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  Gaia DR1 catalogue is available in VizieR and by TAP
3 catalogs found
  J/ApJS/218/25
 Abundances in PNe. III: Se and Kr (Sterling+, 2015)
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2015ApJS..218...25S
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    J/ApJS/218/25/pne(c)Observational data references, model input parameters and comparison of modeled Se and Kr abundances for the 15 PNe exhibiting emission lines from multiple Kr ions (tables 1-3, 7) (Note) (16 rows)
    J/ApJS/218/25/table4Predicted vs. observed diagnostics and line intensities (1147 rows)
    J/ApJS/218/25/table14(c)Se and Kr abundances relative to H, O, and Ar (151 rows)
    J/ApJS/218/25/refsReferences (54 rows)
  J/A+AS/137/157
 O III recombination coefficients (Kisielius+, 1999)
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1999A&AS..137..157K
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    J/A+AS/137/157/table1Indices n1 and energy levels of the 4f and 5g states in O2+ ions (24 rows)
    J/A+AS/137/157/table2Wavelengths in air, electric dipole transition probabilities A(n1,n2) and branching ratios b(n1,n2) for the 5g-4f transitions in O2+ ions (83 rows)
    J/A+AS/137/157/table3Fitting coefficients for the direct recombination coefficients adir to the 5g levels of O2+ (12 rows)
    J/A+AS/137/157/table4Fractions of the cascade contributions from each series to the recombination coefficients of the 5g levels of O2+ (12 rows)
    J/A+AS/137/157/table5Calculated and fitted effective recombination coefficients for the 5g levels of O2+ at the electron temperatures T=10000K and T=20000K and the electron density N=103cm–3. (12 rows)
  J/A+AS/147/111
 Iron Project. XLIV. Fe VI. (Chen+, 2000)
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2000A&AS..147..111C
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    J/A+AS/147/111/table1The 80 fine structure levels corresponding to the 34 LS terms included in the calculations and their observed energies (Ry) in Fe VI (Sugar & Corliss, 1985, Cat. VI/74) (80 rows)
    J/A+AS/147/111/table2Weighted dipole allowed E1 oscillator strengths gfL, gfV in the length and velocity formulations, and the Einstein A-coefficients AL in the length formulation. (867 rows)
    J/A+AS/147/111/table3Comparison of the electric quadrupole (E2) and magnetic dipole (M1) transition probabilities between the first 19 levels of Fe VI in s–1 among the present calculation by SUPERSTRUCTURE, calculations by Garstang et al. (1978ApJ...222..384G) and by Nussba (129 rows)
    J/A+AS/147/111/table4Electric quadrupole (E2) and magnetic dipole (M1) transition probabilities between the first 80 levels of Fe VI in s–1 in the present calculation by SUPERSTRUCTURE. (1101 rows)
    J/A+AS/147/111/table6Line intensity ratios for transitions relative to λ5146Å (8-3: 4F7/2-2G7/2), with Teff=150000K. (177 rows)

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