VizieR Online Data Catalog: Stripping & unwinding galaxies from WINGS surveys (Vulcani+, 2022)

All galaxies considered in this paper have been observed in the context of the WINGS and OMEGAWINGS surveys.

The WINGS data set (Fasano+ 2006A&A...445..805F and Moretti+ 2014A&A...564A.138M) consists of B and V deep photometry of a field of view with the WFC@INT and the WFC@2.2mMPG/ESO for 76 clusters, along with J and K imaging with WFC@UKIRT and some U-band imaging. OMEGAWINGS extends WINGS observations, quadrupling the area covered (one square degree) for 46 of the 76 clusters. It is based on B and V observations with OmegaCAM@VST GTO programs.

For both surveys, a number of spectroscopic follow-ups have been conducted, using 2dF@AAT and WYFFOS@WHT observations for WINGS (Cava+ 2009, J/A+A/495/707), and AAOmega@AAT observations for OMEGAWINGS (Moretti+ 2017, J/A+A/599/A81). To further increase the spectroscopic sample, we carried out a systematic literature search of the available redshifts for the galaxies in the WINGS+OMEGAWINGS photometric sample. The final spectroscopic sample includes 46,700 redshifts. See Section 2.

(2 data files).