Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31088
DC Field | Value | Language |
---|---|---|
dc.contributor.author | D'ORAZI, VALENTINA | en_US |
dc.contributor.author | OLIVA, Ernesto | en_US |
dc.contributor.author | BRAGAGLIA, Angela | en_US |
dc.contributor.author | FRASCA, Antonio | en_US |
dc.contributor.author | SANNA, Nicoletta | en_US |
dc.contributor.author | BIAZZO, Katia | en_US |
dc.contributor.author | Casali, G. | en_US |
dc.contributor.author | DESIDERA, Silvano | en_US |
dc.contributor.author | LUCATELLO, Sara | en_US |
dc.contributor.author | MAGRINI, LAURA | en_US |
dc.contributor.author | ORIGLIA, Livia | en_US |
dc.date.accessioned | 2021-11-16T14:04:55Z | - |
dc.date.available | 2021-11-16T14:04:55Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31088 | - |
dc.description.abstract | GIARPS (the simultaneous observing mode of the spectrographers GIANO and HARPS-N) at the 3.6m telescope TNG was used to target ten solar-type dwarfs in the Praesepe cluster (Table 1). Observations were carried out between December 2018 and January 2019. <P />The instrument configuration allows us to operate with the HARPS-N spectrograph (R=115000, λλ=3800-6900Å), and the GIANO-B near-infrared (NIR) spectrograph (R=50000, 0.97-2.5um). <P />Equivalent width for different species measured in 10 solar-type stars in Praesepe (table2.dat). <P />Stellar parameters and abundances is found in the table stars.dat (table 1 and 5 of the paper). <P />(2 data files). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: EW of 10 solar-type stars of Praesepe (D'Orazi+, 2020) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.36330038 | en_US |
dc.identifier.url | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/633/A38 | en_US |
dc.relation.firstpage | J/A+A/633/A38 | en |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | VizieR Online Data Catalog | en |
dc.type.miur | 295 Banca dati | en_US |
dc.identifier.adsbibcode | 2020yCat..36330038D | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Database | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-2662-3762 | - |
crisitem.author.orcid | 0000-0002-9123-0412 | - |
crisitem.author.orcid | 0000-0002-0338-7883 | - |
crisitem.author.orcid | 0000-0002-0474-0896 | - |
crisitem.author.orcid | 0000-0001-9275-9492 | - |
crisitem.author.orcid | 0000-0002-1892-2180 | - |
crisitem.author.orcid | 0000-0001-8613-2589 | - |
crisitem.author.orcid | 0000-0001-8808-0073 | - |
crisitem.author.orcid | 0000-0003-4486-6802 | - |
crisitem.author.orcid | 0000-0002-6040-5849 | - |
Appears in Collections: | 4.06 Banche Dati |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
ReadMe_AA-573-A13.txt | ReadMe | 5.59 kB | Text | View/Open |
Page view(s)
36
checked on Mar 28, 2024
Download(s)
15
checked on Mar 28, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.