Near-infrared and WISE photometry of selected Pleiades candidates with two or more proper motion measurements. Symbols are as in Fig. 5. The field “young” L and T dwarfs (Cruz et al. 2009; Delorme et al. 2012; Liu et al. 2013; Kuzuhara et al. 2013; Naud et al. 2014) are denoted with open diamonds. The star symbols stand for the bcde planets orbiting HR 8799 (Marois et al. 2008, 2010). The solid line corresponds to the mean observed sequence of field late-M, L, and T dwarfs (Dupuy & Liu 2012) moved to 133.5 pc. All field objects are also taken to the Pleiades distance. Spectral types and objects from the literature are labeled. The WISE photometry of J2149−0403 is quite uncertain; Delorme et al. (2012) argued that the W2 detection lied at the exact expected position, while the W1 detection was slightly offset. Masses are given in Jovian units color-coded as in Fig. 6.