Stellar Abundance for Galactic Archeology (SAGA) Database and Its Extension for Planet-hosting Stars Y. Katsuta1), T. Suda1,2), S. Yamada1), N. Nishimura3), Y. Komiya3), C, Ishizuka1,2), M.Y. Fujimoto1), M. Takada-Hidai4), Y. Gunji4), H. Toyosawa4) 1) Hokkaido University 2) Keele University 3) National Astronomical Observatory of Japan 4) Tokai University
1. SAGA database Collection of observed data http://saga.sci.hokudai.ac.jp/ http://www.astro.keele.ac.uk/saga/ Suda et al.(2008) Collection of observed data taken from the literature on the abundance analyses of metal-poor stars in our Galactic halo Compilation of adopted stellar parameters, derived abundance data, etc. using on-line Data Registration System Access to the data through web browsers Data retrieval system
Contents of SAGA(1) Stars: Complete collection of published data for stars of [Fe/H] ≦-2.5 1305 stars (3208 when duplications included; from 149 papers) Abundance data [X/Fe]: 19,185 [X/H]: 22,835 log ε: 22,835 Complete collection
Contents of the SAGA(2) Atmosphere Photometry Equivalent width Teff, log g, [Fe/H], vturb Photometry U, B, V, R, I, J, H, K Magnitudes Color indexes Equivalent width Equivalent width, log gf, Excitation Potential Isotopic ratio Binarity Referenced solar abundances
Contents of the SAGA(3) Observing logs: Object name, position, Observing date, Telescope, Resolution, Typical S/N, Exposure, Radial velocity Bibliography: Paper title, Author We can
Screen snapshot of SAGA start page http://saga.sci.hokudai.ac.jp Hyperlink to the data retrieval system
Range Specify X and Y axis Additional criteria
SAGA search result Retrieved values and available data. Choose one datum if two or more data are available. Atmospheric parameters adopted for each object and reference Choose to plot this object
Graph plot Automatically generated clickable map Link to quick preview of each object
Abundance distribution of this object Quick Preview of Data Link to SIMBAD Abundance distribution of this object
Extension to the metal-rich stars and planet hosts We have started to extend SAGA for the planet hosts and the metal-rich stars Compiled data 10 papers 940 (1463) stars 72 PHS, 868 non-PHS 12,156 [X/H] data UNDER CONSTRUCTION
[Fe/H] distribution □:non-PHS □:PHS Number [Fe/H] +:non-PHS △:PHS Teff [Fe/H] Well-known characteristics, high surface metallicity, of the PHSs can be seen
Vanadium abundances Sadakane+2002 Potential trend of overabundance of V (Sadakane et al. 2002, Bodaghee et al. 2006, Gilli 2006) [V/Fe] SAGA+ 1.0 +:non-PHS △:PHS -0.2 -0.5 0.5 [Fe/H]
Si abundances [Si/H] [Fe/H] [Fe/H] Clear overabundance (Robinson et al. 2006) Underabundance (Gonzalez & Laws 2007) Robinson+2006 SAGA+ [Fe/H]
Cross-reference data plot [Na/Si] values are internally processed by [Na/Fe] and [Si/Fe] [Na/Si] [Fe/H]
Summary & Future works SAGA database http://saga.sci.hokudai.ac.jp Easy to search, plot, and download data We have started to extend SAGA database into higher metallicity stars and planet host stars Some important data for metal-rich stars and planet hosts are to be installed in the future Stellar masses, Planet orbital parameters, Planet masses
The new database will Reveal the characteristics of planet host stars from the element abundances Reveal the whole history of the star formation and chemical evolution in our Galaxy from the extremely metal-poor stars to the super metal-rich stars Be open to the public in the near future
Ni and Ti abundances 662