Timeline for Can weak gravitational lensing or microlensing-induced wavefront distortion limit resolution of absurdly large aperture telescopes?
Current License: CC BY-SA 4.0
8 events
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| Apr 4, 2019 at 3:40 | history | edited | uhoh | CC BY-SA 4.0 |
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| Apr 2, 2019 at 16:11 | answer | added | cms | timeline score: 1 | |
| Apr 1, 2019 at 14:04 | history | edited | uhoh | CC BY-SA 4.0 |
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| Jan 10, 2019 at 3:01 | history | tweeted | twitter.com/StackAstronomy/status/1083196995895001090 | ||
| Jan 9, 2019 at 18:19 | comment | added | Carl Witthoft | Adaptive optic systems largely depend on a known "clean" reference source, so if your telescopes FoV can see even one star whose output is subject to significant grav microlensing then it could be corrected. | |
| Jan 9, 2019 at 2:27 | history | edited | uhoh | CC BY-SA 4.0 |
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| Jan 9, 2019 at 0:53 | history | edited | uhoh | CC BY-SA 4.0 |
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| Jan 9, 2019 at 0:41 | history | asked | uhoh | CC BY-SA 4.0 |