08:00
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
22:00
23:00
8:00 - 10:00 (2h)
Registration
Registration
10:00 - 10:30 (30min)
Coffee break
10:30 - 11:00 (30min)
Welcome
RunAn
11:00 - 12:00 (1h)
Dust properties
RunAn
Karl Gordon
› PDRs4All: JWST's view of the Orion Bar
- Els Peeters, SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA, Department of Physics & Astronomy & Institute of Earth and Space Exploration, Western University, London ON N6A 3K7, Canada
11:00-11:30 (30min)
› Dust Grain Properties in the Gas-Rich Absorption Systems of Diverse Galaxies at z<2
- Monique Aller, Georgia Southern University
11:30-11:45 (15min)
› The dust population in PDRs: impact on PDR structure and observable tracers
- Raphaël Meshaka, Raphaël Meshaka
11:45-12:00 (15min)
12:00 - 13:30 (1h30)
Lunch
13:30 - 14:45 (1h15)
Dust properties
RunAn
Gunnar Nyman
› AstroPAHs: from laboratory experiments to observational diagnostics
- Christine Joblin, Institut de recherche en astrophysique et planétologie
13:30-14:00 (30min)
› Polycyclic Aromatic Hydrocarbons and dust in star-forming regions and the vicinity of AGN: a JWST view
- Ismael Garcia-Bernete, University of Oxford
14:00-14:15 (15min)
› A computational anharmonic IR database of nanosilicate clusters at astrochemically relevant temperatures
- Zeyuan Tang, Center for Interstellar Catalysis, Aarhus University
14:15-14:30 (15min)
› Temperature-dependent optical properties of dust analogues for the interpretation of astronomical observations
- Karine Demyk, Institut de recherche en astrophysique et planétologie
14:30-14:45 (15min)
14:45 - 15:30 (45min)
Coffee break
15:30 - 17:00 (1h30)
Dust properties
RunAn
Kirsten Knudsen
› Dark Dust
- Ralf Siebenmorgen, European Southern Observatory
15:30-16:00 (30min)
› Dust content of galaxies at high redshift
- Tomoko Suzuki, Kavli IPMU
16:00-16:30 (30min)
› Constraining the dust attenuation law in early galaxies with JWST
- Vladan Markov, Scuola Normale Superiore
16:30-16:45 (15min)
› ALMA view on the dust properties of the HYPERION QSOs
- Roberta Tripodi, University of Trieste, INAF - Osservatorio Astronomico di Trieste
16:45-17:00 (15min)
17:00 - 17:30 (30min)
Poster flash session
RunAn
17:30 - 19:00 (1h30)
Poster session and mingle
8:30 - 9:00 (30min)
Registration
Registration
9:00 - 10:15 (1h15)
Dust properties
RunAn
Karl Gordon
› There and back again — Dust evolution between diffuse and dense environments — It's complicated
- Anthony Jones, Institut d'Astrophysique Spatiale (IAS Orsay)
09:00-09:30 (30min)
› Dust Evolution across the Orion Bar: new insights from the JWST
- Meriem El Yajouri, Institut d'Astrophysique Spatiale (IAS) [France]
09:30-09:45 (15min)
› PASIPHAE Survey: Large optical polarimetric sky survey for dust cloud & magnetic field tomography
- Siddharth Maharana, South African Astronomical Observatory
09:45-10:00 (15min)
› Small amounts of iron(II) sulphides can significantly affect the SEDs of circumstellar disks
- Christian Kranhold, Astrophysical Institute and University Observatory, Friedrich-Schiller-University Jena
10:00-10:15 (15min)
10:15 - 11:00 (45min)
Coffee break
11:00 - 12:00 (1h)
Dust properties
RunAn
Gunnar Nyman
› Assessing the astronomical relevance of interstellar nanosilicate dust grains from IR spectra: theory, experiment and observation
- Stefan Bromley, Institució Catalana de Recerca i Estudis Avançats [Barcelona], Universitat de Barcelona
11:00-11:30 (30min)
› Exploring the dust properties in the nearby diffuse interstellar medium with JWST
- Sascha Zeegers, Sascha Zeegers, ESA - ESTEC (Netherlands)
11:30-11:45 (15min)
› Studying dust grain properties and growth by combining extinction and depletion measurements in the Milky Way
- Marjorie Decleir, Space Telescope Science Institute
11:45-12:00 (15min)
12:00 - 13:30 (1h30)
Lunch
13:30 - 14:30 (1h)
Dust properties
RunAn
Dimitra Rigopoulou
› What do dust grains look like at the onset of the star and disk formation sequence ?
