VizieR Online Data Catalog: IR data of debris disk vs metallicity of stars (Gaspar+, 2016)

To build the largest possible sample of debris disks, we merged data from multiple sources (see section 2 for details). We separate the final sample into two groups: warm and cold debris disks. Systems with Spitzer 24um excesses or upper limits or with WISE W4 excesses are included in the warm disk sample, while systems with Spitzer 70um and/or Herschel 70/100um data (either excesses or upper limits) are included in the cold disk sample.

(5 data files).