AGN 15
Padua
The "XVth Italian meeting on Active Galactic Nuclei: from the present-day Universe to the Dark Ages" is set to uphold a three-decade-long tradition of convening experts to share and discuss contemporary research spanning the breadth of AGN phenomenology, physics, and modelling. Emphasis will be placed on the unique perspectives of Italian astronomy within this realm. The conference will delve into a range of topics, including:
1. The Central Engines of AGN, accretion and ejections (including relativistic jets), and analogies with stellar mass black holes
2. The Circumnuclear Regions
3. Coevolution of Black Holes and Galaxies and AGN Feedback
4. Time domain and variability studies
5. Perspectives offered by the ground and space based instrumentation under development with Italian participation 6. Multimessenger Studies and multiwavelength Surveys, including gravitational wave and neutrino astronomy
7. Large Scale Environment, High-z AGN and Cosmology
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The central engine¶Convener: Elena Dalla Bontà
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Radio-Loud AGN with Hubble and Webb: latest results from low (z~1) to high (z~8) redshift¶Speaker: Marco Chiaberge
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Revisiting the Fourth Fermi LAT Catalog: the rise of gamma-ray emitting jetted Seyfert-type AGN¶Speaker: Luigi Foschini
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A revolutionary view from low-luminosity radio-loud AGN in the local Universe: the FR0 radio galaxies¶Speaker: Ranieri Baldi
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16:00
Coffee break
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The central engine¶Convener: Mauro D'Onofrio
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The nature of mJy Radio Galaxies: the study of the relation between jet and accretion disk properties¶Speaker: Olena Torbaniuk
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Jet reorientation in cluster-central radio galaxies: insights from VLBA and Chandra data¶Speaker: Francesco Ubertosi
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Exploring AGN coronae through X-ray polarimetry: insights from IXPE observations¶Speaker: Daniele Tagliacozzo
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The central engine¶Convener: Enrico Piconcelli
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The X-ray properties of the most luminous quasars with strong outflows¶Speaker: Anastasia Shlentsova
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18
PDS456: a new look at the archetypal AGN-feedback laboratory with the XRISM X-ray microcalorimeter¶Speaker: Alfredo Luminari
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19
Unraveling the Complexity of Ultra-Fast Outflows: X-ray Spectroscopy Insights from IRAS 13224-3809 and PDS 456¶Speaker: Pierpaolo Condò
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20
HYPERION XMM-Newton Heritage Program. The X-rays Strike Back: unique relations between X-ray continuum and disk winds and SMBH mass growth revealed in luminous QSOs at z > 6¶Speakers: Alessia Tortosa, Luca Zappacosta
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10:30
Coffee break
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12:15
Lunch break
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16:00
Coffee break
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Coevolution of Black Holes and Galaxies and AGN Feedback¶Convener: Filippo Mannucci
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The formation and evolution of quasar-host galaxies across cosmic time¶Speaker: Francesco Salvestrini
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34
Sustained super-Eddington accretion and outflow properties in high-redshift quasars¶Speaker: Giada Quadri
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The unprecedented NIRSpec/JWST view of the nuclear region in the prototypical merging galaxy NGC 6240¶Speaker: Matteo Ceci
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Fast & Furious at z∼2: faster ionised winds in type-2 AGN than in type-1 systems¶Speaker: Giulia Tozzi
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The effects of AGN winds and radioloudness in high-redshift type I Quasars¶Speaker: Alice Deconto-Machado
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Coevolution of Black Holes and Galaxies and AGN Feedback¶Convener: Luigi Foschini
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A new benchmark for the local and high-z scaling relations of supermassive black holes: dissecting the roles of AGN feedback and black hole mergers¶Speaker: Francesco Shankar
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The complex (negative and positive) AGN feedback from outflows and jets in the Teacup¶Speaker: Giacomo Venturi
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45
The merging system BR1202-0725: a close pair of AGN at z ∼4.7 from NIRSpec observations¶Speaker: Sandra Zamora
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Expanding the Parameter Space of Circumnuclear Obscuration: Ultra-Thick Highly-Variable Warm Absorbers¶Speaker: Riccardo Middei
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10:15
Coffee break
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12:15
Lunch Break
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Time domain and variability studies¶Convener: Alessandro Marconi (Dipartimento di Fisica e Astronomia, Università di Firenze)
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Time-Resolved Diagnostics of the Ionized Absorbers in NGC 4051¶Speakers: Fabrizio Nicastro, Roberto Serafinelli
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Optical spectral variability in a relativistic jetted AGN: the case of PMN J0948+0022¶Speaker: Benedetta Dalla Barba
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The Luminosity-variability relation in BASS type-1 AGN its connection with physical properties and cosmological implementations¶Speaker: Matilde Signorini
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54
