Table 8: Emission properties of the radio flare events from Sgr A*. In the case of a flare event detection we we give the estimated peak flux density, the full zero start and stop times, the full zero width at the corresponding zero points (FWZP) and the full width at half maximum of the flare events. For the VLA we give the excess flux density over the mean flux density measured on 06 and 08 July.
Observing IR Flare $\lambda$ Start Stop FWZP FWHM peak flux

ID ID (min) (min) (Jy)

SMA-A SMA1 890 $\mu$ m 05 Jul. 07:00 05 Jul. 10:30 210 120 3.5

SMA-A SMA2 890 $\mu$ m 05 Jul. 11:00 $\ge$ 05 Jul. 12:10 - - $\ge$ 3.2

SMA-B SMA3 890 $\mu$ m 06 Jul. 07:45 06 Jul. 10:00 135 <60 3.4

SMA-C SMA4 890 $\mu$ m <07 Jul. 06:00 07 Jul. 08:00 - - $\ge$ 3.5

SMA-C SMA5 890 $\mu$ m 07 Jul. 08:00 $\ge$ 07 Jul. 12:00 - - 3.3

VLA-B VLA1 7 mm <07 Jul. 04:40 >07 Jul. 08:50 >0.5

**Table 8:** Emission properties of the radio flare events from Sgr A*. In the case of a flare event detection we we give the estimated peak flux density, the full zero start and stop times, the full zero width at the corresponding zero points (FWZP) and the full width at half maximum of the flare events. For the VLA we give the excess flux density over the mean flux density measured on 06 and 08 July.
Observing	IR Flare	$\lambda$	Start	Stop	FWZP	FWHM	peak flux
ID	ID				(min)	(min)	(Jy)
SMA-A	SMA1	890 $\mu$ m	05 Jul. 07:00	05 Jul. 10:30	210	120	3.5
SMA-A	SMA2	890 $\mu$ m	05 Jul. 11:00	$\ge$ 05 Jul. 12:10	-	-	$\ge$ 3.2
SMA-B	SMA3	890 $\mu$ m	06 Jul. 07:45	06 Jul. 10:00	135	<60	3.4
SMA-C	SMA4	890 $\mu$ m	<07 Jul. 06:00	07 Jul. 08:00	-	-	$\ge$ 3.5
SMA-C	SMA5	890 $\mu$ m	07 Jul. 08:00	$\ge$ 07 Jul. 12:00	-	-	3.3
VLA-B	VLA1	7 mm	<07 Jul. 04:40	>07 Jul. 08:50			>0.5

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