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Gravitational microlensing is an astronomical phenomenon caused by the gravitational lens effect. It can be used to detect objects that range from the mass of a planet to the mass of a star, regardless of the light they emit. Typically, astronomers can only detect bright objects that emit much light (stars) or large objects that block background light…
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microlensing source lens events star mass event einstein light objects time two displaystyle planet stars lensing images used parallax needed
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Gravitational microlensing | is a | astronomical phenomenon caused by the gravitational lens effect | 0.90 | text |
| brown dwarfs | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| red dwarfs | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| planets | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| white dwarfs | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| neutron stars | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| black holes | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| and massive compact halo objects | instance of | It enables the study of the population of faint or dark objects | 0.80 | text |
| the Hubble Space Telescope | instance of | that the displacement of light by the lens can be resolved with a high resolution telescope | 0.80 | text |
| the transit method | instance of | was reported.Comparing this method of detecting extrasolar planets with other techniques | 0.80 | text |
| one advantage is that the intensity of the planetary deviation does not depend on the planet mass as strongly as effects in other techniques do | instance of | was reported.Comparing this method of detecting extrasolar planets with other techniques | 0.80 | text |
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