International Pulsar Timing Array
E607256
The International Pulsar Timing Array is a global collaboration of radio observatories that precisely monitor millisecond pulsars to detect low-frequency gravitational waves and study fundamental physics.
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
astronomy collaboration
ⓘ
gravitational-wave experiment ⓘ pulsar timing array ⓘ scientific collaboration ⓘ |
| abbreviation | IPTA NERFINISHED ⓘ |
| aimsTo |
constrain the gravitational-wave background
ⓘ
detect low-frequency gravitational waves ⓘ probe supermassive black hole binaries ⓘ study fundamental physics ⓘ test general relativity ⓘ |
| collaboratesWith | radio observatories worldwide ⓘ |
| collaborationType | consortium of regional pulsar timing arrays ⓘ |
| community | international astrophysics community ⓘ |
| coordinates | joint data analysis among member arrays ⓘ |
| dataType |
pulsar timing residuals
ⓘ
radio telescope observations ⓘ |
| field |
astrophysics
ⓘ
gravitational-wave astronomy ⓘ radio astronomy ⓘ |
| focusesOn | nanohertz frequency band of gravitational waves ⓘ |
| goal | first direct detection of nanohertz gravitational waves ⓘ |
| hasMember |
European Pulsar Timing Array
NERFINISHED
ⓘ
North American Nanohertz Observatory for Gravitational Waves NERFINISHED ⓘ Parkes Pulsar Timing Array NERFINISHED ⓘ |
| method |
long-term monitoring of pulsars
ⓘ
precise timing of radio pulses ⓘ |
| monitors | an array of precisely timed pulsars ⓘ |
| observes |
millisecond pulsars in the Milky Way
ⓘ
radio pulsars ⓘ |
| produces | combined pulsar timing datasets ⓘ |
| requires |
high-precision timing instrumentation
ⓘ
long-baseline observations over many years ⓘ |
| scale | global ⓘ |
| studies |
cosmology
ⓘ
equation of state of ultra-dense matter ⓘ nanohertz gravitational waves ⓘ stochastic gravitational-wave background ⓘ supermassive black hole mergers ⓘ |
| testsTheory |
alternative theories of gravity
ⓘ
general relativity in the low-frequency regime ⓘ |
| timeScale | multi-year monitoring ⓘ |
| uses |
millisecond pulsars
ⓘ
pulsar timing ⓘ |
| usesInstrument | large radio telescopes ⓘ |
| usesTechnique |
Bayesian data analysis methods
ⓘ
correlation of timing residuals between pulsars ⓘ noise modeling in pulsar timing data ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.