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Table 2
Upper limits on the detection of a synthetic MIR flare, as well as the corresponding limits on the MIR-NIR spectral slope and particle index.
| Night (July 2007) | 20 | 22 | 23 |
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| On state time interval/s [UT] | 23:07.18 to 00:13:30, | 0:23:12 to 0:39:48, | 5:34:06 to 5:49:0, |
| & 00:50:54 to 2:44:54 | & 1:05:06 to 1:24:48, | & 6:04:30 to 6:19:30 | |
| & 1:57:00 to 2:00:00 | |||
| Off state time interval/s [UT] | 00:17:30 to 00:35.06 | 0:41:06 to 1:03:48, | 5:34:06 to 5:49:06, |
| & 1:26:12 to 1:55:36, | & 6:04:30 to 6:19:30 | ||
| & 2:01:12 to 2:39:12 | |||
| Upper limit for transient emission | 24.2 | 22.4 | 31.2 |
| (dereddened with A8.59 μm = 1.6 ± 0.5) | |||
| Average NIR flux (wavelength) | 2.0 (Ks) | 3.4 (L′) | 4.1 (Ks) |
| on state time intervals | |||
| Lower limit on the νLν spectral index | β > − 0.80 | β > − 1.3 | β > − 0.46 |
| (νLν ∝ νβ) | |||
| Upper limit on the particle index, p | p < 4.6 | p < 5.6 | p < 4.0 |
| (N(γ) ∝ γ − p) | |||
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