LDSS3

E117315

LDSS3 is a wide-field, multi-object spectrograph and imaging instrument used on the Magellan Telescopes for detailed optical observations of faint astronomical objects.

All labels observed (2)

Label Occurrences
LDSS-3 1
LDSS3 canonical 1

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf astronomical instrument
imaging instrument
multi-object spectrograph
abbreviationFor Low Dispersion Survey Spectrograph 3
capability imaging
multi-object spectroscopy
collaboration Magellan Consortium
linked to: Magellan Project
dataProduct optical images
optical spectra
designedFor faint object spectroscopy
survey work
fieldOfView wide-field
fullName Low Dispersion Survey Spectrograph 3
hasMode imaging mode
spectroscopic mode
hostTelescope Magellan II Clay Telescope
locatedAt Magellan Clay Telescope
locationCountry Chile
mountType Cassegrain focus instrument
observatory Las Campanas Observatory
observatoryOperator Carnegie Institution for Science
operationalStatus in use (2020s)
primaryUse spectroscopy of faint astronomical objects
wide-field imaging
scienceDomain extragalactic astronomy
galaxy evolution studies
observational astronomy
quasar spectroscopy
stellar populations
supernova follow-up
scienceOutput redshift surveys
spectral classification of galaxies
spectral classification of stars
spectroscopy of transient events
siteAltitude ~2400 m
successorTo LDSS-2
supports broad-band imaging
long-slit spectroscopy
multi-slit spectroscopy
telescopeAperture 6.5-meter
usedBy international astronomy community
usedOn Magellan Telescopes
uses filters
grisms
slitmasks
wavelengthRange optical

How these facts were elicited

Referenced by (2)

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