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gptkbp:instance_of
|
gptkb:Apache_Pulsar
|
|
gptkbp:conducts_research_on
|
Pulsar Timing Arrays
Neutron Star Physics
|
|
gptkbp:contains_star
|
gptkb:White_Dwarf
|
|
gptkbp:contributes_to
|
Understanding of Neutron Stars
|
|
gptkbp:discovered_by
|
J. A. Hartman
|
|
gptkbp:discovery_year
|
gptkb:1974
|
|
gptkbp:distance_from_earth
|
approximately 2,000 light-years
|
|
gptkbp:emissions_standard
|
pulsed
|
|
gptkbp:exhibition
|
ATNF Pulsar Catalog
|
|
gptkbp:field
|
gptkb:astronomy
|
|
gptkbp:first_appearance
|
gptkb:1974
|
|
gptkbp:has_field
|
gptkb:Yes
|
|
gptkbp:has_gravitational_waves
|
Potentially
|
|
gptkbp:has_luminosity
|
high
|
|
gptkbp:has_pulsar_wind
|
gptkb:Yes
|
|
gptkbp:has_timing_noise
|
gptkb:Yes
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
PSR-23
|
|
gptkbp:is_analyzed_in
|
Relativity
Timing Precision
|
|
gptkbp:is_associated_with
|
Pulsar Timing Arrays
|
|
gptkbp:is_atype_of
|
gptkb:Supernova
|
|
gptkbp:is_considered
|
Astrophysics Models
|
|
gptkbp:is_involved_in
|
Astrophysical Phenomena
|
|
gptkbp:is_monitored_by
|
Various Observatories
|
|
gptkbp:is_observed_in
|
Radio Telescopes
|
|
gptkbp:is_part_of
|
Binary System
|
|
gptkbp:is_related_to
|
gptkb:Apache_Pulsar
|
|
gptkbp:is_studied_for
|
Gravitational Wave Detection
|
|
gptkbp:is_studied_in
|
Multiple Research Teams
|
|
gptkbp:is_used_in
|
Astrophysical Research
|
|
gptkbp:lighting
|
gptkb:Yes
|
|
gptkbp:location
|
Constellation of Cassiopeia
|
|
gptkbp:orbital_period
|
0.5 days
|
|
gptkbp:period
|
0.0231 seconds
|
|
gptkbp:research
|
Radio Astronomy
|
|
gptkbp:significance
|
gptkb:High
|
|
gptkbp:spin_frequency
|
43.3 Hz
|
|
gptkbp:type
|
Millisecond Pulsar
|
|
gptkbp:bfsParent
|
gptkb:PHP_Framework_Interoperability_Group_(PHP-FIG)
|
|
gptkbp:bfsLayer
|
7
|