Table 2
Overview of the data sets and type of analysis performed by recent literature works (not based on RAVE data).
| No. stars | Type of analysis | References |
|
|
||
| 451 | Chemistry (HR spectra), kinematics | (1) |
| 176 | Chemistry (HR spectra), kinematics | (2) |
| 250 | Chemistry (HR spectra), kinematics | (3) |
| 1498 | Str mgren photometry, kinematics |
(4) |
| 306 | Chemistry (HR spectra), kinematics | (5) (2) (9) (11) |
| 412 | Kinematics (HR spectra) | (6) (7) (12) |
| 76 | Chemistry (HR spectra), kinematics | (8) |
| 102 | Chemistry (HR spectra), kinematics | (9) |
| 17 277 | Chemistry (LR spectra), kinematics | (10) |
| 23 767 | Chemistry (LR spectra), kinematics | (13) (14) |
|
|
||
| 38 805 | Kinematics (HR spectra) | present work |
Notes. Column one refers to the number of stars effectively used in the analysis of the thick/thin disk, not to the total number of stars produced by the database. HR/LR in column two stands for high/low spectral resolution respectively as specified in the papers of column three. For comparison we report the number of stars used in the present study in the last row.
References. (1) Neves et al. (2009); (2) Reddy et al. (2006); (3) Fuhrmann (2004); (4) Casagrande et al. (2011); (5) Navarro et al. (2011); (6) Moni Bidin et al. (2012a); (7) Moni Bidin et al. (2012b); (8) Afşar et al. (2012); (9) Bensby et al. (2005); (10) Lee et al. (2011); (11) Nissen & Schuster (2010); (12) Girard et al. (2006); (13) Bovy et al. (2012a); (14) Bovy et al. (2012b).
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