Statements (50)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:camera
gptkb:astronomy |
gptkbp:contributes_to |
cosmology research
|
gptkbp:data_type |
digital images
|
gptkbp:designed_by |
gptkb:NASA
|
gptkbp:filter_type |
broadband and narrowband filters
|
gptkbp:has_achievements |
contributed to the understanding of cosmic expansion
aided in the study of gravitational lensing captured images of distant supernovae contributed to the discovery of exoplanets discovered thousands of galaxies enabled multi-wavelength astronomy enhanced knowledge of star formation rates facilitated the study of the early universe helped in the search for dark energy improved measurements of galaxy distances mapped dark matter distribution provided data for the Hubble Legacy Archive provided insights into galaxy evolution supported the study of galaxy mergers contributed to the understanding of cosmic microwave background |
gptkbp:has_component |
gptkb:Planetary_Camera_2
Infrared Channel Wide Field Channel |
https://www.w3.org/2000/01/rdf-schema#label |
Advanced Camera for Surveys
|
gptkbp:launched_in |
gptkb:2002
|
gptkbp:notable_artists |
gptkb:Abell_370
gptkb:Hubble_Deep_Field_South gptkb:Hubble_Ultra_Deep_Field the Cosmic Evolution Survey |
gptkbp:operated_by |
gptkb:Space_Telescope_Science_Institute
|
gptkbp:operational_status |
decommissioned
|
gptkbp:primary_function |
wide-field imaging
|
gptkbp:provides_information_on |
galaxy formation studies
|
gptkbp:replaced_by |
gptkb:Wide_Field_Camera_3
|
gptkbp:resolution |
0.05 arcseconds
0.05 arcseconds per pixel 4096 x 4096 pixels |
gptkbp:sensitivity |
UV to near-infrared
|
gptkbp:successor |
gptkb:Wide_Field_Camera_3
|
gptkbp:used_for |
gptkb:exoplanet
galaxy cluster studies stellar population studies supernova observations dark matter studies |
gptkbp:uses |
gptkb:Hubble_Space_Telescope
|
gptkbp:view |
202 arcminutes
|
gptkbp:bfsParent |
gptkb:Hubble_Space_Telescope
gptkb:astronomy |
gptkbp:bfsLayer |
4
|