Table 2
LI efficiencies for detecting chromatic perturbations in HM single and CC binary microlensing events and the properties of these events.
| ϵl | ϵh |  |
 |
 |
 |
f100 | f200 | f500 | No. | |
|---|---|---|---|---|---|---|---|---|---|---|
| [%] | [%] | (mmag) | (mmag) | [%] | [%] | [%] | ||||
| HM microlensing | ||||||||||
| BL | 61.1 | 48.7 | 94.2 | 105.0 | –2.31 | 0.75 | 76.5 | 38.2 | 10.8 | 48 955 |
| BL & LD | 62.2 | 50.0 | 98.2 | 112.5 | –2.31 | 0.75 | 75.4 | 37.6 | 11.1 | 58 329 |
| BL & LD & CGP | 64.2 | 53.1 | 58.7 | 79.1 | –2.31 | 0.81 | 75.2 | 35.9 | 7.7 | 30 932 |
| BL & LD & SS | 62.7 | 51.0 | 97.6 | 111.0 | –2.31 | 0.75 | 75.2 | 37.7 | 11.2 | 1721 |
| BL & GD | 62.2 | 53.7 | 35.7 | 35.9 | –2.30 | 0.94 | 93.2 | 43.6 | 8.6 | 3644 |
| CC microlensing | ||||||||||
| BL | 26.1 | 17.3 | 97.9 | 111.1 | –0.75 | 0.74 | 19.1 | 3.5 | 0.1 | 6350 |
| BL & LD | 30.8 | 21.7 | 106.6 | 134.2 | –0.75 | 0.77 | 18.7 | 3.1 | <0.07 | 1333 |
| BL & LD & CGP | 33.2 | 22.7 | 108.8 | 138.1 | –0.71 | 0.78 | 17.9 | 2.9 | <0.1 | 712 |
| BL & LD & SS | 35.8 | 26.8 | 104.9 | 125.6 | –0.72 | 0.80 | 14.7 | 1.1 | <0.2 | 584 |
| BL & GD | 48.2 | 40.9 | 51.7 | 53.9 | –0.67 | 0.93 | 11.3 | 0.8 | 0.8 | 433 |
Notes. BL, LD, CGP, SS, and GD refer to the blending, limb-darkening, close-in giant planet companion, stellar spot, and gravity-darkening effects, respectively. 
and
are the average values of maximum chromatic deviations in detectable (simulated) microlensing events. Also, f100, f200 and f500 represent the fraction of the simulated events with detectable chromatic perturbations, and with the maximum magnification factor higher than 100, 200, and 500, respectively. The last column (No.) reports the number of simulated events with detectable perturbations.
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