MIKE (Magellan Inamori Kyocera Echelle)

E120414
optical echelle spectrograph

MIKE (Magellan Inamori Kyocera Echelle) is a high-resolution optical echelle spectrograph used on the Magellan telescopes for detailed spectroscopic studies of astronomical objects.

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All labels observed (2)

Label Occurrences
Magellan Inamori Kyocera Echelle 2
MIKE (Magellan Inamori Kyocera Echelle) canonical 1

Statements (45)

Predicate Object
instanceOf optical echelle spectrograph ⓘ
acronymFor MIKE (Magellan Inamori Kyocera Echelle) self-linksurface differs ⓘ
surface form: Magellan Inamori Kyocera Echelle
associatedWith Carnegie Observatories ⓘ
countryOfFacility Chile ⓘ
crossDisperser prism ⓘ
dataProduct high-resolution spectra ⓘ
detectorType CCD ⓘ
dispersingElement echelle grating ⓘ
environment ground-based ⓘ
fullName MIKE (Magellan Inamori Kyocera Echelle) self-linksurface differs ⓘ
surface form: Magellan Inamori Kyocera Echelle
fundingSource Inamori Foundation ⓘ
Kyocera Corporation ⓘ
hasChannel blue arm ⓘ
red arm ⓘ
hostFacility Magellan Project ⓘ
instrumentType cross-dispersed echelle spectrograph ⓘ
locatedAt Las Campanas Observatory ⓘ
locatedIn Chile ⓘ
mountedAt Nasmyth focus of Magellan telescope ⓘ
observatoryOperator Carnegie Institution of Washington ⓘ
surface form: Carnegie Institution for Science
observingMode long-slit spectroscopy ⓘ
resolutionType high-resolution ⓘ
scienceTarget damped Lyman-alpha systems ⓘ
galaxies ⓘ
globular clusters ⓘ
quasars ⓘ
stars ⓘ
scienceUse chemical evolution of galaxies ⓘ
detailed spectroscopic studies of astronomical objects ⓘ
galactic archaeology ⓘ
interstellar medium studies ⓘ
quasar absorption line studies ⓘ
stellar abundance analysis ⓘ
spectralRange near-infrared ⓘ
near-ultraviolet ⓘ
optical ⓘ
spectralResolution up to R ~ 65,000 depending on slit ⓘ
telescopeAssociation Baade Telescope ⓘ
surface form: Magellan Baade Telescope

Magellan Clay Telescope ⓘ
typicalUse detailed line profile analysis ⓘ
metal-poor star studies ⓘ
nucleosynthesis studies ⓘ
precision radial velocity measurements ⓘ
usedOn Magellan Telescopes ⓘ
surface form: Magellan telescopes
wavelengthCoverage approximately 335 nm to 950 nm ⓘ

Referenced by (3)

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

Magellan telescope instrumentation suite → hasInstrument → MIKE (Magellan Inamori Kyocera Echelle) ⓘ
MIKE (Magellan Inamori Kyocera Echelle) → fullName → MIKE (Magellan Inamori Kyocera Echelle) self-linksurface differs ⓘ
subject surface form: MIKE
this entity surface form: Magellan Inamori Kyocera Echelle
MIKE (Magellan Inamori Kyocera Echelle) → acronymFor → MIKE (Magellan Inamori Kyocera Echelle) self-linksurface differs ⓘ
subject surface form: MIKE
this entity surface form: Magellan Inamori Kyocera Echelle