Galaxy population synthesis modeling in the golden age of the Milky Way & Local Group research

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• Stefano Pasetto, Carnegie
• Wednesday 19 September 2018, 13:15-13:45
• Sackler Lecture Theatre, IoA.

If you have a question about this talk, please contact Catrina Diener.

The building blocks of the known Universe are stars. To study what governs the structure and evolution of our galaxy, the Milky Way (MW), its companion Andromeda (M31), or the Local Group (LG) dwarf galaxies means to observe and understand the processes that govern the stellar birth, evolution, death, and motion over their evolutionary time-scales. The process of collecting detailed data on our Galaxy represents the first step in this work of archeological research and surveys such as Gaia, SDSS , APOGEE2, RAVE as well as forthcoming missions and telescopes such as SDSS -V, LSST , JWST, GMT , TMT will project us into a golden age of the MW & LG research. Exploiting datasets of this scope is not merely a case of applying the same tools that have been used historically: it demands the development of, and experience with, leading-edge multi-dimensional machine learning techniques for data mining.

I will review the open questions in this research field and introduce my novel population synthesis model (and its related webpage www.GalMod.org) developed to face these new era theoretical challenges.

This talk is part of the Institute of Astronomy Seminars series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Seminars
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• Sackler Lecture Theatre, IoA

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