Table 9
Requirements and settings for deep VIRCAM with ultraVISTA and VIDEO on VISTA.
Filter | texp (s) | Nexp | Njitter | 〈Ndither〉 (per pix) | 〈ttot〉 (s) |
---|---|---|---|---|---|
VIDEO | |||||
Z | 50 | 1 | 10 | 1 | 500 |
Y | 30 | 2 | 8 | 1 | 480 |
J | 30 | 2 | 8 | 1 | 480 |
H | 10 | 6 | 7 | 1 | 420 |
KS | 10 | 6 | 7 | 2 | 840 |
UltraVISTA | |||||
Y | 60 | 2 | 30 | 1 | 3600 |
J | 30 | 4 | 30 | 1 | 3600 |
H | 10 | 6 | 30 | 1 | 1800 |
KS | 10 | 6 | 30 | 1 | 1800 |
Notes. Observation settings for each paw-print (texp, Nexp, Njitter) were used to compute the average number of dithers per-pixel on-sky (〈Ndither〉) that are needed to reach at least VIKING depth. We then randomly sampled 〈Ndither〉 dithers per pixel on-sky to construct our VIKING-like data in these deep fields. Subsequent further degradation of the photometry (in catalogue space) is needed to reach equivalent VIKING depths.
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