The AGN-galaxy coevolution : comparing theory and observations
23-24 Apr 2026 Paris (France)
FR
EN
Login
Lost password ?
Create account
Main menu
Home
Registration
Submit
List of Participants
Planning
Code of conduct
HELP
@ Contact
Planning
Week
Thu. 23
Fri. 24
List
Thu. 23
Fri. 24
09:00
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
18:00
19:00
20:00
21:00
Welcome by Philippe, President of the Observatoire de Paris
9:30 - 9:40 (10min)
Welcome by Philippe, President of the Observatoire de Paris
Welcome by Françoise Combes, President of the Académie des Sciences
9:40 - 9:50 (10min)
Welcome by Françoise Combes, President of the Académie des Sciences
Evolution of BH-galaxy scaling relations
9:50 - 10:30 (40min)
Evolution of BH-galaxy scaling relations
Marta Volonteri
Data-driven constraints on the coevolution of supermassive black holes and their host
10:30 - 11:10 (40min)
Data-driven constraints on the coevolution of supermassive black holes and their host
Daniel Roberts
Coffee break
11:10 - 11:40 (30min)
Coffee break
The diverse pathways of supermassive black hole–galaxy co-evolution
11:40 - 12:20 (40min)
The diverse pathways of supermassive black hole–galaxy co-evolution
James Aird
What regulates black hole growth and star formation? Environmental and structural drivers across cosmic time
12:20 - 13:00 (40min)
What regulates black hole growth and star formation? Environmental and structural drivers across cosmic time
Georgios Mountrichas
Lunch
13:00 - 14:30 (1h30)
Lunch
Black hole-host galaxy coevolution in IMBH regime as seen by Hubble Space Telescope: a critical role of mergers
14:30 - 15:00 (30min)
Black hole-host galaxy coevolution in IMBH regime as seen by Hubble Space Telescope: a critical role of mergers
Kirill Grishin
Deep Learning techniques for the automatic detection of dual AGN in large-scale surveys
15:00 - 15:30 (30min)
Deep Learning techniques for the automatic detection of dual AGN in large-scale surveys
Chloe Mahe
Stellar Black holes with the improved code Pegase.3
15:30 - 16:00 (30min)
Stellar Black holes with the improved code Pegase.3
Brigitte Rocca-Volmerange
Coffee break
16:00 - 16:30 (30min)
Coffee break
Discussion
16:30 - 18:00 (1h30)
Discussion
The Perrault building
18:00 - 19:00 (1h)
The Perrault building
Visit of the Observatory
Cocktail dinner
19:00 - 21:00 (2h)
Cocktail dinner
Resolving molecular tori with ALMA
9:00 - 9:40 (40min)
Resolving molecular tori with ALMA
Francoise Combes
The drivers of quasar winds: strong optical-to-UV emission is key regardless of X-ray strength
9:40 - 10:20 (40min)
The drivers of quasar winds: strong optical-to-UV emission is key regardless of X-ray strength
Ami Rankine
Coffee break
10:20 - 10:50 (30min)
Coffee break
Radiation-ionization hydrodynamic simulations of AGN line-driven winds
10:50 - 11:30 (40min)
Radiation-ionization hydrodynamic simulations of AGN line-driven winds
Nicolas Scepi
Galactic Centers as Large Scale Feedback Machines
11:30 - 12:00 (30min)
Galactic Centers as Large Scale Feedback Machines
Daniel Maschmann
The heating efficiency of AGN
12:00 - 12:40 (40min)
The heating efficiency of AGN
Andrea Cattaneo
Lunch
12:40 - 14:00 (1h20)
Lunch
Outflow Demographics and Over-massive black hole eROSITA quasar
14:00 - 14:40 (40min)
Outflow Demographics and Over-massive black hole eROSITA quasar
Johannes Buchner
The quenching histories of Type-1 and Type-2 AGN host galaxies
14:40 - 15:20 (40min)
The quenching histories of Type-1 and Type-2 AGN host galaxies
Sagyadri Krishna
AGN feedback in galaxy groups and clusters
15:20 - 16:00 (40min)
AGN feedback in galaxy groups and clusters
Stefano Ettori
Coffee break
16:00 - 16:30 (30min)
Coffee break
How do jets heat galaxy cluster atmospheres? A XRISM perspective
16:30 - 17:10 (40min)
How do jets heat galaxy cluster atmospheres? A XRISM perspective
Brian McNamara
Discussion
17:10 - 18:10 (1h)
Discussion
Privacy
|
Accessibility
Loading...