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Table 1.

Photometric dataset used in this paper.

Reference Filter λeff Δλeff CAB texp m(3σ) m(50%) Seeing Area (> 50%)
(nm) (Å) (mag) (ksec) (mag) (mag) (″) (arcmin2)
CFHTLS-D3 u* 382 544 0.312 76.6 28.52 26.97 0.89 3224
CFHTLS-D3 g 490 1309 −0.058 79.6 28.94 26.79 0.84 3224
CFHTLS-D3 r 625 1086 0.176 142.8 28.57 26.30 0.78 3224
CFHTLS-D3 i 766 1330 0.404 249.4 28.24 25.95 0.76 3224
CFHTLS-D3 z 884 1033 0.525 175.4 27.09 25.46 0.69 3224
WUDS Y 1027 1077 0.632 44.9 26.78 26.26 0.63 392
WUDS J 1256 1531 0.949 50.4 26.69 26.17 0.60 396
WIRDS J 26.3 25.80 24.80 0.60 437
WUDS H 1636 2734 1.390 39.6 26.06 25.61 0.55 477
WIRDS H 15.5 25.73 24.80 0.55 681
WUDS Ks 2154 3071 1.862 25.9 25.93 25.46 0.56 450
WIRDS Ks 17.5 25.59 24.63 0.56 547

Notes. Information given in this table: reference field, filter identification, filter effective wavelength, filter width, AB correction (mAB = mVega + CAB), total exposure time, 3σ limiting magnitudes (within 1.3″ diameter aperture), 50% completeness level for point-like sources (in the regions with > 50% of the total exposure time), average seeing for the final stack, and total area covered with > 50% total exposure time.

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