Table 3
The maximuml values and area integrated FFP event rates in SN mode for 100% detection efficiency and assuming umax = 1.
| Lens mass | I-band (ground) | K-band (ground) | H-band (space) | |
|
|
||||
| max | 3700 | 15 000 | 26 000 | |
| Stellar | location |
|
|
|
| global | 58 000 | 450 000 | 710, 000 | |
|
|
||||
| max | 200 [–0.3%] | 850 [0.4%] | 1500 [1.4%] | |
| Jupiter | location |
|
|
|
| global | 3100 | 25 000 | 40 000 | |
|
|
||||
| max | 36 [1.6%] | 170 [–6.5%] | 340 [0.05%] | |
| Neptune | location |
|
|
|
| global | 460 | 4900 | 8900 | |
|
|
||||
| max | 1.1 [–22%] | 12 [–20%] | 68 [–4.9%] | |
| Earth | location |
|
|
|
| global | 18 | 350 | 2000 | |
Notes.The maximum rates are in units of events yr-1 deg-2 with the rate contrast in square brackets for FFPs. The hot-spot location is given in the Galactic coordinates (l,b). The global rates are in units of events yr-1 which covers the whole simulation area of 200 deg2. The errors of these maximum rates are all <1%, and a correction factor of 1.6 has been applied to the rate.
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