MagE

E17449

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

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All labels observed (1)

Label Occurrences
MagE canonical 3

Statements (40)

Predicate Object
instanceOf astronomical instrument
medium-resolution spectrograph
optical echellette spectrograph
abbreviationOf Magellan Echellette Spectrograph (MagE)
surface form: Magellan Echellette
componentType cross-dispersed echellette
dataProduct echelle spectra
medium-resolution optical spectra
dispersionType echelle grating
fieldOfStudy astronomy
astrophysics
fullName Magellan Echellette Spectrograph (MagE)
surface form: Magellan Echellette Spectrograph
hostFacility Magellan I
surface form: 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 of Washington
surface form: 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 Magellan Telescopes
surface form: 6.5-meter Magellan telescopes
usedOn Magellan Telescopes
surface form: Magellan telescopes
wavelengthCoverage optical

Referenced by (3)

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

Magellan Echellette Spectrograph (MagE) alternateName MagE
subject surface form: Magellan Echellette Spectrograph
Magellan Echellette Spectrograph (MagE) hasAbbreviation MagE
subject surface form: Magellan Echellette Spectrograph