'Would you follow me?' X-ray and optical variations of the changing-look AGN J0413-0050¶Speaker: Amelia Vietri
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Testing close massive black hole binary candidates through multi-epoch spectroscopy¶Speaker: Lorenzo Bertassi
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16:15
Coffee break
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Time domain and variability studies¶Convener: Vincenzo Antonuccio (Catania Astrophysical Observatory)
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Mapping of molecular gas in radio-loud AGN at z=0.4 hosted by cool-core brightest cluster galaxies¶Speaker: Gianluca Castignani
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Probing Black Holes in Distant Quasars with Photometric Reverberation Mapping: A smarter faster (150x) way to measure BLR sizes (and black hole masses) in active galaxies¶Speaker: Swayamtrupta Panda
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eROSITA-detected X-ray flaring event in a Seyfert galaxy: a multi-wavelength analysis and interpretation of the physical processes¶Speaker: Saikruba Krishnan
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Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution¶Speaker: Brivael Laloux
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Perspectives offered by the ground and space based instrumentation¶Convener: Elisabeta Lusso (Dipartimento di Fisica e Astronomia, Università di Firenze)
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Perspectives offered by the ground and space based instrumentation under development with Italian participation¶Speaker: Roberto Ragazzoni
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New opportunities in AGN high energy astrophysics from space and from the ground¶Speaker: Massimo Cappi
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The greatest hits of the Whole Earth Blazar Telescope in understanding blazars¶Speaker: Claudia M. Raiteri
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10:15
Coffee break
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Multimessenger Studies and multiwavelength surveys¶Convener: Marco Berton (Università di Padova)
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Simulating the evolution of dual and binary SMBHs/AGNs and their implications for gravitational wave astronomy¶Speaker: Jasbir Singh
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Connecting Gamma-Ray Absorption Features and Neutrinos to investigate the presence of Large-Scale Environments in BL Lac objects¶Speaker: Luca Foffano
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JASSIE: A Customizable Interface for Simulating SEDs in simulated Jetted AGNs¶Speaker: Marco Sortino
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A new look at the extragalactic Very High Energy sky: searching for TeV-emitting candidates among the X-ray bright non-Fermi detected blazar population¶Speaker: Stefano Marchesi
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12:30
Lunch break
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Multimessenger Studies and multiwavelength surveys¶Convener: Fabio La Franca
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Chandra-to-MeerKAT: A complete multi-λ characterisation of obscured AGN at 0.6<z<3¶Speaker: Luigi Barchiesi
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Spectral Energy Distribution Modeling of Broad Emission Line Quasars: From X-ray to Radio Wavelengths¶Speaker: Avinanda Chakraborty
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X-ray VS multiband nuclear properties of luminous quasars at the Cosmic Noon: surprises and confirmation¶Speaker: Cecilia Degli Agosti
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Large Scale Environment, High-z AGN and Cosmology¶Convener: Valentina D'Odorico (Istituto Nazionale di Astrofisica (INAF))
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The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling¶Speaker: Vieri Cammelli
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The radio properties of z>3.5 quasars: Are most high-redshift radio-loud active galactic nuclei obscured?¶Speaker: Alessandro Capetti
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16:45
Coffee break
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Large Scale Environment, High-z AGN and Cosmology¶Convener: Valentina D'Odorico (Istituto Nazionale di Astrofisica (INAF))
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Large Scale Environment, High-z AGN and Cosmology¶Convener: Marco Chiaberge (STScI/JHU)
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AGN under the eye of JWST: new selection techniques and physical properties¶Speaker: Giovanni Mazzolari
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Phenomenology of super-Eddington accretion in AGN¶Speaker: Paola Marziani (Istituto Nazionale di Astrofisica (INAF))
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First systematic investigation of broad-band X-ray-to-NIR SED of z~6-7.5 quasars¶Speaker: Ivano Saccheo
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Too many or just right? Massive jetted quasars in the early Universe¶Speaker: Tullia Sbarrato (Università degli Studi di Milano - Bicocca)
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10:15
Coffee break
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Large Scale Environment, High-z AGN and Cosmology¶Convener: Maurizio Paolillo (Istituto Nazionale di Astrofisica (INAF))
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Shedding X-ray light on the formation sites of high-z Hot Dust Obscured luminous quasars: the case of W0410-09 at z~ 3.6¶Speaker: Ilaria Villani
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Fast SMBH growth in high-redshift gas-rich protoclusters¶Speaker: Fabio Vito (Istituto Nazionale di Astrofisica (INAF))
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The quest for high redshift galaxies¶Speaker: Barbara Balmaverde (Istituto Nazionale di Astrofisica (INAF))
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