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SUMMARY:Constraints on DM and the cusp/core problem with MUSE - Nicolas Bo
 uché (CNRS &amp\; CRAL)
DTSTART:20230922T103000Z
DTEND:20230922T113000Z
UID:TALK203524@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:The concept of dark matter (DM) originates partly from the stu
 dy of rotation curves in the 70s. Soon\, shallow DM profiles (cores) were 
 found in small galaxies instead of the steep (cusp) profiles expected from
  DM simulations. With the advancements in IFU technology and techniques\, 
 it is now possible to probe DM from the rotation curves of distant galaxie
 s. We will show the current constraints on DM from MUSE surveys and discus
 s the prospects for the future.
LOCATION:Ryle seminar room + online
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