University of Cambridge > Talks.cam > Institute of Astronomy Seminars > Galaxy population synthesis modeling in the golden age of the Milky Way & Local Group research

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

Add to your list(s) Download to your calendar using vCal

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.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2020 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity