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gptkbp:instance_of
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gptkb:observatory
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gptkbp:bfsLayer
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6
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gptkbp:bfsParent
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gptkb:Palomar
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gptkbp:associated_with
|
gptkb:George_Ellery_Hale
gptkb:Walter_Baade
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gptkbp:collaborations
|
gptkb:Caltech
gptkb:Palomar_Transient_Factory
gptkb:NASA
gptkb:Keck_Observatory
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gptkbp:collection
|
photometric data
|
|
gptkbp:community
|
gptkb:international_collaboration
|
|
gptkbp:conducts_surveys_on
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gptkb:Palomar_Sky_Survey
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|
gptkbp:constructed_in
|
1936
1948
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|
gptkbp:contribution
|
contributed to understanding of the universe
|
|
gptkbp:design
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gptkb:Cassegrain
|
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gptkbp:diameter
|
130 inches
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gptkbp:discovered_by
|
first detection of a black hole
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|
gptkbp:famous_for
|
large-scale surveys of the sky
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|
gptkbp:field_of_study
|
astrophysics
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gptkbp:focus_area
|
1,200 inches
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|
gptkbp:historical_significance
|
one of the largest telescopes of its time
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Palomar 130-inch telescope
|
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gptkbp:influenced_by
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gptkb:Mount_Wilson_Observatory
|
|
gptkbp:innovation
|
improved telescope design
|
|
gptkbp:instrument
|
gptkb:musician
|
|
gptkbp:is_analyzed_in
|
spectral analysis
galaxy formation studies
|
|
gptkbp:is_capable_of
|
deep-sky observations
|
|
gptkbp:is_monitored_by
|
variable stars
|
|
gptkbp:is_observed_in
|
exoplanet transits
|
|
gptkbp:is_reflected_in
|
gptkb:beer
|
|
gptkbp:is_used_for
|
gptkb:observatory
stellar evolution
|
|
gptkbp:is_used_in
|
other telescopes
|
|
gptkbp:legacy
|
influenced future telescope projects
|
|
gptkbp:lens_type
|
equatorial mount
|
|
gptkbp:lighting
|
1948
|
|
gptkbp:location
|
gptkb:Palomar_Observatory
|
|
gptkbp:maintenance
|
ongoing
|
|
gptkbp:notable_achievement
|
mapping the Milky Way
|
|
gptkbp:notable_event
|
Hubble Space Telescope calibration
discovery of new galaxies
|
|
gptkbp:notable_feature
|
large primary mirror
|
|
gptkbp:notable_for
|
discovery of quasars
|
|
gptkbp:notable_models
|
gptkb:Palomar_Observatory
optical telescope
research observatory
|
|
gptkbp:notable_recipients
|
understanding dark matter
|
|
gptkbp:notable_work
|
gptkb:Palomar_Observatory_Sky_Survey
supernova studies
|
|
gptkbp:objective
|
3.3 meters
|
|
gptkbp:open_to_public
|
limited public tours
|
|
gptkbp:operational_status
|
active
|
|
gptkbp:operator
|
Palomar Observatory staff
|
|
gptkbp:owner
|
gptkb:California_Institute_of_Technology
|
|
gptkbp:part_of
|
gptkb:Palomar_Observatory_complex
|
|
gptkbp:project
|
gptkb:Sloan_Digital_Sky_Survey
|
|
gptkbp:receives_funding_from
|
gptkb:Carnegie_Institution_of_Washington
|
|
gptkbp:research
|
photometry
numerous scientific papers
|
|
gptkbp:research_focus
|
gptkb:spacecraft
|
|
gptkbp:resolution
|
0.5 arcseconds per pixel
|
|
gptkbp:significant_event
|
Hubble's law confirmation
|
|
gptkbp:type
|
reflecting telescope
|
|
gptkbp:used_in
|
professional astronomy
|