8h). International stations were included in some of the observations in 2014 but were not used in any of our analysis, which uses only the Dutch array. <P />(1 data file). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: H-ATLAS NGP LOFAR radio catalogue (Hardcastle+, 2016) | en_US |
dc.type | Database | - |
dc.identifier.url | https://cdsarc.unistra.fr/viz-bin/cat/J/MNRAS/462/1910 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | VizieR Online Data Catalog | - |
dc.type.miur | 295 Banca dati | - |
dc.identifier.adsbibcode | 2018yCat..74621910H | 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.oa | 3 - prodotto già presente in altro archivio Open Access, es. VizieR (allegare file read.me al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Database | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0001-9188-9359 | - |
crisitem.author.orcid | 0000-0003-4120-9970 | - |
crisitem.author.orcid | 0000-0003-4195-8613 | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
Appears in Collections: | 4.06 Banche Dati |
Files in This Item:
File | Description | Size | Format | |
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J-MNRAS-462-1910.pdf | ReadMe | 99.86 kB | Adobe PDF | View/Open |
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