VizieR Online Data Catalog: Properties of LMC star clusters (Gatto+, 2020)

The data used in this work were obtained with the VLT Survey Telescope (VST) The telescope is equipped with OmegaCAM, a camera with a field-of-view of 1x1deg². The camera is a mosaic of 32-CCD, 16000x16000 detectors with a pixel scale of 0.214-arcsec/pix.

For each of the 85 SCs we report: equatorial coordinates, radius, age, reddening, metallicity, apparent and absolute magnitude in the g-band, the tile where the SC in question resides and a flag assessing the reliability of each SC.

(1 data file).