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SUMMARY:EDGE: Predicting Scatter in the Stellar Mass–Halo Mass Relation 
 for Dwarf Galaxies
DTSTART;VALUE=DATE-TIME:20230324T091000Z
DTEND;VALUE=DATE-TIME:20230324T092500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115758Z
UID:indico-contribution-215@meetings.aip.de
DESCRIPTION:Speakers: Stacy Kim (University of Surrey)\nOne of the primary
  hurdles in pushing dark matter constraints to dwarf scales the uncertaint
 y in the stellar-mass--halo-mass (SMHM) relation.  Results from simulation
 s differ by two orders of magnitude at halo masses \n\nhttps://meetings.ai
 p.de/event/20/contributions/215/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/20/contributions/215/
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