LUCI (former LUCIFER) is the full cryogenic near-infrared multi-object spectrograph and imager at the LBT. It presently allows for seeing limited imaging and multi-object spectroscopy at R∼2000-4000 in a 4x4arcmin 2 FOV from 0.9 to 2.5 micron. We report on the instrument performance and the lessons learned during the first two years on sky from a technical and operational point of view. We present the upcoming detector upgrade to Hawaii-2 RG arrays and the operating modes to utilize the binocular mode, the LBT facility AO system for diffraction limited imaging as well as to use the wide-field AO correction afforded by the multi-laser GLAO System ARGOS in multi-object spectroscopy. © 2012 SPIE.
CITATION STYLE
Buschkamp, P., Seifert, W., Polsterer, K., Hofmann, R., Gemperlein, H., Lederer, R., … Genzel, R. (2012). LUCI in the sky: performance and lessons learned in the first two years of near-infrared multi-object spectroscopy at the LBT. In Ground-based and Airborne Instrumentation for Astronomy IV (Vol. 8446, p. 84465L). SPIE. https://doi.org/10.1117/12.926989
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