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2005, ApJ, 621, 695 Wright G. et al. 2004, SPIE, 5487, 653 IFUs: Disentangling the Light from Neighbour Fibers A. Kanaan1 , C. Mendes de Oliveira2 , C. Strauss3 , B. V. Castilho4 and F. Ferrari5 1 2 3 4 5 Dep. br Integral Field Unit (IFU) spectrographs allow continuous space coverage of a small part of the sky by using a microlens array at the telescope focal plane. Each microlens images the telescope pupil onto an optical fiber, which is in turn taken to a bench spectrograph. A larger number of microlenses allows for higher spatial coverage and/or spatial resolution.

It provides three-dimensional near-infrared spectroscopy at the resolution limit of the Keck II telescope, which is equipped with adaptive optics and a laser guide star. The innovative capabilities of OSIRIS enable many new observing projects. OSIRIS can perform detailed studies of the stellar content and dynamical properties of galaxies in the early Universe. In quasars, radio galaxies, and nearby active galactic nuclei, OSIRIS can elucidate the relation of the central black hole to the properties of the host galaxy, and the mechanism feeding gas into the central engine.

The innovative capabilities of OSIRIS enable many new observing projects. OSIRIS can perform detailed studies of the stellar content and dynamical properties of galaxies in the early Universe. In quasars, radio galaxies, and nearby active galactic nuclei, OSIRIS can elucidate the relation of the central black hole to the properties of the host galaxy, and the mechanism feeding gas into the central engine. In the center of our own Galaxy, it is possible to investigate the properties of the massive black hole and the stars in its immediate vicinity.

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