Statements (50)
Predicate | Object |
---|---|
gptkbp:instanceOf |
gptkb:Sultan
|
gptkbp:age |
approximately 1 billion years
|
gptkbp:analyzes |
requires advanced data analysis techniques
|
gptkbp:assigneeCountry |
none
|
gptkbp:associatedWith |
none
|
gptkbp:beam |
potential source
|
gptkbp:collaborations |
involved in collaborative research projects
international astrophysics collaboration |
gptkbp:collection |
ongoing data collection efforts
|
gptkbp:companionPlants |
none
|
gptkbp:dataUsage |
publicly available
|
gptkbp:established |
gptkb:John_W._Taylor
|
gptkbp:field |
high
|
gptkbp:foughtAgainst |
included in the ATNF pulsar catalog
|
gptkbp:frequency |
high
|
gptkbp:geographicalFeature |
l=30.0,_b=-10.0
|
gptkbp:grapeVarieties |
none
|
gptkbp:hasAlumni |
part of pulsar timing array projects
|
gptkbp:hasPopulation |
part of the pulsar population studies
|
gptkbp:historicalResearch |
ongoing studies planned
used in astrophysics research |
https://www.w3.org/2000/01/rdf-schema#label |
PSR A
|
gptkbp:isSimilarTo |
used for precise timing measurements
|
gptkbp:length |
approximately 2000 light years
|
gptkbp:lighting |
high
|
gptkbp:location |
Milky Way Galaxy
|
gptkbp:matingSystem |
not a binary system
|
gptkbp:model |
supports theoretical models of neutron stars
|
gptkbp:officialResidence |
radio astronomy
difficult to observe due to distance utilizes advanced observational techniques |
gptkbp:period |
low
|
gptkbp:publications |
numerous scientific publications exist
|
gptkbp:PWM |
yes
|
gptkbp:radar |
limited
|
gptkbp:releaseYear |
1993
|
gptkbp:researchFocus |
none
|
gptkbp:researchInterest |
used in various research applications
|
gptkbp:scientificName |
recognized by the scientific community
helps understand extreme physics important for studying neutron stars related to high-energy astrophysical phenomena |
gptkbp:stations |
1.4 GHz
|
gptkbp:timePeriod |
5.76 milliseconds
|
gptkbp:torque |
unknown
|
gptkbp:trainTypes |
standard neutron star
|
gptkbp:type |
millisecond pulsar
|
gptkbp:vision |
formed from supernova explosion
|
gptkbp:visitedBy |
Arecibo Observatory
|
gptkbp:weight |
approximately 1.4 solar masses
|