BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Precise constrained cosmological simulations of the Local Group DTSTART;VALUE=DATE-TIME:20230324T111500Z DTEND;VALUE=DATE-TIME:20230324T113000Z DTSTAMP;VALUE=DATE-TIME:20240704T115801Z UID:indico-contribution-221@meetings.aip.de DESCRIPTION:Speakers: Ewoud Wempe (Kapteyn Astronomical Institute)\nCosmol ogical simulations have been used to understand the formation of structure in the LCDM paradigm on small and large scales. Most simulations start wi th unconstrained Gaussian initial conditions\, and therefore generically d o not produce good analogues of the Local Group at present day. While cons trained simulations exist\, these have difficulty in precisely satisfying all our observational constraints on the Local Group\, and their result is not an unbiased and fair sample of the posterior distribution of LCDM uni verses subject to the observational constraints of the Local Group. Some a pplications of such a sample include putting into cosmological context our distribution of satellites\, the alignment of the dark-matter haloes and their spin and the relation to the assembly history\, and to determine the effect of our environment on the Local Group's spatial configuration and kinematics.\n\nIn this work\, we extend the BORG algorithm (Bayesian Origi n Reconstruction from Galaxies)\, that has already been used to model the Local Large-Scale Structure\, to reconstruct the Local Group. Using this t oolset\, we perform a statistical inference on the history of the Local Gr oup\, following a LCDM prior on the cosmological initial conditions\, and a likelihood that constrains local observational quantities\, like the mas ses\, positions\, and velocities of the Milky Way and Andromeda haloes. In the near future\, we plan to embed our Local Group in a realistic large-s cale structure as well. To the best of our knowledge\, this is the first t ime a cosmological simulation has been able to reproduce all these propert ies simultaneously with high precision.\n\nhttps://meetings.aip.de/event/2 0/contributions/221/ LOCATION:Haus H\, Telegrafenberg URL:https://meetings.aip.de/event/20/contributions/221/ END:VEVENT END:VCALENDAR