The PINGS galaxy sample is composed mainly of normal symmetric face-on spiral galaxies, although lopsided, interacting and barred spirals were also considered. A large fraction of the sample has a rich set of ancillary observations in the UV, infrared, HI, IR and radio. The sample covers a good range of galactic properties and star forming environments with multiwavelength public data. For more information see the Publications section.
Objects and mosaicking
Digital sky images of the PINGS galaxy sample. On each image, an array of hexagonal fields corresponding to the PPAK aperture is shown on scale. Each image is 10’ x 10’.
