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 Project
surface form: Magellan Consortium
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 Clay Telescope
surface form: Magellan II Clay Telescope
locatedAt Magellan Clay Telescope
locationCountry Chile
mountType Cassegrain focus instrument
observatory Las Campanas Observatory
observatoryOperator Carnegie Institution of Washington
surface form: 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.

Magellan telescope instrumentation suite hasInstrument LDSS3
this entity surface form: LDSS-3