J/MNRAS/380/712      ZYJHK photometry in Pleiades                (Lodieu+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table4.dat tablea1.dat table[bcde]1.dat tablef1.dat
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/MNRAS/380/712

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Beginning of ReadMe : J/MNRAS/380/712 ZYJHK photometry in Pleiades (Lodieu+, 2007) ================================================================================ A wide deep infrared look at the Pleiades with UKIDSS: new constraints on the substellar binary fraction and the low-mass initial mass function. Lodieu N., Dobbie P.D., Deacon N.R., Hodgkin S.T., Hambly N.C., Jameson R.F. <Mon. Not. R. Astron. Soc., 380, 712-732 (2007)> =2007MNRAS.380..712L ================================================================================ ADC_Keywords: Clusters, open ; Photometry, infrared ; Proper motions Keywords: techniques: photometric - stars: low-mass, brown dwarfs - stars: luminosity function, mass function - open clusters and associations: individual: Pleiades - infrared: star Abstract: We present the results of a deep wide-field near-infrared survey of 12deg^2^ of the Pleiades conducted as part of the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) Galactic Cluster Survey (GCS). We have extracted over 340 high-probability proper motion (PM) members down to 0.03M_sun_ using a combination of UKIDSS photometry and PM measurements obtained by cross-correlating the GCS with data from the Two Micron All Sky Survey, the Isaac Newton Telescope and the Canada-France-Hawaii Telescope. Additionally, we have unearthed 73 new candidate brown dwarf (BD) members on the basis of five-band UKIDSS photometry alone. We have identified 23 substellar multiple system candidates out of 63 candidate BDs from the (Y-K, Y) and (J-K, J) colour-magnitude diagrams, yielding a binary frequency of 2844 per cent in the 0.075-0.030M_sun_ mass range.