MagE

E17449

MagE is a medium-resolution optical echellette spectrograph used on the Magellan telescopes for detailed spectroscopic studies of astronomical objects.


Statements (40)
Predicate Object
instanceOf astronomical instrument
medium-resolution spectrograph
optical echellette spectrograph
abbreviationOf Magellan Echellette
componentType cross-dispersed echellette
dataProduct echelle spectra
medium-resolution optical spectra
dispersionType echelle grating
fieldOfStudy astronomy
astrophysics
fullName Magellan Echellette Spectrograph
hostFacility Magellan Project
instrumentClass faint-object spectrograph
locatedAt Las Campanas Observatory
locatedIn Chile
measurementType chemical abundances
radial velocities
redshifts
spectral line profiles
mountedOn Magellan Clay Telescope
observationMode long-slit spectroscopy
observatoryOperator Carnegie Institution for Science
opticalBand visible light
primaryUse detailed spectroscopic studies of astronomical objects
scienceUse galaxy spectroscopy
intergalactic medium studies
interstellar medium studies
quasar spectroscopy
stellar spectroscopy
scientificGoal high signal-to-noise optical spectroscopy
medium-resolution spectral surveys
spectralResolution medium
targetType compact objects
galaxies
quasars
stars
supernovae
telescopeType 6.5-meter Magellan telescopes
usedOn Magellan telescopes
wavelengthCoverage optical


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