To select my sample to study the rest frame NIR luminosity function of high z galaxies.

1. Run SExtractor on K band ISAAC image archive and make source list.

2. Select samples with magnitude cut in K band

3. Cross-correlate them with COMBO-17 catalog in GOODS/CDF-S

GOODS/CDF-S has been observed by ESO/ISAAC with imaging mode.

ESO archive

1. J(21 tiles) and Ks(23 tiles) band images are available

2. Each tile is 2.5 arcmin by 2.5 arcmin and pixel scale is 0.15 arcsec. Therefore each tile is 1000 by 1000 pixel image.


~ by ilsangyoon on October 1, 2008.

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