Alicante, Spain, 14-17 November 2017
High resolution spectroscopy is a fundamental tool in X-ray Astrophysics. It provides unique plasma diagnostics in a variety of Astrophysical contexts from clusters of galaxies to solar system bodies. Current grating based spectrometers (XMM-RGS, Chandra HETG) provide the highest spectral resolution achievable nowadays. The calorimeters (XARM, Athena) will increase the resolution to unprecedented levels opening a new era of X-ray astrophysics that will expand our knowledge of the high energy Universe.
AHEAD aims at providing young astronomers the specific theoretical and practical skills to successfully exploit the current and future generation of X-ray instruments. To this end, world class experts in several fields will deliver lectures and conduct hands on sessions, including analysis of real calorimeter data. The students will have the opportunity to interact with renowned scientists in a highly motivating environment.
Students and postdocs. Although the course will be self contained, previous background in X-ray astronomy (not necessarily high spectral resolution) is highly recommended. The School is limited to 40 students.
System requirement and network connection
Network connection will be provided via eduroam. Please install the required certificates in your computers. If you are not able to install eduroam let us know well in advance.
Registration is now open and is free of charge (covered by AHEAD).
Current and future X-ray high resolution spectrometers
High Mass X-ray Binaries
Jelle de Plaa
University of Alicante Campus, San Vicente del Raspeig, Building "Germán Bernácer".