DC2-analysis icon indicating copy to clipboard operation
DC2-analysis copied to clipboard

Published 20 hours ago • verified publisher icon LSSTDESC

Compute purity and completeness for stars, galaxies for DC2 Run2.1i

Open wmwv opened this issue 5 years ago • 0 comments

  1. [ ] Compare the Object (coadd) catalog with the truth catalog to calculate purity and completeness for star-galaxy identification as a function of magnitude.
  2. [ ] Compute a variability metric and compare its additional distinguishing power.
    • May need to include some systematic stochastic intrinsic variability parameter for each of stars and galaxies (AGN?).
  3. [ ] Compute a seeing-weighted variability metric to identify stars vs. galaxies by * how their magnitude changes under different seeing.

wmwv avatar Jun 26 '19 15:06 wmwv