Table A.2
The lower detection limits for MuSCAT.
| Filter | FWHM [min] | Amplitude | Ebol[1030erg] |
|---|---|---|---|
| g | [5.4, 5.76] | [0.059, 0.075] | 0.74 ± 0.05 |
| r | [4.32, 4.68] | [0.03, 0.04] | 3.12 ± 0.18 |
| i | [3.96, 4.32] | [0.035, 0.053] | 8.13 ± 0.45 |
| zs | [2.02,2.16] | [0.04, 0.05] | 8.48 ± 0.81 |
The lower detection limits in FWHM and amplitude for all filters associated with the bolometric energy adopting a blackbody temperature of 7000 K. Even though the adopted photometric scatter is lower in zs and i, the detection limits in g and r are lower in terms of energy, because the flare flux from a 7000 K is peaked closer to the blue than the red light.
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