Telescope has monitored over 50,000 galaxies using uninterrupted, high-precision, high-cadence optical photometry. This public data set is known to include at least 40 supernovae which await analysis.
• Planets around bright and nearby stars ex. GJ 9827, TRAPPIST-1. • Rotation and activity in young and old star clusters ex. Taurus, Pleiades, Beehive, Lagoon Nebula, M67. • Hundreds of pulsating White Dwarfs and Cataclysmic Variables => continuous monitoring across 80-day periods
discover the accelerating expansion of the Universe, we still do not understand the nature of the progenitor system, e.g. • White Dwarf accreting from a companion? (single degenerate scenario) • Merger of two White Dwarfs? (double degenerate scenario) Do multiple scenarios lead to SN Ia’s? In what proportion?!
SN were observed. (Olling+ 2015) Result: none showed excess flux in the early-rise lightcurve. Were they all double degenerate progenitors, or single degenerate systems with a particular line of sight? The K2 Supernova Experiment aims to increase the sample ten-fold.
Experiment” => Kepler studied 50,000 galaxies in two fields across 6 months, accompanied by multi-color monitoring from the ground. (Including PanSTARRS and ASASSN.)
to add a new dimension to the study of high energy transients. The data are public and await analysis; including Supernovae, AGN, and CVs. Significant opportunities exist for future exoplanet transit surveys!