Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27582
DC Field | Value | Language |
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dc.contributor.author | BARONCHELLI, IVANO | en_US |
dc.contributor.author | Rodighiero, G. | en_US |
dc.contributor.author | Teplitz, H. I. | en_US |
dc.contributor.author | Scarlata, C. M. | en_US |
dc.contributor.author | Franceschini, A. | en_US |
dc.contributor.author | Berta, S. | en_US |
dc.contributor.author | Barrufet, L. | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.contributor.author | Bonato, M. | en_US |
dc.contributor.author | Ciesla, L. | en_US |
dc.contributor.author | Zanella, A. | en_US |
dc.contributor.author | Carraro, R. | en_US |
dc.contributor.author | Mancini, C. | en_US |
dc.contributor.author | Puglisi, A. | en_US |
dc.contributor.author | Malkan, M. | en_US |
dc.contributor.author | Mei, S. | en_US |
dc.contributor.author | Marchetti, L. | en_US |
dc.contributor.author | Colbert, J. | en_US |
dc.contributor.author | Sedgwick, C. | en_US |
dc.contributor.author | Serjeant, S. | en_US |
dc.contributor.author | Pearson, C. | en_US |
dc.contributor.author | Radovich, M. | en_US |
dc.contributor.author | Grado, A. | en_US |
dc.contributor.author | Limatola, L. | en_US |
dc.contributor.author | Covone, G. | en_US |
dc.date.accessioned | 2020-10-05T13:26:09Z | - |
dc.date.available | 2020-10-05T13:26:09Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27582 | - |
dc.description.abstract | The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field (SEP) covers an area of 7.74 sq. deg to a depth of ~5.80 microJy (3sigma) at 3.6 microns and 5.25 microJy at 4.5 microns. The 90% and 50% completeness limits are at 14 and 9 microJy, respectively. The multiwavelength catalog includes the WFI-Rc, MIPS-24 micron, SPIRE 250, 350 and 500 micron fluxes of the counterparts that were identified by searching for the closest neighbor. <P />The indicator P quantifies the reliability of each association (example, for P1: SPIRE to MIPS) considering both the distance between the SPIRE source and the closest MIPS association and the presence of further possible MIPS associations in the MIPS-SPIRE searching radius. <P />For bands other than IRAC 3.6 microns, a null flux means no coverage in that band, while a flux of zero means that the position is covered in that band but the source is not detected. <P />(1 data file). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: Multiwavelength catalog in the SEP field. II. (Baronchelli+, 2018) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.18570064 | en_US |
dc.identifier.url | https://cdsarc.unistra.fr/viz-bin/cat/J/ApJ/857/64 | en_US |
dc.relation.firstpage | J/ApJ/857/64 | en |
dc.description.international | sì | 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 | 2018yCat..18570064B | 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 | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0003-0556-2929 | - |
crisitem.author.orcid | 0000-0001-9139-2342 | - |
crisitem.author.orcid | 0000-0001-8600-7008 | - |
crisitem.author.orcid | 0000-0002-0501-8256 | - |
Appears in Collections: | 4.06 Banche Dati |
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File | Description | Size | Format | |
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README_vizier.txt | ReadMe | 18.51 kB | Text | View/Open |
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