|
gptkbp:instance_of
|
gptkb:musician
|
|
gptkbp:bfsLayer
|
5
|
|
gptkbp:bfsParent
|
gptkb:VLT_(Very_Large_Telescope)
gptkb:VLT
|
|
gptkbp:adapted_into
|
various observational techniques
|
|
gptkbp:collaborated_with
|
international research projects
|
|
gptkbp:collaborates_with
|
various astronomical projects
|
|
gptkbp:collaborations
|
other observatories
|
|
gptkbp:contributed_to
|
studies of star formation
|
|
gptkbp:developed_by
|
gptkb:European_Southern_Observatory
gptkb:Chile
|
|
gptkbp:enables
|
detection of exoplanets
|
|
gptkbp:enhances
|
spectroscopic studies
|
|
gptkbp:exhibited_at
|
astronomy conferences
|
|
gptkbp:frequency
|
0.9 to 5.5 micrometers
|
|
gptkbp:has_ability
|
multi-object spectroscopy
|
|
gptkbp:has_feature
|
high dynamic range
|
|
gptkbp:has_programs
|
gptkb:planet
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
CRIRES
|
|
gptkbp:improves
|
sensitivity of observations
|
|
gptkbp:instrument
|
high-resolution imaging
highly sensitive detectors
|
|
gptkbp:is_associated_with
|
high-energy astrophysics
|
|
gptkbp:is_capable_of
|
detecting faint objects
|
|
gptkbp:is_compatible_with
|
various telescopes
|
|
gptkbp:is_designed_for
|
infrared spectroscopy
|
|
gptkbp:is_documented_in
|
scientific publications
astronomical databases
|
|
gptkbp:is_evaluated_by
|
peer-reviewed journals
scientific accuracy
|
|
gptkbp:is_incorporated_in
|
various research studies
|
|
gptkbp:is_integrated_with
|
VLT's adaptive optics system
|
|
gptkbp:is_involved_in
|
stellar evolution studies
|
|
gptkbp:is_known_for
|
its precision in measurements
|
|
gptkbp:is_linked_to
|
various scientific discoveries
|
|
gptkbp:is_part_of
|
gptkb:VLT_instrument_suite
gptkb:VLT_Observatory
global astronomical initiatives
|
|
gptkbp:is_prominent_in
|
modern astronomy.
|
|
gptkbp:is_promoted_by
|
ESO publications
|
|
gptkbp:is_recognized_by
|
astronomical societies
|
|
gptkbp:is_recognized_for
|
its contribution to astrophysics
|
|
gptkbp:is_subject_to
|
regular upgrades
|
|
gptkbp:is_supported_by
|
gptkb:Research_Institute
grants and funding
|
|
gptkbp:is_used_by
|
gptkb:Very_Large_Telescope
|
|
gptkbp:is_used_for
|
studying stellar atmospheres
|
|
gptkbp:is_used_in
|
planetary science research
|
|
gptkbp:is_utilized_in
|
astronomers worldwide
spectral line observations
|
|
gptkbp:lighting
|
gptkb:2006
|
|
gptkbp:operated_by
|
ESO staff
|
|
gptkbp:operates_in
|
near-infrared spectrum
|
|
gptkbp:performed_by
|
understanding cosmic phenomena
|
|
gptkbp:provides
|
high-resolution spectra
|
|
gptkbp:receives_funding_from
|
gptkb:legislation
|
|
gptkbp:resolution
|
up to 100,000
|
|
gptkbp:social_responsibility
|
chemical composition analysis
|
|
gptkbp:supports
|
observations of distant galaxies
|
|
gptkbp:utilizes
|
adaptive optics
|