Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections

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Table 2

Characteristics of the two drifting Stokes V stellar bursts.

Burst ID	Time of arrival (t₀) (MJD)	Burst flux density (S₀) (mJy)	Burst width (Δt)^a (s)	Burst drift delay (a) (min)	Burst drift rate (a) (MHz s⁻¹)
B20^b	${57525.924011}_{- 0.000001}^{+ 0.000001}$ $\[57525.924011_{-0.000001}^{+0.000001}\]$	$- {71.4}_{- 1.7}^{+ 1.7}$ $\[-71.4_{-1.7}^{+1.7}\]$	${62.3}_{- 0.1}^{+ 0.1}$ $\[62.3_{-0.1}^{+0.1}\]$	${0.998}_{- 0.004}^{+ 0.004}$ $\[0.998_{-0.004}^{+0.004}\]$	$- {0.801}_{- 0.003}^{+ 0.003}$ $\[-0.801_{-0.003}^{+0.003}\]$
B21	${58552.202540}_{- 0.000178}^{+ 0.000111}$ $\[58552.202540_{-0.000178}^{+0.000111}\]$	$- {4.5}_{- 1.3}^{+ 1.4}$ $\[-4.5_{-1.3}^{+1.4}\]$	$63_{- 11}^{+ 31}$ $\[63_{-11}^{+31}\]$	${13.3}_{- 0.5}^{+ 0.4}$ $\[13.3_{-0.5}^{+0.4}\]$	$- {0.060}_{- 0.002}^{+ 0.002}$ $\[-0.060_{-0.002}^{+0.002}\]$

Notes. ^aWidth at a fixed frequency channel, or the sweep-corrected burst width.

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