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Future Instrumentation for the Study of the Warm-Hot Intergalactic Medium
Authors:Frits Paerels  Jelle Kaastra  Takaya Ohashi  Philipp Richter  Andrei Bykov  Jukka Nevalainen
Institution:1. Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY, 10027, USA
2. SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands
3. Sterrenkundig Instituut, Universiteit Utrecht, P.O. Box 80000, 3508 TA, Utrecht, The Netherlands
4. Department of Physics, School of Science, Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo, 192-0397, Japan
5. Institut für Physik, Universit?t Potsdam, Am Neuen Palais 10, 14469, Potsdam, Germany
6. A.F. Ioffe Institute of Physics and Technology, Russian Academy of Sciences, 26 Polytekhnicheskaya, St. Petersburg, 194021, Russia
7. Observatory, University of Helsinki, P.O. Box 14, 00014, T?htitornim?ki, Finland
Abstract:We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.
Keywords:Instrumentation: spectrographs  Instrumentation: photometers  Ultraviolet: general  X-rays: general            γ  -rays: general
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