All attendees are expected to show respect and courtesy to other attendees and staff, and to adhere to the NAM Code of Conduct.
Parallel sessions
Sessions
The multi-wavelength picture of AGN, from (sub-)kpc to cosmic scales
Extragal3
Studying AGN and their host galaxies in detail is a crucial step to understand the physical processes driving and regulating the growth of supermassive black holes (SMBHs), the extent and impact of their energetic feedback on the surrounding environment and thus on the star-formation activity within the host galaxy, and the overall role of AGN in shaping galaxies over cosmic time. Complementing earlier high-resolution optical, near-IR and X-ray instruments (e.g. HST, Chandra, XMM-Newton, Herschel), the unprecedented resolution and sensitivity provided by the latest generation of telescopes (e.g. VLT/MUSE, VLTI/Matisse, ALMA and the SKA precursors/pathfinders) have opened up the new regimes that have started revolutionising our view of the AGN-host galaxy interplay, leading to a clearer picture across different AGN populations/host galaxy types. A great diversity of physical phenomena have been uncovered in recent years by multi-wavelength spectroscopy and imaging, including ultra-fast outflows, warm absorbers, nuclear bars, massive multi-phase (i.e. ionized, neutral and molecular) outflows and cold gas inflows. All this provides clear evidence of a connection between the AGN fuelling/feedback processes and their host galaxy evolution, although the complexity of these phenomena, as well as the lack of statistically meaningful and conclusive studies, still leave many open questions. With the advent of next-generation telescopes (e-ROSITA, JWST, SKA, Athena. SPICA), we are at the brink of an exciting new era of discoveries in terms of AGN physics, with deep insights that will translate to the broader field of galaxy evolution. The aim of this meeting is to summarise our state of knowledge on this topic in both the nearby and high-redshift Universe. We will focus on the results obtained from the wealth of multi-wavelength observations acquired over the past few years, including complementary theoretical understanding, and look towards future perspectives in the context of forthcoming facilities. We plan to have three 90 minute blocks, which will be organised as follows: 1) AGN feeding and nuclear geometry. This session will focus on the current observational and theoretical understanding of the accretion flow onto central SMBHs and inner geometry across different AGN populations in the nearby Universe. 2) Circumnuclear environment and AGN feedback. This session will focus on the different types of AGN feedback (i.e. radiative and/or kinetic) and the impact that these can have on the circum-nuclear material and the host galaxy as a whole. 3) AGN/host galaxy interplay across cosmic times. This session will focus on studies that link AGN activity to the broader picture of galaxy evolution and the impact of AGN feedback processes on host galaxy properties over cosmic time.
Ilaria Ruffa, Timothy A. Davis, Robert A. Laing, Christopher Harrison, David Rosario, Carolin Villforth, Myrto Symeonidis, James Aird
Mon. 09:00-10:00 / Mon 14:30-16:00 / Mon. 16:30-18:00
09.00-09.20 Ismael Garcia-Bernete: Torus and dusty polar outflow dependence on AGN properties [invited]
09.20-09.30 Alba Vega Alonso Tetilla: Probing the relative roles of evolution, orientation and multi-scale gas distributions in shaping the obscuration of Black Holes through cosmic time
09.30-09.40 Clara Marie Pennock: Discovery of a class of super-AGN behind the Magellanic Clouds using multiwavelength data and unsupervised machine learning
09.40-09.50 Jacob Elford: The Link Between Circumnuclear Molecular Gas Reserviors and Active Galactic Nuclei Fuelling
09.50-10.00 Robbie Webbe: X-ray variability in a super-soft AGN -- Oscillation or Eruption?
10.00-10.10 Victoria Fawcett: Why is colour special? Identifying fundamental differences between red and blue quasars
10.10-10.20 Jiachen Jiang: A highly accreting low-mass black hole hidden in the dust
10.20-10.22 Cressida Cleland: Optical variability as a tracer for low-mass AGN and a precursor to reduced star formation
10.22-10.24 Mohammed Al-Fadhli: The morphology of the active galactic nucleus and its impact on accretion flows and relativistic jets
10.24-10.26 Jan Scholtz: Detection of massive molecular and dust reservoirs around z~2 extremely red quasars: CGM enrichment by quasar-driven outflows
10.26-10.28 Darshan Kakkad: The impact of AGN outflows on star formation at cosmic noon using spatially resolved AO-assisted observations: Insights from the SUPER survey
10.28-10.30 Ricarda Beckmann: The impact of cosmic rays on how AGN jets regulate cluster cooling flows
14.30-14.40 Jan Scholtz: Do powerful large-scale AGN outflows really suppress star formation?
