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The school is designed to offer a comprehensive training to graduate and advanced undergraduate students in observational techniques and tools for follow up of transient events at X-ray, UV, optical, infrared and radio wavelengths. The school sessions are organized by wavelength range and the format includes a short lecture that introduces the topic followed by an interactive workshop where students will be engaged in data analysis using real data from the LIGO, Keck Observatory in Hawaii, Palomar Observatory in California, the VLA in New Mexico and telescopes in the GROWTH global network of observatories.
