[ASA] "Evolution of Dust and Gas throughout Cosmic Time" Conference in Hiroshima, Japan in December 2024

[Andrew Battisti]

Dear colleagues,

A final reminder that the abstract deadline is this coming Friday, June 28th for the “Evolution of Dust and Gas throughout Cosmic Time” conference (details below).

Best,
Andrew Battisti (on behalf of the SOC)

From: Andrew Battisti <Andrew.Battisti at anu.edu.au>
Date: Wednesday, 22 May 2024 at 7:22 AM
To: ASA at mailman.sydney.edu.au <ASA at mailman.sydney.edu.au>
Subject: "Evolution of Dust and Gas throughout Cosmic Time" Conference in Hiroshima, Japan in December 2024
Dear colleagues,

Please find below the second announcement for the “Evolution of Dust and Gas throughout Cosmic Time” conference to be held on December 9-13, 2024 in Hiroshima, Japan. Please note that this conference overlaps with the  ESO-SKA 2024 conference being held in Western Australia.

The abstract deadline closes in ~1 month (June 28).

Best,
Andrew Battisti (on behalf of the SOC)

---------------------------------------
Dear colleagues,

We are pleased to announce the upcoming “Evolution of Dust and Gas throughout Cosmic Time” conference, set to take place on December 9-13, 2024, in the beautiful city of Hiroshima, Japan. This conference aims to focus on the latest advancements in our understanding of star formation, active galactic nuclei (AGN), and the interstellar medium (ISM), and their evolution across cosmic time. We look forward to your participation.

Abstract Submission (Due June 28th)
https://url.au.m.mimecastprotect.com/s/OTmQCzvkyVC8JYn8gI4zExj?domain=dg2024.hasc.hiroshima-u.ac.jp

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

Invited Speakers
Laia Barrufet (University of Edinburgh)
Leindert Boogaard (Max Planck Institute for Astronomy)
Tanio Diaz-Santos (Institute of Astronomy, FORTH)
Mariko Kubo (Tohoku University)
Claudia Lagos (University of Western Australia, International Centre for Radio Astronomy Research)
Lihwai Lin (Academia Sinica Institute of Astronomy and Astrophysics)
Gergö Popping (European Southern Observatory)
Anna Sajina (Tufts University)
Anita Zanella (INAF, Osservatorio Astronomico di Padova)

Website
https://url.au.m.mimecastprotect.com/s/1NU0CANpgjCr7KVr6u8HtqF?domain=dg2024.hasc.hiroshima-u.ac.jp

Important Dates
Mark your calendars for the key dates below:

  *   Abstract Deadline: Friday, June 28th
  *   Registration Deadline for Presenters: Friday, September 6th
  *   General Registration Deadline: Late October

Location
Hiroshima, our chosen conference venue, is a city with a powerful history. Situated within convenient reach from Tokyo, Japan's bustling capital, Hiroshima offers a unique blend of cultural significance and contemporary charm. While it stands as a poignant symbol of resilience and peace, Hiroshima also boasts picturesque landscapes, modern amenities, and delicious food! Traveling from Tokyo to Hiroshima is both convenient and efficient, with options including high-speed Shinkansen trains, which take you from the heart of Tokyo to Hiroshima in just a few hours. Whether you're drawn to explore Hiroshima's iconic landmarks or eager to immerse yourself in its vibrant culture, our conference provides the perfect opportunity to experience the warmth and allure of this remarkable city.

Contact
SOC: dg2024-soc at ml.hiroshima-u.ac.jp<mailto:dg2024-soc at ml.hiroshima-u.ac.jp>
LOC: dg2024-loc at ml.hiroshima-u.ac.jp<mailto:dg2024-loc at ml.hiroshima-u.ac.jp>

We kindly ask you to share this announcement with anyone who might be interested in attending the conference. We apologize if you receive this email more than once; our aim is to ensure that all interested parties have the opportunity to participate in this enriching event.

Warm regards,

On behalf of the SOC:

Andrew Battisti
Veronique Buat
Chian-Chou Chen
Roberto Decarli
Hanae Inami (co-chair)
Desika Narayanan
Toshiki Saito
Irene Shivaei (co-chair)
Vivian U


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