Conveners
AGN Dynamics
- chair: Andjelka Kovacevic
Alister Graham
(Swinburne University of Technology)
24/07/2024, 12:30
The scaling relations between the mass of black holes and the properties of galaxies are becoming more specific to the different galaxy morphologies. I will present an update on the current status of these relations and explain how we can refine the virial factor(s), f, used to calculate black hole masses from AGN virial products.
Benedict Rouse
(pontificia universidad católica de chile)
24/07/2024, 12:50
We employ natural language processing algorithms with attention, repurposed to receive QSO spectra to predict unseen spectra, broad lines, and super massive black hole masses. We find that the trained algorithm is able to reproduce with high significance masked broad lines and/or continua in QSO spectra, highlighting an ability to learn from and leverage physical information imprinted amongst...
