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doi: 10.5281/zenodo.58412
The Herschel DEBRIS survey has been a great success, revealing a wide variety of resolved disks, suggesting a correlation between bright debris disks and systems of low-mass planets, and enabling us to estimate the true incidence of debris disks, rather than just a detection rate. I will review the survey and some of its key results and then highlight key areas of inquiry for future surveys.
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