Módszerek összehasonlítása

	Rotációs görbe analízis	Pulzár időzítési tömb
Tudományterület	Csillagászat	Csillagászat
Módszercsalád	Process / pipeline	Process / pipeline
Keletkezés éve	1970	1979
Megalkotó	Vera Rubin	Stephen Detweiler
Típus	Observational kinematic method	Observational timing method
Alapmű	Vera C. Rubin & W. Kent Ford Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. Astrophysical Journal, 159, 379-403.	Sazhin, M. V. (1978). Opportunities for detecting ultralong gravitational waves. Soviet Astronomy, 22, 36-38.
Alternatív nevek	Galactic Rotation Curves, Rotation Curve Method, Velocity Curve Analysis	PTA, Millisecond Pulsar Timing, Pulsar Timing Residuals
Kapcsolódó	3	3
Összefoglaló	Galaxy rotation curve analysis is the technique of measuring how orbital velocities change with distance from the center of a galaxy. Pioneered by Vera Rubin and W. Kent Ford Jr. in 1970, rotation curves revealed one of astronomy's great mysteries: galaxies rotate too fast to be held together by their visible stars alone, providing direct evidence for dark matter.	A pulsar timing array uses multiple millisecond pulsars as a distributed network of gravitational wave detectors across the galaxy. Proposed theoretically by Stephen Detweiler in 1979, this method exploits the extraordinary timing precision of pulsars to detect the subtle spacetime distortions caused by gravitational waves. In 2023, the first evidence for a stochastic background of gravitational waves was announced using pulsar timing arrays.