Table 2
Characteristics of the flares observed by CARMA, APEX, the VLT, and Chandra.
| Spectral | Date | Flare start | Flare stop | FWZP | FWHM | Aperture | Flare | Offset | |
| domain | (min) | (min) | Size | state | |||||
| (arcsec) | |||||||||
|
|
|||||||||
| 100 GHz | 18 May 2009 | 10:10 ± 10 min | >12:13 | >150 | >140 | 3 | 0.24 ± 0.05 Jy | 0.9 Jy | |
| 345 GHz | 18 May 2009 | 09:30 ± 20 min | >12:05 | >150 | 120 ± 10 | 19 | 0.85 ± 0.15 Jy | 2.9 Jy | |
| NIR | 18 May 2009 | 09:10 ± 10 min | >10:20 | >70 | >50 | 0.06 | 10 ± 0.5 mJy | 1.0 mJy | |
| X-ray | 18 May 2009 | 09:10 ± 10 min | 11:10 ± 10 min | 100 ± 10 | 60 ± 10 | 1.50 | 40 ± 5 nJy | 20 nJy | |
Notes. For all bands, we list the estimated start and stop times, the full width at zero power (FWZP) and FHWM values, as well as the peak and quiescent flux densities. The NIR refers to the 2.2 μm Ks-band. The X-ray refer to the 2 − 8 keV band. In the radio, the aperture size refers to the FWHM of the synthesized (CARMA) and primary beam (APEX).
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