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Table 3.
Summary of the numbers of Pleiades sources from earlier studies recovered in our full Gaia sample (i.e. up to three times the tidal radius of the cluster).
Method | in Gaia | Kinematic | in Rtidal | Comments |
---|---|---|---|---|
Hambly et al. (1993) | 429/440 | 385 | 334 | Photographic plates |
Zapatero Osorio et al. (1997b) | 3/10 | 1 | 2 | CCD-based R, I survey |
Stauffer et al. (1998b) | 16/20 | 12 | 9 | Lithium depletion boundary; MHO targets |
Bouvier et al. (1998) | 19/26 | 13 | 8 | Proper motions in Moraux et al. (2001) |
Moraux et al. (2003) | 103/109 | 93 | 78 | Brown dwarfs and IMF |
Deacon & Hambly (2004) | 882/916 | 776 | 642 | Astrometry and photometry of photographic plates |
Bihain et al. (2006) | 14/34 | 11 | 6 | Deep I + J survey of 1.8 deg2 |
Stauffer et al. (2007) | 1361/1416 | 1129 | 928 | Compilation of earlier studies (their Table 1) |
Casewell et al. (2007) | 8/23 | 7 | 2 | Deep CFH12K survey combined with UKIDSS |
Lodieu et al. (2007) | 82/116 | 69 | 46 | UKIDSS GCS DR1 combined with 2MASS |
Lodieu et al. (2012b) | 1176/1314 | 863 | 700 | Selection in UKIDSS GCS DR9 |
Zapatero Osorio et al. (2014a) | 5/24 | 4 | 2 | See Zapatero Osorio et al. (2014b) for spectroscopy |
Bouy et al. (2015) | 1775/2010 | 1421 | 1070 | See also Bouy et al. (2013) and Sarro et al. (2014) |
Olivares et al. (2018b) | 1960/2152 | 1467 | 1097 | p ≥ 0.75 from Bayesian hierarchical model |
Gaia Collaboration (2018a) | 1326/1326 | 1295 | 1087 | Gaia DR2 |
Notes. We have 106, 495, 1248, and 2195 kinematic member candidates in 3.1, 4.5, 11.6, and 34.8 pc, respectively.
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