Items related to Optical 3D-Spectroscopy for Astronomy
Synopsis
DAS Referenzwerk mit aktuellen Informationen zu 3D-Spektrographen, die bei astronomischen Beobachtungen weit verbreitet sind, beschäftigt sich mit Licht im sichtbaren Nah-Infrarot- und Nah-UV-Bereich, erläutert die besten Beobachtungsstrategien und Instrumente und zeigt, wie die erzielten Daten verwaltet werden.
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About the Author
Roland Bacon is astrophysicist, directeur de recherche au CNRS and former director of the Lyon Observatory (1994-2004). He has played a pioneering role in the development of integral field spectroscopy as leader of 4 major and innovative instruments for ground based telescope: TIGER and OASIS at the 3.6m Canada France Hawaii telescope, SAURON at the 4.2m William Herschel telescope and MUSE at the 8m ESO Very Large Telescope. His main research field is extragalactic astronomy. He is the owner since 2014 of an advanced grant from the European Research Commission.
Guy Monnet is an astrophysicist, with 50-year experience of developing astronomical instrumentation, on the ground and in space, mostly with a 3D spectroscopic flavor. Successively, he was director of the Marseilles Observatory, Lyon Observatory and the Canada France Hawaii Telescope Corporation. He then took the position of Head of Instrumentation at the European Southern Observatory (1995-2009) and the Australian Astrophysical Observatory (2010-2011). His main scientific domain is the dynamics of stars and ionized gas in galaxies.
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