Remarks: (a) This value (Monet et al. 2003) was not used in the final proper motion due to its unreasonably small error of PM in declination, which makes it inconsistent with the measurements using the SuperCOSMOS Sky Survey in comparison to data from the New Technology Telescope (NTT) instrument Son of ISAAC (SSS-SofI). (b) From the Pre-main Sequence Stars Proper Motion Catalog (Ducourant et al. 2005).