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## Table 1. SDWFS-DIA Variability Catalog. 

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Note. — This is an abridged version of the full table, presenting the variability statistics for the combined channels [3.6] and [4.5] only. The electronic table includes additional columns showing the variability statistics for the separate channels [3.6] and [4.5], and the photometric uncertainties for the IRAC channels. Here, quantities v ([ X ]) and Nϵ , are respectively, the variability standard deviation in channel [ X ] and the common number of epochs in both channels used in the calculation of the joint variability. With C$_{12}$ , r , and σ$_{12}$ we denote the covariance and the correlation between the channels 1 and 2, and the joint variability significance, respectively. The mask is 0 (1) if there is (is no) bright star with the 2mass K -band magnitude within 260(1 − K/ 11) arcsec affecting the measurement. The Vega magnitudes presented in the table are measured in 4 arcsec apertures (see Ashby et al. 2009). The error code for magnitudes, reflecting no measurement, is 99.999. The error code for v , C$_{12}$ , r , and σ$_{12}$ is 99.999. 

(This table is available in its entirety in a machine-readable form in the online journal. A portion is shown here for guidance regarding its form and content.) 

