MUSE

E176896

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

All labels observed (1)

Label Occurrences
MUSE canonical 6

How this entity was disambiguated

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 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 ⓘ

How these facts were elicited

Referenced by (6)

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