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Fig. 2.

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Example pv–diagrams along the major and minor kinematic axes of NGC 3627 (top) and NGC 4654 (bottom) used to search for outflows. The color scale represents the intensity at a given position along the offset averaged over a width of 3 pixels. The contours are multiples of the noise at 2.5σ, 3.5σ, followed by niσ with ni = 2ni − 1, for n0 = 2.5σ and i = 1, 2, 3, …. The color range is saturated to emphasize the faint emission we are interested in. The pv–diagrams of NGC 3627 (NGC 4654) correspond to OCLs of 3, 2, 2 (0, 0, 0) from the three different inspectors. The systemic velocity (yellow horizontal line) is added for comparison and is subtracted from the velocity axis.

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