gptkbp:instance_of
|
gptkb:musician
|
gptkbp:bfsLayer
|
3
|
gptkbp:bfsParent
|
gptkb:Hubble_Space_Telescope
gptkb:observatory
|
gptkbp:archives
|
gptkb:Mikulski_Archive_for_Space_Telescopes
|
gptkbp:data_type
|
FITS
|
gptkbp:designed_by
|
gptkb:NASA
|
gptkbp:discovered_by
|
gptkb:Monarch
gptkb:interstellar_medium
cosmic microwave background
galaxy mergers
star formation rates
structure of the universe
exoplanet atmospheres
chemical composition of stars
stellar populations in galaxies
black hole growth
evolution of galaxies
formation of planetary systems
|
gptkbp:frequency
|
1100 to 10000 Å
|
gptkbp:function
|
gptkb:musician
|
gptkbp:has_symbol
|
52 arcseconds
|
https://www.w3.org/2000/01/rdf-schema#label
|
Space Telescope Imaging Spectrograph
|
gptkbp:instrument
|
gptkb:musician
|
gptkbp:is_analyzed_in
|
photometric calibration
spectral calibration
|
gptkbp:is_part_of
|
gptkb:Hubble_Space_Telescope
|
gptkbp:launch_date
|
1997-04-24
|
gptkbp:launched
|
gptkb:Hubble_Space_Telescope
|
gptkbp:lighting
|
1997-05-20
|
gptkbp:mission_duration
|
15 years
|
gptkbp:operated_by
|
gptkb:Space_Telescope_Science_Institute
|
gptkbp:operates_in
|
visible light
ultraviolet
|
gptkbp:primary_source
|
study distant galaxies
analyze exoplanet atmospheres
examine stellar populations
|
gptkbp:provides_information_on
|
gptkb:observatory
|
gptkbp:radar
|
ultraviolet to near-infrared
|
gptkbp:resolution
|
high resolution
|
gptkbp:supports
|
gptkb:spacecraft
galaxy formation
stellar evolution
|
gptkbp:technology
|
CCD detectors
|