gptkbp:instance_of
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gptkb:observatory
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gptkbp:aims_to
|
star formation
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gptkbp:analyzes
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galactic structures
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gptkbp:collaborated_with
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gptkb:spacecraft
international research teams
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gptkbp:collaborates_with
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various universities
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gptkbp:conducted
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gptkb:NASA
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gptkbp:contributed_to
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gptkb:spacecraft
understanding of dark matter
the study of cosmic dust
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gptkbp:discovered_by
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new galaxy types
exotic galaxy features
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gptkbp:focuses_on
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nearby galaxies
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gptkbp:has_influence_on
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galactic dynamics
galaxy clusters
star formation rates
galaxy formation processes
galaxy interactions
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gptkbp:has_written
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over 100 galaxies
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https://www.w3.org/2000/01/rdf-schema#label
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Spitzer Infrared Nearby Galaxies Survey
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gptkbp:includes
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infrared observations
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gptkbp:instrument
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gptkb:Spitzer_Space_Telescope
spectrometers
infrared cameras
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gptkbp:is_a
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gptkb:spacecraft
major astronomical project
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gptkbp:is_analyzed_in
|
gptkb:interstellar_medium
galactic chemical evolution
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gptkbp:is_associated_with
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gptkb:NASA's_Great_Observatories_program
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gptkbp:is_cited_in
|
numerous research papers
|
gptkbp:is_involved_in
|
the study of galaxy mergers
multi-wavelength studies
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gptkbp:is_part_of
|
gptkb:NASA's_astrophysics_program
Spitzer Space Telescope mission
|
gptkbp:is_recognized_for
|
its innovative techniques
its contributions to astronomy
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gptkbp:is_studied_in
|
galactic evolution
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gptkbp:is_supported_by
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gptkb:NASA's_Science_Mission_Directorate
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gptkbp:is_utilized_in
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stellar evolution studies
astronomers worldwide
the study of cosmic microwave background
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gptkbp:launched
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gptkb:2003
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gptkbp:provides_information_on
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gptkb:starburst_galaxies
galaxy formation
galaxy luminosity functions
galaxy redshift measurements
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gptkbp:recognizes
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dusty galaxies
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gptkbp:research
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gptkb:active_galactic_nuclei
stellar populations
galaxy morphology
galactic outflows
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gptkbp:research_interest
|
infrared astronomy
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gptkbp:result
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gptkb:academic_journal
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gptkbp:significance
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gptkb:planet
|
gptkbp:targets
|
local group galaxies
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gptkbp:utilizes
|
infrared wavelengths
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gptkbp:bfsParent
|
gptkb:SIRTF
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gptkbp:bfsLayer
|
5
|