Variable accretion as a mechanism for brightness variations in T Tauri S

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Table 3:

Summary of the VLT/NACO photometry in the $K_{\rm S}$ band obtained between 2001 December and 2009 October.
Date			$\Delta K_{\rm S}$ (Sa-N)	$\Delta K_{\rm S}$ (Sb-N)
2001	Dec.	8	1.67 $\pm$ 0.05	3.02 $\pm$ 0.02
2002	Dec.	15	3.61 $\pm$ 0.05	3.14 $\pm$ 0.02
2003	Dec.	12	4.75 $\pm$ 0.05	3.25 $\pm$ 0.02
2004	Dec.	9	4.79 $\pm$ 0.05	3.31 $\pm$ 0.02
2006	Oct.	11	3.14 $\pm$ 0.05	2.94 $\pm$ 0.02
2007	Sep.	16	3.09 $\pm$ 0.05	2.92 $\pm$ 0.02
2008	Feb.	1	3.07 $\pm$ 0.05	3.05 $\pm$ 0.02
2008	Oct.	17	3.46 $\pm$ 0.05	3.07 $\pm$ 0.02
2008	Nov.	6	3.84 $\pm$ 0.05	2.88 $\pm$ 0.02
2009	Feb.	18	3.45 $\pm$ 0.05	2.88 $\pm$ 0.02
2009	Oct.	7	3.05 $\pm$ 0.05	3.07 $\pm$ 0.02

Notes. All magnitudes are relative to T Tau N.

Source LaTeX | All tables | In the text

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