Photometric redshifts for the CFHTLS T0004 deep and wide fields

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Volume 500 / No 3 (June IV 2009)

A&A, 500 3 (2009) 981-998

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Table 4:

Star/galaxy selection results, the table shows the galaxy incompleteness (Inc.) and the star contamination (Cont.) for the W1 field, with a large PSF size and the highly star crowded field, W4. ``Stars'' represent the intrinsic proportion of stars in the field.
Deep ( $i'_{\rm AB} < 24$ )
Field	$r_{\rm hlimit}$	Stars	Inc.	Cont.
D1	2.7	11.0%	0.80%	1.1%
W1 ( $i'_{\rm AB} < 22.5$ )
Field	$r_{\rm hlimit}$	Stars	Inc.	Cont.
022539-050800	3.1	23.5%	3.1%	0.4%
022539-041200	2.8	18.8%	2.3%	0.9%
022929-041200	3.1	20.6%	2.9%	0.7%
All	3.0	19.0%	2.6%	1.0%
W4 ( $i'_{\rm AB} < 22.5$ )
Field	$r_{\rm hlimit}$	Stars	Inc.	Cont.
221318-003100	2.2	57.2%	0.6%	7.7%
221318+002300	2.1	52.5%	0.0%	9.0%
221318+011900	2.6	44.7%	0.8%	2.5%
221706-003100	2.7	53.2%	1.0%	7.9%
221706+002300	2.3	51.9%	1.0%	6.4%
221706+011900	1.9	51.7%	0.4%	7.3%
222054-003100	2.5	52.6%	1.0%	6.1%
222054+002300	2.4	52.8%	1.2%	7.3%
222054+011900	2.1	45.8%	0.3%	6.3%
All	2.3	51.8%	0.8%	6.9%

Source LaTeX | All tables | In the text

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