Optical imaging for the Spitzer Survey of Stellar Structure in Galaxies. Data release and notes on interacting galaxies
Johan H. Knapen, Santiago Erroz-Ferrer, Javier Roa, Judit Bakos,, Mauricio Cisternas, Ryan Leaman, Nik Szymanek

TL;DR
This paper presents a comprehensive optical imaging dataset for the S4G galaxy survey, including re-processed SDSS images, new observations, and a catalog of interactions, supporting studies of galaxy structure and evolution.
Contribution
It provides the first large-scale, publicly available optical imaging dataset for the S4G galaxies, including interaction classifications and a catalog of companions.
Findings
17% of S4G galaxies have close companions
5% show morphological evidence of interactions
Over 8000 images and a catalog are publicly released
Abstract
(Abridged) The Spitzer Survey for Stellar Structure in Galaxies (S4G) and its more recently approved extension will lead to a set of 3.6 and 4.5 micron images for 2829 galaxies, which can be used to study many different aspects of the structure and evolution of local galaxies. We collected and re-processed optical images in five bands from the Sloan Digital Sky Survey for 1657 galaxies, which are publicly released with the publication of this paper. We observed, in only the g-band, an additional 111 S4G galaxies in the northern hemisphere with the 2.5 m Liverpool Telescope, so that optical imaging is released for 1768 galaxies, or for 62% of the S4G sample. We visually checked all images. We noted interactions and close companions in our optical data set and in the S4G sample, confirming them by determining the galaxies' radial velocities and magnitudes in the NASA-IPAC Extragalactic…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
