KELT was designed to find transiting planets that are good candidates for follow-up observations, and so we have found about twenty planets to date, identifying some of the brightest known hosts of transiting planets in the process. With the long baseline of KELT, we have also contributed to the study of clusters, variable stars, and eclipsing binaries and other eclipsing but non-planetary events.
As LSST has still not begun operations and the cadence has been open to suggestion from the scientific community, I have also been involved in working on characterizing the cadence for time-domain science, with a particular interest in finding other science cases that will benefit from observations similar to the preferred observations for transiting planets. Much of this work has appeared in the LSST Observing Schedule white paper, and in the additional cadence white papers that are currently in development.
In the firm belief that creativity is essential in science, I am the proud founder, editor, and primary contributor to the exclusive annual journal Acta Prima Aprilia.