- Anaëlle Maury, Unité Mixte CEA/CNRS AIM, Université Paris Saclay
13:30-14:00 (30min)
› Modelling the cold dust in nearby spiral galaxies with radiative transfer
- Angelos Nersesian, Ghent University
14:00-14:15 (15min)
› The X-ray view of dust in the Milky Way
- Elisa Costantini, SRON Netherlands Institute for Space Research, Astronomical Institute Anton Pannekoek
14:15-14:30 (15min)
14:30 - 15:15 (45min)
Coffee break
15:15 - 16:45 (1h30)
Dust properties
RunAn
Wouter Vlemmings
› Dust Properties from the Lab applied to young disks: 3D-printing and a Microwave Analogy Experiment
- Francois MENARD, IPAG- Institut de Planetologie et d'Astrophysique de Grenoble
15:15-15:45 (30min)
› The influence of a clumpy outflow and companion star on the surface composition of AGB dust
- Marie Van de Sande, University of Leeds
15:45-16:00 (15min)
› The far-UV-extinction-to-H2 correlation and insights from IR emission in photodissociation regions
- Dries Van De Putte, Space Telescope Science Institute
16:00-16:15 (15min)
› The Si K Edge Gas and Dust Optical Depths Toward the Galactic Bulge
- Jun Yang, Massachusetts Institute of Technology
16:15-16:30 (15min)
› Investigating the Magnetic Fields under stellar feedback using dust polarization
- Ekta Sharma, National Astronomical Observatories of China
16:30-16:45 (15min)
16:45 - 17:00 (15min)
Poster flash session
RunAn
17:00 - 18:30 (1h30)
Poster session and mingle
19:00 - 22:00 (3h)
Astronomy on Tap
Astronomy on Tap
9:00 - 10:30 (1h30)
Dust formation
RunAn
Elvire De Beck
› Dust in AGB Stars
- Martha Boyer, Space Telescope Science Institute
09:00-09:30 (30min)
› The contribution of dust from AGB stars to the ISM
- Matthias Maercker, Chalmers University of Technology [Gothenburg, Sweden]
09:30-09:45 (15min)
› Stardust: From micro-physics to global dynamics
- Susanne Höfner, Department of Physics and Astronomy, Uppsala University
09:45-10:00 (15min)
› Small pieces make up the big story
- Leen Decin, Instituut voor Sterrenkunde, KU Leuven
10:00-10:15 (15min)
› Dust millimetre emission in Nearby Galaxies with NIKA2/IRAM-30m: major challenges and latest results of the IMEGIN Large Program.
- Lara Pantoni, IAS, Irfu/Dap
10:15-10:30 (15min)
10:30 - 11:15 (45min)
Coffee break
11:15 - 12:45 (1h30)
Dust formation
RunAn
Liv Hornekær
› Laboratory studies on the production and processing of major cosmic dust components in laboratory
- Cornelia Jäger, Laboratory Astrophysics Group, Max Planck Institute for Astronomy, Heidelberg, and Institute of Solid State Physics, Friedrich Schiller University Jena
11:15-11:45 (30min)
› Supernova dust formation: a high-resolution view with JWST
- Ilse De Looze, Department of physics and astronomy, Ghent University
11:45-12:15 (30min)
› Modeling dust formation in supernovae in the JWST era
- Arkaprabha Sarangi, Niels Bohr Institute [Copenhagen]
12:15-12:30 (15min)
› Massive Dust Reservoirs in Normal Galaxies at Redshift 7
- Hiddo Algera, Hiroshima University, National Astronomical Observatory of Japan
12:30-12:45 (15min)
12:45 - 14:00 (1h15)
Lunch
13:30 - 18:30 (5h)
Excursion to Varberg
Social activity
9:00 - 10:15 (1h15)
Dust growth
RunAn
Frederic Galliano
› Dust growth in nearby galaxies
- Anja Andersen, University of Copenhagen = Københavns Universitet
09:00-09:30 (30min)
› The z<1 drop of cosmic dust abundance
- Massimiliano Parente, SISSA, INAF - Osservatorio Astronomico di Trieste
09:30-09:45 (15min)
› The origin of dust grains within galaxies seen in the first billion years of cosmic time
