|
gptkbp:instance_of
|
gptkb:Ninjutsu
|
|
gptkbp:bfsLayer
|
5
|
|
gptkbp:bfsParent
|
gptkb:PHP_Framework_Interoperability_Group_(PHP-FIG)
|
|
gptkbp:contains
|
gptkb:White_Dwarf
|
|
gptkbp:contributed_to
|
Understanding of Neutron Stars
|
|
gptkbp:discovered_by
|
J. A. Hartman
|
|
gptkbp:distance
|
approximately 2,000 light-years
|
|
gptkbp:emissions_standard
|
pulsed
|
|
gptkbp:exhibition
|
ATNF Pulsar Catalog
|
|
gptkbp:field
|
gptkb:observatory
gptkb:battle
|
|
gptkbp:first_appearance
|
gptkb:1974
|
|
gptkbp:frequency
|
43.3 Hz
|
|
gptkbp:has_lore
|
gptkb:battle
|
|
gptkbp:has_luminosity
|
high
|
|
gptkbp:historical_period
|
0.0231 seconds
|
|
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:physicist
|
|
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:Ninjutsu
|
|
gptkbp:is_studied_in
|
Gravitational Wave Detection
Multiple Research Teams
|
|
gptkbp:is_used_in
|
Astrophysical Research
|
|
gptkbp:lighting
|
gptkb:battle
|
|
gptkbp:location
|
Constellation of Cassiopeia
|
|
gptkbp:noise_level
|
gptkb:battle
|
|
gptkbp:orbital_period
|
0.5 days
|
|
gptkbp:research
|
Radio Astronomy
Pulsar Timing Arrays
Neutron Star Physics
|
|
gptkbp:significance
|
gptkb:High
|
|
gptkbp:type
|
Millisecond Pulsar
|
|
gptkbp:universe
|
Potentially
|
|
gptkbp:year_created
|
gptkb:1974
|