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

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D2 u−band (25% best−seeing images)<br />

D2 u−band (85% best−seeing images)<br />

3.0<br />

ul ur ul ur<br />

3.0<br />

Dec [deg]<br />

2.5<br />

2.0<br />

cc<br />

Dec [deg]<br />

2.5<br />

2.0<br />

cc<br />

1.5<br />

ll<br />

lr<br />

1.5<br />

ll<br />

lr<br />

N<br />

151.0<br />

150.5<br />

150.0<br />

149.5<br />

149.0<br />

151.0<br />

150.5<br />

150.0<br />

149.5<br />

149.0<br />

RA [deg]<br />

RA [deg]<br />

E<br />

Figure 46: Locations of u ∗ -band pointings used to produced the D2-u ∗ stack. The colored squares represent the<br />

different MegaCam fields, and the colored points are the center positions of each CFHTLS and COSMOS images<br />

that are combined to produce the D-25-u ∗ and D-85u ∗ images. The dark squares are located at the D2 center<br />

position and outline the contour of the final D2-u ∗ . The D2-u ∗ characteristics quoted in Tables 18 and 19 only<br />

refer to the central regions delimited by the black squares. The bold squares show the central region containing<br />

all exposures. The stacks inside this narrow region are extremely deep: 51012 s. for D2-u ∗ -25, and 142970 s. for<br />

D2-u ∗ -85.<br />

82

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