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Table C.3
Stellar parameters, ages, abundance ratios, uncertainties, and kinematical properties for the 714 stars.
| Column | Label | Unit | Comment |
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| (1) | HIP | ||
| (2) | Spec | Spectrograph | |
| (3) | Teff | K | |
| (4) | ϵ(Teff) | K | |
| (5) | log g | ||
| (6) | ϵ(log g) | ||
| (7) | ξt | km s-1 | |
| (8) | ϵ(ξt) | km s-1 | |
| (9) | log ε(Fe i) | Absolute abundance from Fe i lines | |
| (10) | log ε(Fe ii) | Absolute abundance from Fe ii lines | |
| (11) | mass | sun | Best mass |
| (12) | massl | sun | Lower limit on mass |
| (13) | massu | sun | Upper limit on mass |
| (14) | Age | Gyr | Best age |
| (15) | Agel | Gyr | Lower limit on age |
| (16) | Ageu | Gyr | Upper limit on age |
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| (17) | [Fe/H] | Sun | |
| (18) | [O/Fe] | Sun | |
| (19) | [Na/Fe] | Sun | |
| (20) | [Mg/Fe] | Sun | |
| (21) | [Al/Fe] | Sun | |
| (22) | [Si/Fe] | Sun | |
| (23) | [Ca/Fe] | Sun | |
| (24) | [Ti/Fe] | Sun | |
| (25) | [Cr/Fe] | Sun | |
| (26) | [Ni/Fe] | Sun | |
| (27) | [Zn/Fe] | Sun | |
| (28) | [Y/Fe] | Sun | |
| (29) | [Ba/Fe] | Sun | |
| (30) | ϵ [Fe/H] | Abundance ratio uncertainty | |
| (31) | ϵ [O/Fe] | ||
| (32) | ϵ [Na/Fe] | ||
| (33) | ϵ [Mg/Fe] | ||
| (34) | ϵ [Al/Fe] | ||
| (35) | ϵ [Si/Fe] | ||
| (36) | ϵ [Ca/Fe] | ||
| (37) | ϵ [Ti/Fe] | ||
| (38) | ϵ [Cr/Fe] | ||
| (39) | ϵ [Ni/Fe] | ||
| (40) | ϵ [Zn/Fe] | ||
| (41) | ϵ [Y/Fe] | ||
| (42) | ϵ [Ba/Fe] | ||
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| (43) | [Ti/H] | Sun | |
| (44) | [O/Ti] | Sun | |
| (45) | [Na/Ti] | Sun | |
| (46) | [Mg/Ti] | Sun | |
| (47) | [Al/Ti] | Sun | |
| (48) | [Si/Ti] | Sun | |
| (49) | [Ca/Ti] | Sun | |
| (50) | [Cr/Ti] | Sun | |
| (51) | [Ni/Ti] | Sun | |
| (52) | [Fe/Ti] | Sun | |
| (53) | [Zn/Ti] | Sun | |
| (54) | [Y/Ti] | Sun | |
| (55) | [Ba/Ti] | Sun | |
| (56) | ϵ [Ti/H] | Abundance ratio uncertainty | |
| (57) | ϵ [O/Ti] | ||
| (58) | ϵ [Na/Ti] | ||
| (59) | ϵ [Mg/Ti] | ||
| (60) | ϵ [Al/Ti] | ||
| (61) | ϵ [Si/Ti] | ||
| (62) | ϵ [Ca/Ti] | ||
| (63) | ϵ [Cr/Ti] | ||
| (64) | ϵ [Ni/Ti] | ||
| (65) | ϵ [Fe/Ti] | ||
| (66) | ϵ [Zn/Ti] | ||
| (67) | ϵ [Y/Ti] | ||
| (68) | ϵ [Ba/Ti] | ||
| (69) | N(Fe i) | Number of lines used | |
| (70) | N(Fe ii) | ||
| (71) | N(O i) | ||
| (72) | N(Na i) | ||
| (73) | N(Mg i) | ||
| (74) | N(Al i) | ||
| (75) | N(Si i) | ||
| (76) | N(Ca i) | ||
| (77) | N(Ti i) | ||
| (78) | N(Ti ii) | ||
| (79) | N(Cr i) | ||
| (80) | N(Cr ii) | ||
| (81) | N(Ni i) | ||
| (82) | N(Zn i) | ||
| (83) | N(Y ii) | ||
| (84) | N(Ba ii) | ||
| (85) | σ(Fe i) | 1-σ line-to-line dispersion | |
| (86) | σ(Fe ii) | ||
| (87) | σ(O i) | ||
| (88) | σ(Na i) | ||
| (89) | σ(Mg i) | ||
| (90) | σ(Mg i) | ||
| (91) | σ(Si i) | ||
| (92) | σ(Ca i) | ||
| (93) | σ(Ti i) | ||
| (94) | σ(Ti ii) | ||
| (95) | σ(Cr i) | ||
| (96) | σ(Cr ii) | ||
| (97) | σ(Ni i) | ||
| (98) | σ(Zn i) | ||
| (99) | σ(Y ii) | ||
| (100) | σ(Ba ii) | ||
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| (101) | π | mas | Hipparcos plx |
| (102) | σπ | mas | plx uncertainty |
| (103) | d | kpc | Distance |
| (104) | l | deg | Galactic longitude |
| (105) | b | deg | Galactic latitude |
| (106) | ULSR | km s-1 | |
| (107) | VLSR | km s-1 | |
| (108) | WLSR | km s-1 | |
| (109) | Rmin | kpc | |
| (110) | Rmax | kpc | |
| (111) | zmax | kpc | |
| (112) | e | ||
| (113) | LZ | ||
| (114) | E/ELSR | Total energy normalised to the LSR | |
| (115) | TD/D | ||
| (116) | TD/H | ||
| (117) | Her/TD | ||
| (118) | Her/D | ||
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| (119) | Teff (u.i.b) | K | Un-corrected ion.bal temp |
| (120) | log g (u.i.b) | Un-corrected ion.bal grav | |
| (121) | Teff (hip) | K | Hipparcos temp |
| (122) | log g (hip) | Hipparcos grav | |
| (123) | log ε(Fe i) (hip) | Absolute abundance using Hipparcos plx | |
| (124) | log ε(Fe ii) (hip) | Absolute abundance using Hipparcos plx | |
Notes. The table is only available in electronic form at the CDS.
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