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Documentation [PDF] - Canada France Hawaii Telescope ...

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stacks made with the y-(i.MP9702) filter. The y stacks are listed in Tables 31 and quoted in Tables 15<br />

and 16. All Deep fields comprise both i and y-band stacks, but the i stacks contain much more images<br />

and are much deeper.<br />

The two input-ldac and output-ldac catalogues as well as the chi2-RSC catalogue contain the 75 parameters<br />

described in Table 28 to 30. However, they do not have the same input nor the same of output<br />

parameter values. Some of them are vectors, so the number of entries are also not the same and can be<br />

much higher than 75. In particular, they do not have the same detection threshold, or the same number<br />

of MAG_APER aperture magnitudes. Columns of catalogues with both the ’.cat’ or the ’.ldac’<br />

extensions are defined in the ’.param’ files. For the Wide survey, there are 77 columns in the .ldac<br />

catalogues, 181 columns in the chi2-RSC, 24 (resp 30) in the merged MAG_AUTO (resp MAG_SNLS) M-SC<br />

catalogues, 536 in the merged MAM-SC catalogues and 827 in the patch-merged catalogues WPM-SC.<br />

All images have a new magnitude ZP set to 30 AB magnitudes. The magnitudes of objects in the final<br />

stacks are computed as follows:<br />

m = 30 − 2.5 log(counts) . (19)<br />

It is important to realise that the .cat catalogues are produced using specific selection criteria or filters<br />

selected by TERAPIX from past experience and after discussions with experienced users and the CFHTLS<br />

Steering Group. They are certainly not suitable for all scientific goals. Please examine the configuration<br />

and parameter list files and check they meet your needs. In case different selections or configuration<br />

parameters are needed, it may be better to produce a new and more suitable catalogue, or to produce a<br />

new chi2 image. TERAPIX can provide specific help to users who want to produce their own images or<br />

catalogues.<br />

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