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Evolution of Dust and Gas throughout Cosmic Time
Scientific Rationale
In recent years, our view of star formation, active galactic nuclei (AGN), the dusty interstellar medium (ISM), and their connection over cosmic time has been revolutionized thanks to technological advances in infrared and submillimeter facilities such as JWST and ALMA. Recent observations now enable direct comparisons of ISM properties from z=0 to the early Universe, from resolved studies to direct observations of dust and gas in different phases. At the same time, simulations have made significant progress in their ability to include the physics of a multi-phase ISM, as well as interstellar dust. Therefore, it is now timely to bring together observers and theorists to discuss new insights and findings on linking dust and gas properties of galaxies observed at different scales and cosmic times, as we prepare for the exciting years ahead. The main goals are to discuss the state of our knowledge about:
• Evolution of dust and metals from the local Universe to high redshifts
• Galaxy growth and resolved studies of star formation and AGN
• Interpretations of new observations and constraints for the latest simulations
• Future prospects of infrared astronomy
Family-Friendly Services
The conference warmly welcomes caregivers and parents along with their children. We offer childcare during the conference hours upon request (due Friday, October 4). The conference hall has a soundproof family room from where you can watch and listen to the talks (see also the Family-Friendly Services page).
Invited Speakers
Laia Barrufet (University of Edinburgh)
Leindert Boogaard (Leiden University)
Tanio Diaz-Santos (Institute of Astrophysics, FORTH)
Mariko Kubo (Tohoku University)
Claudia Lagos (University of Western Australia, International Centre for Radio Astronomy Research)
Lihwai Lin (Academia Sinica Inst. of Astronomy and Astrophysics)
Gergö Popping (European Southern Observatory)
Anna Sajina (Tufts University)
Anita Zanella (INAF, Osservatorio Astronomico di Padova)
Key Information
When: 09 Dec - 13 Dec, 2024
Where: Hiroshima, Japan (Venue)
Abstract Deadline: Friday, June 28th
Registration Deadline:
Early bird: September 30th
Late registration: October 20th
For further details, click here: (Registration)
Scientific Organizing Committee
Andrew Battisti (Australian National University & University of Western Australia)
Veronique Buat (Aix-Marseille University)
Chian-Chou Chen (Academia Sinica Inst. of Astronomy and Astrophysics)
Roberto Decarli (Inst. Nazionale di Astrofisica)
Hanae Inami (Hiroshima University, chair)
Desika Narayanan (University of Florida)
Toshiki Saito (Shizuoka University)
Irene Shivaei (Centro de Astrobiología, chair)
Vivian U (Univeristy of California, Irvine)
Local Organizing Committee
Hiddo Algera (Academia Sinica Inst. of Astronomy and Astrophysics)
Thomas Bohn (Hiroshima University)
Jean-Paul Breuer (Hiroshima University)
Bunyo Hatsukade (National Astronomical Observatory of Japan)
Hanae Inami (Hiroshima University, chair)
Ayumi Ishikawa (Hiroshima University)
Koji Kawabata (Hiroshima University, chair)
Tohru Nagao (Ehime University)
Taiga Nozawa (Hiroshima University)
Mau Otsuki (Hiroshima University)
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