08-12 November 2021
Shinjuku, Tokyo, Japan
This meeting will focus on the latest results on high-redshift galaxies from ALMA. The topics will include the epoch of reionization, high-spatial resolution studies, blind surveys, simulations of high-redshift galaxies, and measurement of the physical properties of the galaxies.
28 February - 04 March 2022
UCLA Lake Arrohead Lodge
Lake Arrowhead, California, USA
The far infrared contains critical information about galactic ecosystem; The circle of life of stars and planets. What is the initiation of interstellar chemistry -- via light hydrides? What is the role of feedback (from young and old stars) on the interstellar medium (ISM)? What is the role of magnetic fields in the evolution of the ISM and star formation?
SOFIA provides a flexible, and our currently only, general access to the far infrared (30-300 µm) and its tracers of atomic and molecular lines and FIR polarization. This conference will allow in-person discussions of the results and future opportunities in studying galactic ecosystem using FIR methods, from SOFIA and other platforms. A goal will be to explore synergy with other observatories, including JWST and ALMA, and with theory.
Visit the website for registration informatio and other preliminary information about the meeting. The registration deadline in 15 December 2021, with late registration available until 14 February 2022.