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5 catalogs found
  
J/ApJ/764/78
  Oxygen abundances in nearby FGK stars (Ramirez+, 2013)
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    J/ApJ/764/78/stars(c)Kinematic data, atmospheric parameters, ages, masses and oxygen abundances of the nearby FGK stars (tables 2, 4, 5 and 6) (825 rows)
    J/ApJ/764/78/table3Iron Line List (144 rows)
  
J/ApJ/860/109
  Keck HIRES obs. of 245 subgiants (retired A stars) (Ghezzi+, 2018)
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    J/ApJ/860/109/subgiants(c)Atmospheric, broadening and evolutionary parameters of the subgiant sample and Galactic UVW space velocities and photometric effective temperatures (Tables 1, 3, 5, 6, 7 and 8) (247 rows)
    J/ApJ/860/109/table2List of Fe I and Fe II lines (176 rows)
  
J/ApJ/871/193
  A combined Chandra & LAMOST study of stellar activity (He+, 2019)
timeSerie
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    J/ApJ/871/193/stars(c)LAMOST (Table 2) and key results (Table 3) for the stars in our sample[timeSerie] (484 rows)
    J/ApJ/871/193/table1X-ray information for the 484 stars in our sample (1084 rows)
    J/ApJ/871/193/table4Stars with Hα emission lines in our sample (24 rows)
    J/ApJ/871/193/table5Stars with X-ray flares in our sample (12 rows)
  
J/A+A/275/101
  Chemical evolution of the galactic disk I. (Edvardsson+ 1993)
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    J/A+A/275/101/stars(c)Fundamental data and chemical abundances of 14 species for the programme stars (189 rows)
    J/A+A/275/101/table8Atomic line data and solar equivalent widths (86 rows)
  
J/PASJ/59/335
  Properties of 160 F-K disk dwarfs/subgiants (Takeda+, 2007)
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    J/PASJ/59/335/catalog(c)Results on program stars: astrophysical parameters, abundances, kinematic parameters (tables 1, E1, E2 and E3 of paper) (160 rows)
    J/PASJ/59/335/mabundAverage abundances (from tablee3) (2552 rows)
    J/PASJ/59/335/xhcorCorrections on the final (line-averaged) results of [ScII/H], [VI/H], [MnI/H] and [CoI/H] caused by inclusion of the hyper-fine splitting effect for each of the relevant lines (from tablee4) (569 rows)
    J/PASJ/59/335/lgf*Wavelength and the loggf data of each hyper-fine splitting (hfs) component (from tablee4) (Note) (365 rows)
    J/PASJ/59/335/difResults of abundance corrections caused by inclusion of the hyper-fine splitting (hfs) effect for the relevant line (from tablee4) (2824 rows)

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       (c)  indicates tables which contain celestial coordinates 
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