Surveying the High-Redshift Universe with KMOS

Details Surveying the High-Redshift Universe with KMOS Surveying the High-Redshift Universe with KMOS

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005msngr.122....2s&link_type=abstract

The Messenger (ISSN0722-6691), No.122, p. 2-5 (December 2005)

Physics

1

Scientific paper

KMOS is a near-infrared multi-object integral-field spectrometer which has been selected by ESO as one of a suite of second-generation instruments to be constructed for the VLT. The instrument will be built by a consortium of UK and German institutes working in partnership with ESO and is currently in the preliminary design phase. KMOS will be capable of obtaining simultaneous spatially resolved spectroscopy at a sampling of 0.2 arcseconds for up to 24 targets distributed over a field of view of 7.2 arcminutes diameter.

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