1 code implementation • 17 Sep 2018 • Jens Erler, Miriam E. Ramos-Ceja, Kaustuv Basu, Frank Bertoldi
The application of these new filters is demonstrated by applying them to microwave and X-ray mock data of galaxy clusters with the aim of reducing contamination by point-like sources, which are well approximated by the instrument beam.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
