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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
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/380/712
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-rw-r--r-- 1 cats archive 2232 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 43008 Mar 1 2008 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 11438 Mar 1 2008 tablea1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 3975 Mar 1 2008 tableb1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1680 Mar 1 2008 tablec1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2851 Mar 1 2008 tabled1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1321 Mar 1 2008 tablee1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2988 Jan 5 2008 tablef1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/MNRAS/380/712 ZYJHK photometry in Pleiades (Lodieu+, 2007)
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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
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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.