Table 3
Integration times (in seconds) per visit.
| Filter | wide | deep |
|
|
||
| g | 400 | 1600 |
| r | 400 | 1600 |
| i | 500 | 1600 |
| z | 700 | 2400 |
|
|
||
| y | 650 | 1800 |
| J | 650 | 2400 |
| H | 650 | 3000 |
Notes. Integration time proposed for the wide and deep supernova surveys with a 5 days cadence. The wide and deep surveys have to cover respectively 100 and 20 pointings. The CCD type we simulate has a modest quantum efficiency in the z band, which drives exposure times up in this band.
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