Disambiguation evidence for GMOS-S (Gemini Multi-Object Spectrograph South) via surface form

"GMOS-S"


As subject (50)

Triples where this entity appears as subject under the label "GMOS-S".

Predicate Object
counterpartLocatedAt Gemini North Observatory
surface form: Gemini North telescope
dataProduct 1D extracted spectra
dataProduct 2D spectra
dataProduct optical images
designedFor distant-universe studies
designedFor faint-object spectroscopy
enables deep spectroscopy of faint sources
enables kinematic studies of galaxies
enables redshift measurements of distant galaxies
enables simultaneous spectroscopy of multiple targets
enables spectral line diagnostics
fieldOfViewType wide-field optical imager
fullName GMOS-S (Gemini Multi-Object Spectrograph South) self-linksurface differs
surface form: Gemini Multi-Object Spectrograph South
hasCounterpart GMOS-N (Gemini Multi-Object Spectrograph North)
surface form: GMOS-N
hasMode imaging mode
hasMode long-slit spectroscopy mode
hasMode multi-object spectroscopy mode
hasMode nod-and-shuffle spectroscopy mode
instanceOf Gemini South instrument
instanceOf astronomical imager
instanceOf multi-object spectrograph
instanceOf optical spectrograph
locatedAt Cerro Pachón
surface form: Cerro Pachón, Chile
locatedAt Gemini South Observatory
surface form: Gemini South telescope
mountedOn Gemini South Cassegrain focus
observatory Gemini Observatory
surface form: International Gemini Observatory
operatedBy Gemini Observatory
operatedBy NOIRLab
surface form: NSF NOIRLab
partOf GMOS-S (Gemini Multi-Object Spectrograph South) self-linksurface differs
surface form: Gemini South instrument suite
primaryFunction long-slit spectroscopy
primaryFunction multi-object spectroscopy
scienceGoal cluster of galaxies spectroscopy
scienceGoal gravitational lens spectroscopy
scienceGoal stellar population studies
scienceGoal study of active galactic nuclei
scienceGoal study of distant galaxies
scienceGoal study of faint astronomical sources
scienceGoal study of galaxy evolution
scienceGoal supernova spectroscopy
secondaryFunction optical imaging
supports classical observing
supports queue scheduling operations
telescopeAperture 8.1-meter
usedIn extragalactic astronomy research
usedIn observational cosmology research
uses filters
uses gratings
uses slit masks
wavelengthCoverageApprox ~0.36–1.0 microns
wavelengthRange optical