3 code implementations • 12 Oct 2009 • Dustin Lang, David W. Hogg, Keir Mierle, Michael Blanton, Sam Roweis
We have built a reliable and robust system that takes as input an astronomical image, and returns as output the pointing, scale, and orientation of that image (the astrometric calibration or WCS information).
Instrumentation and Methods for Astrophysics
