{"id":4,"date":"2026-03-04T14:18:49","date_gmt":"2026-03-04T17:18:49","guid":{"rendered":"https:\/\/congresos.unlp.edu.ar\/xiilapis2026\/?page_id=4"},"modified":"2026-07-08T10:11:21","modified_gmt":"2026-07-08T13:11:21","slug":"home","status":"publish","type":"page","link":"https:\/\/congresos.unlp.edu.ar\/xiilapis2026\/","title":{"rendered":"Home"},"content":{"rendered":"
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Important News<\/div>
Registration is close
Mid July announcement of selected participants and financial support decisions.<\/div><\/div> <\/div>\n<\/div><\/div><\/div>
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About the School<\/h3>\n
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Local Volume cosmology<\/strong> is entering a new era driven by the extraordinary quantity and precision of modern astronomical surveys. New datasets are transforming our understanding of nearby galaxies, stellar structures, and the small-scale distribution of dark matter.<\/strong><\/span><\/p>\n

This school will provide an overview of current challenges and opportunities in the field, with a particular focus on the synergy between precise astrometry from Gaia<\/strong>, deep wide-field photometry from the Vera C. Rubin Observatory (LSST)<\/strong>, and upcoming spectroscopic surveys<\/strong>. Together, these data are enabling new tests of the \u039b-CDM model<\/strong> on small scales.<\/span><\/p>\n

The program will combine lectures by international experts<\/strong>\u00a0with hands-on sessions using public datasets and simulations<\/strong>. Poster sessions and short student presentations<\/strong> will foster discussion and collaboration among participants.<\/span><\/p>\n

The school is designed for about 60 advanced students and early-career researchers<\/strong> from Argentina and neighboring countries.<\/span><\/p>\n<\/div>\n<\/div><\/div><\/div>

Topics<\/h3>\n
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The school will cover key topics in Local Volume cosmology<\/strong>, including:<\/p>\n

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    Dwarf galaxies with resolved stellar populations<\/strong> in the Milky Way and M31, using data from Gaia DR3<\/strong> and Rubin Observatory (LSST)<\/strong> together with cosmological simulations.<\/p>\n<\/li>\n

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    Stellar streams<\/strong> as probes of galaxy assembly, the Galactic potential, and dark matter substructure<\/strong>.<\/p>\n<\/li>\n

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    Numerical modelling of tidal streams and galactic dynamics<\/strong>, using modern N-body techniques and tools such as PeTar, StreamSim, StreamSculptor, Agama, Galpy, Gala<\/strong>, and Dynamigal<\/strong>.<\/p>\n<\/li>\n

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    Constraints on dark matter physics<\/strong> from nearby galaxies and their satellites.<\/p>\n<\/li>\n

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    Metal-poor stars<\/strong> in the halo, dwarf galaxies, and streams as tracers of early galaxy formation.<\/p>\n<\/li>\n

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    Extending near-field cosmology beyond the Local Group<\/strong>.<\/p>\n<\/li>\n

  • The cosmological origin<\/strong> and direct detection<\/strong> of dark matter.<\/strong><\/li>\n<\/ul>\n<\/div>\n<\/div><\/div><\/div><\/div><\/div>","protected":false},"excerpt":{"rendered":"

    Important NewsRegistration is close Mid July announcement of selected participants and financial support decisions. Important Dates About the School Local Volume cosmology is entering a new era driven by the extraordinary quantity and precision of modern astronomical surveys. New datasets are transforming our understanding of nearby galaxies, stellar structures, and the small-scale distribution of dark […]<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"advgb_blocks_editor_width":"","advgb_blocks_columns_visual_guide":"","footnotes":""},"class_list":["post-4","page","type-page","status-publish","hentry","post"],"aioseo_notices":[],"aioseo_head":"\n\t\t\n\t\n\t\n\t\n\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t\n\t\t