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We have collected a catalog of 1095 debris disks with properties andclassification (resolved, planet, gas) information. From the catalog, wedefined a less biased sample with 612 objects and presented the distributionsof their stellar and disk properties to search for correlations between disksand stars. We found debris disks were widely distributed from B to M-type starswhile planets were mostly found around solar-type stars, gases were easier todetect around early-type stars and resolved disks were mostly distributed fromA to G- type stars. The fractional luminosity dropped off with stellar age andplanets were mostly found around old stars while gas-detected disks were muchyounger. The dust temperature of both one-belt systems and cold components intwo-belt systems increased with distance while decreasing with stellar age. Inaddition, we defined a less biased planet sample with 211 stars with debrisdisks but no planets and 35 stars with debris disks and planets and found thestars with debris disks and planets had higher metallicities than stars withdebris disks but no planets. Among the 35 stars with debris disks and planets,we found the stars with disks and cool Jupiters were widely distributed withage from 10 Myr to 10 Gyr and metallicity from -1.56 to 0.28 while the otherthree groups tended to be old (> 4Gyr) and metal-rich (> -0.3). Besides, theeccentricities of cool Jupiters are distributed from 0 to 0.932 wider than theother three types of planets (< 0.3).

A catalog of collected debris disks: properties, classifications and correlations between disks and stars/planets