Adaptable Radiative Transfer Innovations for Submillimeter Telescopes (ARTIST)
Marco Padovani, Jes J{\o}rgensen (for the ARTIST Collaboration)
TL;DR
ARTIST is a project developing advanced multi-dimensional radiative transfer models to interpret submillimeter observations from upcoming large telescopes like ALMA and Herschel, aiding astrophysical research.
Contribution
It introduces a next-generation model suite for comprehensive radiative transfer calculations of dust and line emission, including polarization, tailored for new submillimeter telescopes.
Findings
Enhanced modeling capabilities for dust and line emission.
Improved interpretation of submillimeter observational data.
Support for polarization analysis in astrophysical environments.
Abstract
Submillimeter observations are a key for answering many of the big questions in modern-day astrophysics, such as how stars and planets form, how galaxies evolve, and how material cycles through stars and the interstellar medium. With the upcoming large submillimeter facilities ALMA and Herschel a new window will open to study these questions. ARTIST is a project funded in context of the European ASTRONET program with the aim of developing a next generation model suite for comprehensive multi-dimensional radiative transfer calculations of the dust and line emission, as well as their polarization, to help interpret observations with these groundbreaking facilities.
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