Stellar Sequence (PDR2)

The color offset and scatter around the stellar sequence on a color-color diagram are computed as part of the validation tests. Only a few plots are shown in the data release paper, but the plots for all the fields are available below. In each field, the top row shows the color offset and bottom row shows the color scatter. Most fields have good colors, but there are small regions where the photometry is somewhat poor. The sharp borders often seen in the riz plots are due to the i/i2 difference (see the data release paper for details).

• Wide

DUD-COSMOS

g, r, i r, i, z i, z, y N387, g, r r, N816, z i, N921, y
offset
scatter

DUD-SXDS

g, r, i r, i, z i, z, y N387, g, r r, N816, z i, N921, y
offset
scatter

D-ELAIS-N1

g, r, i r, i, z i, z, y N387, g, r r, N816, z i, N921, y
offset
scatter

D-DEEP2-F3

g, r, i r, i, z i, z, y N387, g, r r, N816, z i, N921, y
offset
scatter

Wide

W-WIDE01H

g, r, i r, i, z i, z, y
offset
scatter

W-XMM-LSS

g, r, i r, i, z i, z, y
offset
scatter

W-GAMA09H

g, r, i r, i, z i, z, y
offset
scatter

W-WIDE12H

g, r, i r, i, z i, z, y
offset
scatter

W-WIDE15H

g, r, i r, i, z i, z, y
offset
scatter

W-HECTOMAP

g, r, i r, i, z i, z, y
offset
scatter

W-VVDS

g, r, i r, i, z i, z, y
offset
scatter

W-VVDS contd.

g, r, i r, i, z i, z, y
offset
scatter