|
13:30 - 16:30
|
the Broad Line Region |
(+)
|
|
14:00 - 14:15 |
› The iron lines in spectra of Active Galactic Nuclei: a two-component model - Jelena Kovačević-Dojčinović, Astronomical Observatory Belgrade |
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14:15 - 14:30 |
› Spiral Arms in Broad-line Regions of Active Galactic Nuclei - Pu Du, Institute of High Energy Physics, Chinese Academy of Sciences |
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|
14:30 - 14:45 |
› Resolving close binaries of supermassive black holes in the era of optical interferometry - Yu-Yang Songsheng, Institute of High Energy Physics, Chinese Academy of Sciences |
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|
14:45 - 15:00 |
› Resolving the BLR with VLTI/GRAVITY - Eckhard Sturm, Max Planck Institute for Extraterrestrial Physics |
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15:00 - 15:15 |
› Confronting AGN outflow and accretion models with SDSS quasar demographics - Matthew Temple, Universidad Diego Portales |
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15:30 - 15:45 |
› Spectroastrometric Reverberation Mapping of Broad-line Region - Yan-Rong Li, Institute of High Energy Physics, Chinese Academy of Sciences |
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|
15:45 - 16:00 |
› Probing the size and kinematics of the quasar broad line region with gravitational microlensing - Damien Hutsemekers, University of Liege |
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16:00 - 16:15 |
› Origin of the Changing-state AGNs - Keiichi Wada, Kagoshima University |
|
|
16:15 - 16:30 |
› Sub-pc supermassive binary black holes in the active galactic nuclei: Broad line shapes and variability - Luka C. Popovic, Astronomical Observatory, Volgina 7, 11150 Belgrade - Dragana Ilic, Department of Astronomy, University of Belgrade—Faculty of Mathematics, Studentski trg 16, 11000 Belgrade, |
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|
16:30 - 17:15
|
Sub-parsec scales and jets |
(+)
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|
16:30 - 16:45 |
› Blazars' variability on intranight to year-long timescales using the ZTF survey - Vibhore Negi |
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|
16:45 - 17:00 |
› Probing Long-term Variations of Blazars Using Multi-wavelength Observations - Krishna Mohana A, Aryabhatta Research Institute of Observational Sciences (ARIES),Manora Peak, Nainital - 263001, Uttarakhand, India |
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|
17:00 - 17:15 |
› Intranight optical variability of low-mass active galactic nuclei: a pointer to blazar-like activity - Krishan Chand, Aryabhatta Research Institute of observational sciencES (ARIES) |
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17:15 - 17:45
|
Discussion |
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