MUSE

E176896

MUSE is an advanced integral-field spectrograph used in optical astronomy to capture detailed spatial and spectral information from celestial objects.

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Label Occurrences
MUSE canonical 2

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Statements (48)

Predicate Object
instanceOf astronomical instrument
integral-field spectrograph
acronymFor Multi Unit Spectroscopic Explorer
dataProduct spectra for each spatial element
three-dimensional data cubes
developedBy European Southern Observatory
international consortium of institutes
fieldOfView approximately 1 arcminute squared (wide-field mode)
fullName Multi Unit Spectroscopic Explorer
hasCapability adaptive optics assisted observations
integral-field data cubes
medium spectral resolution
optical wavelength coverage
simultaneous spatial and spectral coverage
wide field of view
hasComponent detector arrays
image slicer
spectrographs
installedOn Very Large Telescope
surface form: Unit Telescope 4 of the VLT
locatedAt Paranal Observatory
locatedIn Chile
mode narrow-field mode with adaptive optics
wide-field mode
observes celestial objects
galaxies
nebulae
star clusters
stars
operatedAt Very Large Telescope
operatedBy European Southern Observatory
scientificGoal map physical conditions in ionized gas
measure redshifts of distant galaxies
study dynamics of stellar systems
study formation and evolution of galaxies
spectralRange optical wavelengths
telescopeAperture 8.2-metre class telescope
usedFor 3D spectroscopy
deep field observations
integral-field spectroscopy
kinematic studies of galaxies
observations of galaxy clusters
observations of planetary nebulae
optical astronomy
searches for high-redshift galaxies
spatially resolved spectroscopy
spectroscopic surveys of galaxies
spectroscopy of faint objects
studies of star-forming regions

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Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.