Rotation-disk connection for very low mass and substellar objects in the Orion Nebula Cluster

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Table 1:

Number of periodic variables from Paper I with a near-infrared counterpart.
	Periodic variables
	At least one band	All JHK bands
UKIDSS	419	210
VLT	113	113
2MASS	684	409^a

Notes. ^(a) 684 periodic variables in our sample have 2MASS JHK colors, but since UKIDSS and VLT data have higher priority than 2MASS, 2MASS colors have been used only for the 409 objects without UKIDSS and VLT data.

Source LaTeX | All tables | In the text

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