- Joris Witstok, Kavli Institute for Cosmology - University of Cambridge
09:45-10:00 (15min)
› Constraining ISM dust properties with stellar polarization and dust emission
- Gina Panopoulou, Chalmers University of Technology [Gothenburg, Sweden]
10:00-10:15 (15min)
10:15 - 11:00 (45min)
Coffee break
11:00 - 12:00 (1h)
Dust growth
RunAn
Liv Hornekær
› Influence of grain growth on ices spectroscopic profiles
- Emmanuel Dartois, Institut des Sciences Moléculaires d'Orsay
11:00-11:30 (30min)
› Molecular content in Si + C dust growth processes for laboratory astrophysics
- Sandra Wiersma, IRAP, Université de Toulouse III - Paul Sabatier, CNRS, CNES
11:30-11:45 (15min)
› From dust to pebbles: revisiting grain growth in protoplanetary disks
- Leonardo Testi, Università di Bologna
11:45-12:00 (15min)
12:00 - 13:30 (1h30)
Lunch
13:30 - 15:00 (1h30)
Dust growth
RunAn
Arka Sarangi
› The nearby universe:A laboratory to study the cosmic build-up of interstellar dust in galaxies
- Julia Roman-Duval, Space Telescope Science Institute
13:30-14:00 (30min)
› Rethinking the Nature of Dust in the Diffuse ISM
- Brandon Hensley, JPL/Caltech
14:00-14:30 (30min)
› Predicting the dust condensation sequence from a bottom-up perspective
- David Gobrecht, University of Gothenburg
14:30-14:45 (15min)
› Using JWST Photometry to Determine What Sets the PAH Distribution in Nearby Galaxies
- Jessica Sutter, University of California [San Diego]
14:45-15:00 (15min)
15:00 - 15:45 (45min)
Coffee break
15:45 - 17:00 (1h15)
Dust growth
RunAn
Susanne Aalto
› Dust growth in high-redshift galaxies and its impact on the grain size distribution
- Hiroyuki Hirashita, Academia Sinica
15:45-16:15 (30min)
› Observational constrains on dust grain alignment: from protostellar cores to PDRs
- Valentin LE GOUELLEC, NASA Ames Research Center
16:15-16:30 (15min)
› Observational evidence of morphological quenching in dusty elliptical galaxies
- Aleksandra Leśniewska, Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University, Dark Cosmology Centre
16:30-16:45 (15min)
› Rise and Fall of Anomalous Microwave Emission in Extragalactic Star Forming Regions
- ILSANG YOON, National Radio Astronomy Observatory
16:45-17:00 (15min)
17:00 - 17:15 (15min)
Poster and quiz prices
RunAn
19:00 - 23:00 (4h)
Conference dinner
9:00 - 10:15 (1h15)
Dust destruction
RunAn
Arka Sarangi
› Dust destruction in supernova remnants
- Elisabetta Micelotta, Nanoform, University of Helsinki
09:00-09:30 (30min)
› The Disappearing Act: Exploring the PAH Deficit at Low Metallicities
- Elizabeth Tarantino, Space Telescope Science Institute
09:30-09:45 (15min)
› Empirical constraints on dust destruction in supernova remnants
- Felix Priestley, Cardiff University
09:45-10:00 (15min)
› Interstellar carbonaceous dust erosion induced by X-rays irradiation of water ice in star-forming Regions
- Ko-Ju Chuang, Leiden Observatory [Leiden]
10:00-10:15 (15min)
10:15 - 11:00 (45min)
Coffee break
11:00 - 11:45 (45min)
Dust destruction
RunAn
Frederic Galliano
› Radiative Torque Disruption and Implications
- Le Ngoc Tram, Max Planck Institute for Radio Astronomy - Thiem Hoang, Korea Astronomy and Space Science Institute
11:00-11:30 (30min)
› From total destruction to complete survival: Dust in supernova remnants at different evolutionary stages
- Florian Kirchschlager, Ghent University
11:30-11:45 (15min)
11:45 - 12:00 (15min)
Conclusion
13:00 - 17:45 (4h45)
Excursion to Onsala Space Observatory
Social activity
