Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26816
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | MORETTI, ALESSIA | en_US |
dc.contributor.author | GULLIEUSZIK, MARCO | en_US |
dc.contributor.author | POGGIANTI, Bianca Maria | en_US |
dc.contributor.author | Paccagnella, Angela | en_US |
dc.contributor.author | Couch, Warrick J. | en_US |
dc.contributor.author | Vulcani, Benedetta | en_US |
dc.contributor.author | BETTONI, Daniela | en_US |
dc.contributor.author | Fritz, Jacopo | en_US |
dc.contributor.author | Cava, Antonio | en_US |
dc.contributor.author | Fasaano, Giovanni | en_US |
dc.contributor.author | D'ONOFRIO, MAURO | en_US |
dc.contributor.author | Omizzolo, Alessandro | en_US |
dc.date.accessioned | 2020-08-25T14:45:49Z | - |
dc.date.available | 2020-08-25T14:45:49Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26816 | - |
dc.description.abstract | Redshifts, magnitude/radial completeness, and memberships are given for the 17985 galaxies observed as part of the OmegaWINGS survey of local clusters of galaxies over 1 square degree. Redshifts have been measured using both absorption and emission lines features. The sample magnitude completeness is 80% at V=20. Thanks to the observing strategy, the radial completeness turned out to be relatively constant (90%) within the AAOmega field of view. The success rate in measuring redshifts is 95%, at all radii. Cluster members are flagged 1 or 2, depending on the cluster structure/secondary structure, and 0 if they are not cluster members. (1 data file). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: OmegaWINGS local clusters of galaxies redshifts (Moretti+, 2017) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.35990081 | en_US |
dc.identifier.url | https://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/599/A81 | en_US |
dc.relation.firstpage | J/A+A/599/A81 | en |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | VizieR Online Data Catalog | en |
dc.type.miur | 295 Banca dati | - |
dc.identifier.adsbibcode | 2017yCat..35990081M | 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::PE9_9 Clusters of galaxies and large scale structures | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Database | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
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.orcid | 0000-0002-1688-482X | - |
crisitem.author.orcid | 0000-0002-7296-9780 | - |
crisitem.author.orcid | 0000-0001-8751-8360 | - |
crisitem.author.orcid | 0000-0003-0980-1499 | - |
crisitem.author.orcid | 0000-0002-4158-6496 | - |
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