LSST Cadence Workshop
The science of the LSST will, in part, be driven by how it observes the sky (the footprint and cadence of the survey). The objectives of this meeting are to train astronomers in the tools available to simulate the properties of the LSST; to revisit the science drivers for various LSST programs with an eye towards optimization of the baseline observing cadence; and the development of metrics that might be used to quantify the science performance of the LSST as a function of its cadence. Examples where further cadence optimization is likely to yield tangible improvements in the LSST science include the coverage of the Galactic plane, characterization of supernovae light curves, the reduction of systematics through dithering, deep drilling fields, and active area vs. sampling rate tradeoffs (also known as “rolling cadence”).
This workshop will include an introduction to the cadence issues for the LSST, a set of tutorials that will train people in how to use the LSST tools, and a series of breakout or hack sessions where the impact of cadence on the science will be discussed (including summarizing the current understanding of various cadence issues and identifying a roadmap to address these issues in a quantitative manner).
To register for this meeting please go here