8 July 2014 Performance of the K-band multi-object spectrograph (KMOS) on the ESO VLT
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Abstract
KMOS is a multi-object near-infrared integral field spectrograph built by a consortium of UK and German institutes for the ESO Paranal Observatory. We report on the on-sky performance verification of KMOS measured during three commissioning runs on the ESO VLT in 2012/13 and some of the early science results.
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Ray Sharples, Ray Sharples, Ralf Bender, Ralf Bender, Alex Agudo Berbel, Alex Agudo Berbel, Richard Bennett, Richard Bennett, Naidu Bezawada, Naidu Bezawada, Roberto Castillo, Roberto Castillo, Michele Cirasuolo, Michele Cirasuolo, Paul Clark, Paul Clark, George Davidson, George Davidson, Richard Davies, Richard Davies, Roger Davies, Roger Davies, Marc Dubbeldam, Marc Dubbeldam, Alasdair Fairley, Alasdair Fairley, Gert Finger, Gert Finger, Natascha Förster Schreiber, Natascha Förster Schreiber, Reinhard Genzel, Reinhard Genzel, Reinhold Haefner, Reinhold Haefner, Achim Hess, Achim Hess, Ives Jung, Ives Jung, Ian Lewis, Ian Lewis, David Montgomery, David Montgomery, John Murray, John Murray, Bernard Muschielok, Bernard Muschielok, Jeff Pirard, Jeff Pirard, Suzanne Ramsay, Suzanne Ramsay, Philip Rees, Philip Rees, Josef Richter, Josef Richter, David Robertson, David Robertson, Ian Robson, Ian Robson, Stephen Rolt, Stephen Rolt, Roberto Saglia, Roberto Saglia, Ivo Saviane, Ivo Saviane, Joerg Schlichter, Joerg Schlichter, Linda Schmidtobreik, Linda Schmidtobreik, Alex Segovia, Alex Segovia, Alain Smette, Alain Smette, Matthias Tecza, Matthias Tecza, Stephen Todd, Stephen Todd, Michael Wegner, Michael Wegner, Erich Wiezorrek, Erich Wiezorrek, } "Performance of the K-band multi-object spectrograph (KMOS) on the ESO VLT", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91470W (8 July 2014); doi: 10.1117/12.2055496; https://doi.org/10.1117/12.2055496
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