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A tidal tail is a thin, elongated region of stars and interstellar gas that extends into space from a galaxy. Tidal tails occur as a result of galactic tide forces between interacting galaxies. Examples of galaxies with tidal tails include the Tadpole Galaxy and the Mice Galaxies.
Regions near the polyA tail are sequenced, and flourescently labeled streptavidin molecules are attached to the biotinylated dUTPs. Signal intensity is measured to determine polyA tail length. This method is useful because it avoids direct sequencing of the polyA tail. In recent experiments, PAL-seq has revealed that polyA tail lengths are relatively conserved across organisms, and that polyA tail lengths change during development, indicating an embryonic switch in translational control.