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Radio Astronomy Centre

National Centre for Radio Astrophysics

Tata Institute of Fundamental Research


             We would like to thank e-Callisto groups at Institute for Astronomy, ETH Zurich and FHNW Brugg/Windisch, Switzerland and NCRA – TIFR for their support. This work has made use of SunPy, an open-source and free community-developed solar data analysis package written in Python (http://sunpy.org).