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The LOFAR two-metre sky survey : III. First data release : optical/infrared identifications and value-added catalogue
surveys
catalogues
radio continuum: general
Reproduced with permission from Astronomy & Astrophysics, © ESO
The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120–168 MHz survey of the northern sky with diverse and ambitious science goals. Many of the scientific objectives of LoTSS rely upon, or are enhanced by, the association or separation of the sometimes incorrectly catalogued radio components into distinct radio sources and the identification and characterisation of the optical counterparts to these sources. We present the source associations and optical and/or IR identifications for sources in the first data release, which are made using a combination of statistical techniques and visual association and identification. We document in detail the colour- and magnitude-dependent likelihood ratio method used for statistical identification as well as the Zooniverse project, called LOFAR Galaxy Zoo, used for visual classification. We describe the process used to select which of these two different methods is most appropriate for each LoTSS source. The final LoTSS-DR1-IDs value-added catalogue presented contains 318 520 radio sources, of which 231 716 (73%) have optical and/or IR identifications in Pan-STARRS and WISE.
dc.abstract.en | The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120–168 MHz survey of the northern sky with diverse and ambitious science goals. Many of the scientific objectives of LoTSS rely upon, or are enhanced by, the association or separation of the sometimes incorrectly catalogued radio components into distinct radio sources and the identification and characterisation of the optical counterparts to these sources. We present the source associations and optical and/or IR identifications for sources in the first data release, which are made using a combination of statistical techniques and visual association and identification. We document in detail the colour- and magnitude-dependent likelihood ratio method used for statistical identification as well as the Zooniverse project, called LOFAR Galaxy Zoo, used for visual classification. We describe the process used to select which of these two different methods is most appropriate for each LoTSS source. The final LoTSS-DR1-IDs value-added catalogue presented contains 318 520 radio sources, of which 231 716 (73%) have optical and/or IR identifications in Pan-STARRS and WISE. | pl |
dc.affiliation | Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne | pl |
dc.contributor.author | Williams, W. L. | pl |
dc.contributor.author | Hardcastle, M. J. | pl |
dc.contributor.author | Best, P. N. | pl |
dc.contributor.author | Sabater, J. | pl |
dc.contributor.author | Croston, J. H. | pl |
dc.contributor.author | Duncan, K. J. | pl |
dc.contributor.author | Shimwell, T. W. | pl |
dc.contributor.author | Röttgering, H. J. A. | pl |
dc.contributor.author | Nisbet, D. | pl |
dc.contributor.author | Gürkan, G. | pl |
dc.contributor.author | Alegre, L. | pl |
dc.contributor.author | Cochrane, R. K. | pl |
dc.contributor.author | Goyal, Arti | pl |
dc.contributor.author | Hale, C. L. | pl |
dc.contributor.author | Jackson, N. | pl |
dc.contributor.author | Jamrozy, Marek - 128434 | pl |
dc.contributor.author | Kondapally, R. | pl |
dc.contributor.author | Kunert-Bajraszewska, M. | pl |
dc.contributor.author | Mahatma, V. H. | pl |
dc.contributor.author | Mingo, B. | pl |
dc.contributor.author | Morabito, L. K. | pl |
dc.contributor.author | Prandoni, I. | pl |
dc.contributor.author | Roskowinski, C. | pl |
dc.contributor.author | Shulevski, A. | pl |
dc.contributor.author | Smith, D. J. B. | pl |
dc.contributor.author | Tasse, C. | pl |
dc.contributor.author | Urquhart, S. | pl |
dc.contributor.author | Webster, B. | pl |
dc.contributor.author | White, G. J. | pl |
dc.contributor.author | Beswick, R. J. | pl |
dc.contributor.author | Callingham, J. R. | pl |
dc.contributor.author | Chyży, Krzysztof - 100034 | pl |
dc.contributor.author | de Gasperin, F. | pl |
dc.contributor.author | Harwood, J. J. | pl |
dc.contributor.author | Hoeft, M. | pl |
dc.contributor.author | Iacobelli, M. | pl |
dc.contributor.author | McKean, J. P. | pl |
dc.contributor.author | Mechev, A. P. | pl |
dc.contributor.author | Miley, G. K. | pl |
dc.contributor.author | Schwarz, D. J. | pl |
dc.contributor.author | van Weeren, R. J. | pl |
dc.date.accessioned | 2019-09-04T09:17:26Z | |
dc.date.available | 2019-09-04T09:17:26Z | |
dc.date.issued | 2019 | pl |
dc.date.openaccess | 0 | |
dc.description.accesstime | w momencie opublikowania | |
dc.description.additional | Reproduced with permission from Astronomy & Astrophysics, © ESO | pl |
dc.description.version | ostateczna wersja wydawcy | |
dc.description.volume | 622 | pl |
dc.identifier.articleid | A2 | pl |
dc.identifier.doi | 10.1051/0004-6361/201833564 | pl |
dc.identifier.eissn | 1432-0746 | pl |
dc.identifier.issn | 0004-6361 | pl |
dc.identifier.project | ROD UJ / OP | pl |
dc.identifier.uri | https://ruj.uj.edu.pl/xmlui/handle/item/81771 | |
dc.language | eng | pl |
dc.language.container | eng | pl |
dc.rights | Udzielam licencji. Uznanie autorstwa - Użycie niekomercyjne - Na tych samych warunkach 4.0 Międzynarodowa | * |
dc.rights.licence | Inna otwarta licencja | |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.pl | * |
dc.share.type | inne | |
dc.subject.en | surveys | pl |
dc.subject.en | catalogues | pl |
dc.subject.en | radio continuum: general | pl |
dc.subtype | Article | pl |
dc.title | The LOFAR two-metre sky survey : III. First data release : optical/infrared identifications and value-added catalogue | pl |
dc.title.journal | Astronomy & Astrophysics | pl |
dc.title.volume | LOFAR Surveys : a new window on the Universe | pl |
dc.type | JournalArticle | pl |
dspace.entity.type | Publication |
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