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KMOS @ the VLT: Commissioning and Early Science

Published online by Cambridge University Press:  09 February 2015

Ray Sharples
Affiliation:
Department of Physics, University of Durham, Durham, UK email: [email protected]
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Abstract

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KMOS is a multi-object near-infrared integral field spectrograph built by a consortium of UK and German institutes for the ESO Paranal Observatory. KMOS completed commissioning at the ESO VLT in Spring 2013 and was made available to the user community from Oct 2013. We present the unique capabilities of KMOS for 3D galaxy surveys and report on the on-sky performance verification measured during three commissioning runs on the ESO VLT in 2012/13 and some of the early science results.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Sharples, R., et al., Proc. SPIE 5492, 1179 (2004)Google Scholar
Sharples, R., et al., Proc. SPIE 6269, 44 (2006)Google Scholar
Rees, P., et al., Proc. SPIE 7735, 166 (2010)Google Scholar
Dubbeldam, M., et al., Proc. SPIE 8450, 84501M (2012)Google Scholar
Masters, R., et al., Proc. SPIE 7735, 168 (2010)Google Scholar
Finger, G., et al., Proc. SPIE 7021, 20 (2008)Google Scholar
Bezawada, N., et al., Proc. SPIE 7014, 121 (2008)Google Scholar
Hess, A., et al., Proc. SPIE 7735, 93 (2010)Google Scholar
Davies, R., et al., Astronomy & Astrophysics, Vol 558, A56 (2013)CrossRefGoogle Scholar
Wegner, M., et al., Proc. SPIE 7740, 28 (2010)Google Scholar
Sharples, R., et al., Proc. SPIE 8446, 84460K (2012)Google Scholar
Sharples, R., et al., The Messenger 151, 21 (2013)Google Scholar
Davies, R., MNRAS 375, 1009 (2007)Google Scholar