Add to ORKGKMOS is a near-infrared multi-object in-tegral-field spectrometer which has been selected by ESO as one of a suite of second-generation instruments to be constructed for the VLT. The instru-ment 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 simultane-ous 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. The past decade has seen remarkabl
"After a general description of the instrument, we review the current monitoring and calibration pla...
In this talk I will discuss recent progress studying the rest-frame optical properties of quiescent ...
The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic e ffort in...
KMOS is a near-infrared multi-object integral field spectrometer which has been selected as one of a...
KMOS is a near-infrared multi-object integral-field spectrometer which is one of a suite of second-g...
We describe the design of a 2nd generation instrument for the ESO VLT which will deliver a unique mu...
International audienceWe present an overview of the KMOS instrument, currently under construction by...
We describe a proposed 2nd generation instrument (KMOS) for the ESO VLT which will deliver a unique ...
We present the results of a design study for the spectrograph module for KMOS - a cryogenic near-inf...
We describe the design of a 2nd generation instrument for the ESO VLT which uses 24 cryogenic pickof...
Near-infrared integral field unit (IFU) spectrographs are powerful tools for investigating galaxy ev...
The Galactic centre is a unique target to study the central region of a galaxy. At a distance of onl...
This Thesis contains two parts. Part I details my work on KMOS, a new instrument for the VLT and Par...
We present the first results of the K-band Multi-Object Spectrometer (KMOS) Lens-Amplified Spectrosc...
The KMOS Lens-Amplified Spectroscopic Survey (KLASS) is an ESO Large Program (PI: A. Fontana) which ...
"After a general description of the instrument, we review the current monitoring and calibration pla...
In this talk I will discuss recent progress studying the rest-frame optical properties of quiescent ...
The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic e ffort in...
KMOS is a near-infrared multi-object integral field spectrometer which has been selected as one of a...
KMOS is a near-infrared multi-object integral-field spectrometer which is one of a suite of second-g...
We describe the design of a 2nd generation instrument for the ESO VLT which will deliver a unique mu...
International audienceWe present an overview of the KMOS instrument, currently under construction by...
We describe a proposed 2nd generation instrument (KMOS) for the ESO VLT which will deliver a unique ...
We present the results of a design study for the spectrograph module for KMOS - a cryogenic near-inf...
We describe the design of a 2nd generation instrument for the ESO VLT which uses 24 cryogenic pickof...
Near-infrared integral field unit (IFU) spectrographs are powerful tools for investigating galaxy ev...
The Galactic centre is a unique target to study the central region of a galaxy. At a distance of onl...
This Thesis contains two parts. Part I details my work on KMOS, a new instrument for the VLT and Par...
We present the first results of the K-band Multi-Object Spectrometer (KMOS) Lens-Amplified Spectrosc...
The KMOS Lens-Amplified Spectroscopic Survey (KLASS) is an ESO Large Program (PI: A. Fontana) which ...
"After a general description of the instrument, we review the current monitoring and calibration pla...
In this talk I will discuss recent progress studying the rest-frame optical properties of quiescent ...
The Complete Calibration of the Colour-Redshift Relation survey (C3R2) is a spectroscopic e ffort in...