KMOS Extension
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
This proposal covers the final phase of Oxford work on the three KMOS spectrographs through final integration at the UKATC and readiness for acceptance testing.
Planned Impact
Due to the unique nature of the KMOS instrument, the impact of this research on the study of galaxy evolution and the star formation history of the Universe will be considerable. These results will be based on the work of the KMOS consortium and other ESO users and will be published in scientific journals and conference proceedings. Oxford's existing outreach activities with local events and schools visits will naturally provide a vehicle for dissemination of the findings, and the technology behind the instrument to a wider public audience.
Organisations
Publications
Alatalo K
(2013)
NGC 1266 AS A LOCAL CANDIDATE FOR RAPID CESSATION OF STAR FORMATION
in The Astrophysical Journal
Alatalo K
(2013)
The ATLAS3D project - XVIII. CARMA CO imaging survey of early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Bayet E
(2013)
The ATLAS3D project - XVI. Physical parameters and spectral line energy distributions of the molecular gas in gas-rich early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Cappellari M
(2013)
The ATLAS3D project - XV. Benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, Fundamental Plane and Mass Plane
in Monthly Notices of the Royal Astronomical Society
Cappellari M
(2013)
The ATLAS3D project - XX. Mass-size and mass-s distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function
in Monthly Notices of the Royal Astronomical Society
Chan J
(2018)
The KMOS Cluster Survey (KCS). II. The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift 1.39 < z < 1.61*
in The Astrophysical Journal
D'Eugenio F
(2013)
Fast and slow rotators in the densest environments: a FLAMES/GIRAFFE integral field spectroscopy study of galaxies in A1689 at z = 0.183
in Monthly Notices of the Royal Astronomical Society
Davis T
(2013)
The ATLAS3D Project - XIV. The extent and kinematics of the molecular gas in early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Kimura M
(2010)
Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope
in Publications of the Astronomical Society of Japan
Krajnovic D
(2013)
The ATLAS3D Project - XXIII. Angular momentum and nuclear surface brightness profiles
in Monthly Notices of the Royal Astronomical Society
Krajnovic D
(2013)
The ATLAS3D project - XVII. Linking photometric and kinematic signatures of stellar discs in early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Martig M
(2013)
The ATLAS3D project - XXII. Low-efficiency star formation in early-type galaxies: hydrodynamic models and observations
in Monthly Notices of the Royal Astronomical Society
Pastorello N
(2013)
The planetary nebulae population in the nuclear regions of M31: the SAURON view
in Monthly Notices of the Royal Astronomical Society
Rees P
(2010)
First end-end performance testing and results for KMOS
Sarzi M
(2013)
The ATLAS3D project - XIX. The hot gas content of early-type galaxies: fast versus slow rotators
in Monthly Notices of the Royal Astronomical Society
Scott N
(2013)
The ATLAS3D project - XXI. Correlations between gradients of local escape velocity and stellar populations in early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Serra P
(2013)
Discovery of a giant H i tail in the galaxy group HCG 44
in Monthly Notices of the Royal Astronomical Society
Sharples R
(2006)
Design of the KMOS multi-object integral-field spectrograph
Tecza M
(2006)
Opto-mechanical design of the KMOS spectrograph module
Description | KMOS spectrographs delivered and working on the ESO VLT. |
Exploitation Route | The KMOS instrument is available for use by astronomers across Europe. |
Sectors | Education |