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Line emission from the Interstellar Medium (ISM) of galaxies carries information that can can help us understand galaxy evolution. Observing line emission at different wavelengths, has the prospect of revealing amount, composition and state of the ISM, as well as trace galaxy properties such as star formation rate (SFR), metallicity and dynamics. Vital for the interpretation of such observations, and the focus of this meeting, was the theoretical modeling of line emission escaping a galaxy. The aim of this workshop was to shed light on the following:
➵ What are the best emission lines to trace various ISM properties? ➵ How can we use emission lines to trace feedback and ISM evolution with redshift? ➵ Where do we stand in deriving sub-grid physics and comparing codes? And finally; what are the next big questions for theorists in this field, and how do we coordinate our efforts? Confirmed invited speakers: Gary Ferland Gergö Popping Andrea Pallottini This workshop gathered experts from around the world for three intense days of presentations, group discussion and break-out sessions. The workshop sessions was not limited to any particular wavelength or redshift, and joined theoretical astronomers, from grad students to professors, to further advance the field of synthetic observations. |
Dec 15 |
Announcement: Registration open |
Jan 15 |
Registration deadline |
March 14 |
Conference begins |
March 16 |
Conference ends |
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Prof. Rogier Windhorst, Co-Director of the ASU Cosmology Initiative, and James Webb Space Telescope Interdisciplinary Scientist.
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LOC
Karen Pardos Olsen Evan Scannapieco Karen Knierman Michael Ruppert Judd Bowman Lily Whitler Sean Bryan Jacob Cluff Michael McLendon Margaret Hufford |
SOC
Karen Pardos Olsen Claudia Lagos Enrique Vazquez Semadeni Livia Vallini Kristian Finlator Thomas Greve Desika Narayanan Evan Scannapieco Thomas Bisbas Thomas Haworth |