Table 1: Source widths (half intensity) and flux density of the flare emission at $\sim$ 11:10 UT (extended phase). Note the significantly larger diameter at the higher frequency.
Frequency Beamwidth $\Theta_{{\rm meas}}$ $\Theta_{{\rm source}}$ Flux density

[GHz] [arcsec] [arcsec] [arcsec] [sfu]

230 $117\pm 7$ 124 $42\pm20$ 112⁺⁵_-4

345 $88\pm 5$ 112 $70\pm6$ 196 ⁺¹⁴_-9

**Table 1:** Source widths (half intensity) and flux density of the flare emission at $\sim$ 11:10 UT (extended phase). Note the significantly larger diameter at the higher frequency.
Frequency	Beamwidth	$\Theta_{{\rm meas}}$	$\Theta_{{\rm source}}$	Flux density
[GHz]	[arcsec]	[arcsec]	[arcsec]	[sfu]
230	$117\pm 7$	124	$42\pm20$	112⁺⁵_-4
345	$88\pm 5$	112	$70\pm6$	196 ⁺¹⁴_-9

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