Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26214
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | INNO, LAURA | en_US |
dc.contributor.author | Matsunaga, N. | en_US |
dc.contributor.author | Romaniello, M. | en_US |
dc.contributor.author | Bono, G. | en_US |
dc.contributor.author | Monson, A. | en_US |
dc.contributor.author | Ferraro, I. | en_US |
dc.contributor.author | Iannicola, G. | en_US |
dc.contributor.author | Persson, E. | en_US |
dc.contributor.author | Buonanno, R. | en_US |
dc.contributor.author | Freedman, W. | en_US |
dc.contributor.author | Gieren, W. | en_US |
dc.contributor.author | Groenewegen, M. A. T. | en_US |
dc.contributor.author | Ita, Y. | en_US |
dc.contributor.author | Laney, C. D. | en_US |
dc.contributor.author | Lemasle, B. | en_US |
dc.contributor.author | Madore, B. F. | en_US |
dc.contributor.author | Nagayama, T. | en_US |
dc.contributor.author | Nakada, Y. | en_US |
dc.contributor.author | NONINO, Mario | en_US |
dc.contributor.author | Pietrzynski, G. | en_US |
dc.contributor.author | Primas, F. | en_US |
dc.contributor.author | Scowcroft, V. | en_US |
dc.contributor.author | Soszynski, I. | en_US |
dc.contributor.author | Tanabe, T. | en_US |
dc.contributor.author | Udalski, A. | en_US |
dc.date.accessioned | 2020-06-25T14:20:27Z | - |
dc.date.available | 2020-06-25T14:20:27Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26214 | - |
dc.description.abstract | Our analysis is based on the largest available sample of fundamental-mode Cepheids with well-covered light-curves in the NIR and in optical (V, I) bands. This sample covers a very broad period range (1-100 days). We collected J, H, and KS band observations from four different data sets: Laney & Stobie (1992A&AS...93...93L, 51) and Monson & Pierce (2011ApJS..193...12M, 131) for Galactic Cepheids, Persson et al. (2004AJ....128.2239P, 92) for LMC Cepheids, and the IRSF survey catalog for ~500 Small Magellanic Cloud (SMC) Cepheids. (2 data files). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: NIR light-curve templates for classical Cepheids (Inno+, 2015) | en_US |
dc.type | Database | - |
dc.identifier.doi | https://doi.org//10.26093/cds/vizier.35760030 | en_US |
dc.identifier.url | https://cdsarc.unistra.fr/viz-bin/cat/J/A+A/576/A30 | en_US |
dc.relation.firstpage | J/A+A/576/A30 | 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 | 2015yCat..35760030I | 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.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. Capodimonte | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0002-0271-2664 | - |
crisitem.author.orcid | 0000-0001-6342-9662 | - |
È visualizzato nelle collezioni: | 4.06 Banche Dati |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
A30.vizier.txt | ReadMe | 5.35 kB | Text | Visualizza/apri |
Page view(s)
157
controllato il 2-mag-2024
Download(s)
10
controllato il 2-mag-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.