Recurring millimeter flares as evidence for star-star magnetic reconnection events in the DQ Tauri PMS binary system

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Table 3:

Millimeter track and light curve statistics.
UT date	Track ID	Beam size	$\nu_{\rm c}$	$F_{\rm start}$	$F_{\rm end}$	$\sigma_{\rm avg}$	Linear	Orbital phase	Hours from	t =0
		['']	[GHz]	[mJy]	[mJy]	[mJy]	Polariz.	Coverage [ $\Phi$ ]	Periastron (0.0)	[ $\Phi$ ]
2008 Dec. 28	Dec08-IRAM	1.34 $\times$ 1.02	90.0	43.0	20.2	1.2	<4.65%	-0.02 to 0.00	-6.8 to 1.5	-0.056
2009 Mar. 17	Mar09-IRAM	3.39 $\times$ 2.79	90.0	12.6	16.9	1.1	<8.15%	-0.03 to -0.01	-13.7 to -5.3	-0.007
2010 Jan. 11	Jan10-IRAM	1.32 $\times$ 0.70	90.0	62.4	29.2	1.1	<7.60%	-0.04 to -0.02	-14.4 to -6.5	-0.067
2010 Jan. 12	Jan10-CARMA	0.87 $\times$ 0.67	92.5	30.3	12.4	3.9	-	-0.02 to 0.00	-7.2 to 1.1	-0.067
2010 Jan. 12	Jan10-SMA	1.25 $\times$ 1.00	238.5	95.6	85.2	5.6	-	-0.01 to 0.01	-4.7 to 3.6	-0.067
2008 Apr. 19	Apr08-CARMA	3.66 $\times$ 1.00	113.1	468	194	-	-	-0.02 to -0.01	-8.7 to -2.7	-0.020

Source LaTeX | All tables | In the text

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