Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31511
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Christiansen, J. L. | en_US |
dc.contributor.author | Vanderburg, A. | en_US |
dc.contributor.author | Burt, J. | en_US |
dc.contributor.author | Fulton, B. J. | en_US |
dc.contributor.author | Batygin, K. | en_US |
dc.contributor.author | Benneke, B. | en_US |
dc.contributor.author | Brewer, J. M. | en_US |
dc.contributor.author | Charbonneau, D. | en_US |
dc.contributor.author | Ciardi, D. R. | en_US |
dc.contributor.author | Cameron, A. C. | en_US |
dc.contributor.author | Coughlin, J. L. | en_US |
dc.contributor.author | Crossfield, I. J. M. | en_US |
dc.contributor.author | Dressing, C. | en_US |
dc.contributor.author | Greene, T. P. | en_US |
dc.contributor.author | Howard, A. W. | en_US |
dc.contributor.author | Latham, D. W. | en_US |
dc.contributor.author | MOLINARI, Emilio Carlo | en_US |
dc.contributor.author | Mortier, A. | en_US |
dc.contributor.author | Mullally, F. | en_US |
dc.contributor.author | Pepe, F. | en_US |
dc.contributor.author | Rice, K. | en_US |
dc.contributor.author | Sinukoff, E. | en_US |
dc.contributor.author | SOZZETTI, Alessandro | en_US |
dc.contributor.author | Thompson, S. E. | en_US |
dc.contributor.author | Udry, S. | en_US |
dc.contributor.author | Vogt, S. S. | en_US |
dc.contributor.author | Barman, T. S. | en_US |
dc.contributor.author | Batalha, N. E. | en_US |
dc.contributor.author | Bouchy, F. | en_US |
dc.contributor.author | Buchhave, L. A. | en_US |
dc.contributor.author | Butler, R. P. | en_US |
dc.contributor.author | Cosentino, R. | en_US |
dc.contributor.author | Dupuy, T. J. | en_US |
dc.contributor.author | Ehrenreich, D. | en_US |
dc.contributor.author | Fiorenzano, A. | en_US |
dc.contributor.author | Hansen, B. M. S. | en_US |
dc.contributor.author | Henning, T. | en_US |
dc.contributor.author | Hirsch, L. | en_US |
dc.contributor.author | Holden, B. P. | en_US |
dc.contributor.author | Isaacson, H. T. | en_US |
dc.contributor.author | Johnson, J. A. | en_US |
dc.contributor.author | Knutson, H. A. | en_US |
dc.contributor.author | Kosiarek, M. | en_US |
dc.contributor.author | Lopez-Morales, M. | en_US |
dc.contributor.author | Lovis, C. | en_US |
dc.contributor.author | Malavolta, L. | en_US |
dc.contributor.author | Mayor, M. | en_US |
dc.contributor.author | MICELA, Giuseppina | en_US |
dc.contributor.author | Motalebi, F. | en_US |
dc.contributor.author | Petigura, E. | en_US |
dc.contributor.author | Phillips, D. F. | en_US |
dc.contributor.author | Piotto, G. | en_US |
dc.contributor.author | Rogers, L. A. | en_US |
dc.contributor.author | Sasselov, D. | en_US |
dc.contributor.author | Schlieder, J. E. | en_US |
dc.contributor.author | Segransan, D. | en_US |
dc.contributor.author | Watson, C. A. | en_US |
dc.contributor.author | Weiss, L. M. | en_US |
dc.date.accessioned | 2022-03-01T14:29:58Z | - |
dc.date.available | 2022-03-01T14:29:58Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31511 | - |
dc.description.abstract | The final data set includes observations obtained with Keck/HIRES, Automated Planet Finder (APF)/Levy, and HARPS-N. Our observational setup for both Keck/HIRES and the APF/Levy was essentially identical to those described in Fulton et al. (2016, J/ApJ/830/46) and Burt et al. (2014ApJ...789..114B). We collected a total of 60 RV measurements using Keck/HIRES (Vogt et al. 1994SPIE.2198..362V), and 116 measurements using the Levy Spectrograph on the APF (Radovan et al. 2014SPIE.9145E..2BR; Vogt et al. 2014PASP..126..359V) at Lick Observatory between 2016 July 7 and 2016 December 2. We also observed HD 3167 with the HARPS-N spectrograph (Cosentino et al. 2012SPIE.8446E..1VC) located at the 3.58 m Telescopio Nazionale Galileo on the island of La Palma, Spain. HARPS-N is a stabilized spectrograph designed for precise RV measurements. We observed HD 3167 76 times between 2016 July 7 (independently beginning the same night as the HIRES/APF campaign) and 2016 December 7, obtaining high-resolution optical spectra with a spectral resolving power of R=115000. <P />(1 data file). | en_US |
dc.language.iso | eng | en_US |
dc.title | VizieR Online Data Catalog: Radial velocities for the HD 3167 system (Christiansen+, 2017) | en_US |
dc.type | Database | - |
dc.identifier.doi | 10.26093/cds/vizier.51540122 | en_US |
dc.identifier.url | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/122 | en_US |
dc.relation.firstpage | J/AJ/154/122 | 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..51540122C | 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_2 Planetary systems sciences | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Database | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.orcid | 0000-0002-1742-7735 | - |
crisitem.author.orcid | 0000-0002-7504-365X | - |
crisitem.author.orcid | 0000-0002-9900-4751 | - |
Appears in Collections: | 4.06 Banche Dati |
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File | Description | Size | Format | |
---|---|---|---|---|
J AJ 154 122.pdf | ReadMe | 1.76 MB | Adobe PDF | View/Open |
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