Using NASA data to determine if observation indicates that an exoplanet was located
Discovering exoplanets is approached with several techniques:
- Astrometry (1) - star wobbles compared to nearby stars
- Disk Kinematics (1) - looking for gaps in material around star (where it collected into an object
- Eclipse Timing Variations (16) - a binary star system where eclipsing has variation due to other object(s)
- Imaging (50) - removing the star's light from the image to find what remains
- Microlensing (96) - light from the star is gravitationally bent
- Orbital Brightness Modulation (6) - the brightness of the star changes because of reflected light off object
- Pulsar Timing (7) - slight regular variation in pulsar bursts due to other objects
- Pulsation Timing Variations (2) - Doppler shift in bursts from a pulsar
- Radial Velocity (810) - star's motion displays a wobble
- Transit (3191) - an object block some of the star's light
- Transit Timing Variations (21) - measuring variations in the transit times to detect other objects
https://en.wikipedia.org/wiki/List_of_exoplanet_search_projects
https://en.wikipedia.org/wiki/Sagittarius_Window_Eclipsing_Extrasolar_Planet_Search
https://en.wikipedia.org/wiki/CoRoT#List_of_planets_discovered
https://en.wikipedia.org/wiki/Transiting_Exoplanet_Survey_Satellite
https://en.wikipedia.org/wiki/CHEOPS