Abstract
OSIRIS, the optical Day One instrument for the GTC, will shortly be shipped to La Palma to start the commissioning at the telescope. Some results of the final laboratory characterization of the instrument are shown, together with the upgrades that are planned to be operational after Day One. Several large programs using the OSIRIS Tunable Filters are presented as well, to demonstrate the scientific capabilities of this characteristic OSIRIS observing mode.
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Acknowledgements
OSIRIS instrument has been funded by the Spanish Plan Nacional de Astronomía y Astrofísica of the Ministry of Science and Technology under grants AYA2000–0333–P4–02, AYA2002–12070–E, and AYA2005–04149, GRANTECAN S.A., and the IAC.
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Cepa, J. (2010). OSIRIS: Final Characterization and Scientific Capabilities. In: Diego, J., Goicoechea, L., González-Serrano, J., Gorgas, J. (eds) Highlights of Spanish Astrophysics V. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11250-8_2
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DOI: https://doi.org/10.1007/978-3-642-11250-8_2
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Online ISBN: 978-3-642-11250-8
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