14.40-14.50 Luke Holden: Precise Diagnostics of Multiphase Outflows in the Nearby Seyfert 2 Galaxy IC 5063
14.50-15.00 Gareth Jones: Evidence for Gaseous Halos Around AGN at Cosmic Noon from ALMA CO(3-2) Observations
15.00-15.10 Darshan Kakkad: Scaling relations between multi-phase outflows and AGN across cosmic time
15.10-15.20 Alyssa Drake: Fuelling Quasars at the edge of the Epoch of Reionisation
15.20-15.30 Alexander Richings: Unravelling the physics of multiphase AGN winds through emission line tracers
15.30-15.40 Samuel Ruthven Ward: The Impact of Quasars from Sub-kpc to Galaxy-wide Scales
15.40-16.00 Qingling Ni: The link between AGNs and their host galaxies across cosmic time [invited]
16.30-16.40 Rebecca Smethurst: Which non-merger mechanisms are powering the majority of SMBH growth and AGN feedback? A study with KCWI
16.40-16.50 Stephen Wilkins: The emergence of the first AGN
16.50-17.00 Yana Khusanova: The properties of the host galaxies of radio-loud quasars at z>6
17.00-17.10 Imogen Whittam: Exploring radio-loud AGN with the MIGHTEE survey
17.10-17.20 Brendan Webster: Jet Feedback in a sample of Galaxy Scale Jets from the LOFAR Two Metre Sky Survey
17.20-17.30 Sean Dougherty: Enhanced AGN activity for close galaxy pairs at 0.5 < z < 3.0
17.30-17.40 Cassandra L. Barlow-Hall: Constraints on the X-ray Luminosity Function of AGN at high redshift, with ExSeSS
17.40-17.42 Jan Scholtz: Detection of Multi-phase outflows in Hot Dust Obscured Galaxies
17.42-17.44 Emmanuel Bempong-Manful: Resolving key questions in extragalactic jet physics: results from the e-MERLIN Jets Legacy programme
17.44-17.46 Emma Curtis-Lake: Tracing metallicities in obscured AGN over cosmic time with BEAGLE-AGN
17.46-17.48 Keir Birchall: The Incidence of X-ray selected AGN in the Nearby Universe
17.48-18.00 All participants + Session organisers: FINAL DISCUSSION
09.00-09.20 Ismael Garcia-Bernete: Torus and dusty polar outflow dependence on AGN properties [invited]
09.20-09.30 Alba Vega Alonso Tetilla: Probing the relative roles of evolution, orientation and multi-scale gas distributions in shaping the obscuration of Black Holes through cosmic time
09.30-09.40 Clara Marie Pennock: Discovery of a class of super-AGN behind the Magellanic Clouds using multiwavelength data and unsupervised machine learning
09.40-09.50 Jacob Elford: The Link Between Circumnuclear Molecular Gas Reserviors and Active Galactic Nuclei Fuelling
09.50-10.00 Robbie Webbe: X-ray variability in a super-soft AGN -- Oscillation or Eruption?
10.00-10.10 Victoria Fawcett: Why is colour special? Identifying fundamental differences between red and blue quasars
10.10-10.20 Jiachen Jiang: A highly accreting low-mass black hole hidden in the dust
10.20-10.22 Cressida Cleland: Optical variability as a tracer for low-mass AGN and a precursor to reduced star formation
10.22-10.24 Mohammed Al-Fadhli: The morphology of the active galactic nucleus and its impact on accretion flows and relativistic jets
10.24-10.26 Jan Scholtz: Detection of massive molecular and dust reservoirs around z~2 extremely red quasars: CGM enrichment by quasar-driven outflows
10.26-10.28 Darshan Kakkad: The impact of AGN outflows on star formation at cosmic noon using spatially resolved AO-assisted observations: Insights from the SUPER survey
10.28-10.30 Ricarda Beckmann: The impact of cosmic rays on how AGN jets regulate cluster cooling flows
14.30-14.40 Jan Scholtz: Do powerful large-scale AGN outflows really suppress star formation?
14.40-14.50 Luke Holden: Precise Diagnostics of Multiphase Outflows in the Nearby Seyfert 2 Galaxy IC 5063
14.50-15.00 Gareth Jones: Evidence for Gaseous Halos Around AGN at Cosmic Noon from ALMA CO(3-2) Observations
15.00-15.10 Darshan Kakkad: Scaling relations between multi-phase outflows and AGN across cosmic time
15.10-15.20 Alyssa Drake: Fuelling Quasars at the edge of the Epoch of Reionisation
15.20-15.30 Alexander Richings: Unravelling the physics of multiphase AGN winds through emission line tracers
15.30-15.40 Samuel Ruthven Ward: The Impact of Quasars from Sub-kpc to Galaxy-wide Scales
15.40-16.00 Qingling Ni: The link between AGNs and their host galaxies across cosmic time [invited]
16.30-16.40 Rebecca Smethurst: Which non-merger mechanisms are powering the majority of SMBH growth and AGN feedback? A study with KCWI
16.40-16.50 Stephen Wilkins: The emergence of the first AGN
16.50-17.00 Yana Khusanova: The properties of the host galaxies of radio-loud quasars at z>6
17.00-17.10 Imogen Whittam: Exploring radio-loud AGN with the MIGHTEE survey
17.10-17.20 Brendan Webster: Jet Feedback in a sample of Galaxy Scale Jets from the LOFAR Two Metre Sky Survey
17.20-17.30 Sean Dougherty: Enhanced AGN activity for close galaxy pairs at 0.5 < z < 3.0
17.30-17.40 Cassandra L. Barlow-Hall: Constraints on the X-ray Luminosity Function of AGN at high redshift, with ExSeSS
17.40-17.42 Jan Scholtz: Detection of Multi-phase outflows in Hot Dust Obscured Galaxies
17.42-17.44 Emmanuel Bempong-Manful: Resolving key questions in extragalactic jet physics: results from the e-MERLIN Jets Legacy programme
17.44-17.46 Emma Curtis-Lake: Tracing metallicities in obscured AGN over cosmic time with BEAGLE-AGN
17.46-17.48 Keir Birchall: The Incidence of X-ray selected AGN in the Nearby Universe
17.48-18.00 All participants + Session organisers: FINAL DISCUSSION
Social Sciences S0.21
Social Sciences S0.21
Social Sciences S0.21
© 2023 Royal Astronomical Society