Measuring accretion disk sizes of lensed quasars with microlensing time delay in multi-band light curves
Time-delay cosmography in strongly lensed quasars offers an independent way of measuring the Hubble constant, H 0 . However, it has been proposed that the combination of microlensing and source-size effects, also known as microlensing time delay, can potentially increase the uncertainty in time-dela...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2021-03, Vol.647, p.A115 |
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Sprache: | eng |
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