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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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