8–13 Sept 2019
Europe/Rome timezone
All inquiries about receipts for the payment of the conference fee and/or dinner should be addressed to: a.vriz@fondazionealmamater.it, d.bordignon@fondazionealmamater.it

Size of the ISCO and hot corona from gravitational lensing

11 Sept 2019, 14:30
15m

Speaker

Dr George Chartas (College of Charleston)

Description

We present current X-ray observations and simulations showing how gravitational lensing is used to infer the structure near the event horizons of black holes, constrain the spin of the supermassive black hole and its evolution over cosmic time and test general relativity in the strong-gravity regime.
We also show how these observations can be expanded to a statistically large sample of z = 0.5-5 lensed quasars with the predicted discovery by LSST of > 4,000 additional gravitationally lensed systems and with a next generation X-ray telescope having a spatial resolution of <?0.5arcsec to resolve the lensed images and a collecting area of >? 0.5 m^2 at 1 keV.

Affiliation College of Charleston
Topic Active Galactic Nuclei: accretion physics and evolution across cosmic time

Primary author

Dr George Chartas (College of Charleston)

Presentation materials