BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Schwarzschild self-consistent modeling of the Fornax dSph galaxy u
 sing line-of-sight velocity distribution.
DTSTART;VALUE=DATE-TIME:20241025T154500Z
DTEND;VALUE=DATE-TIME:20241025T160000Z
DTSTAMP;VALUE=DATE-TIME:20260422T083730Z
UID:indico-contribution-4138@cern.ch
DESCRIPTION:Speakers: Galina Shchelkanova (Kurchatov Institute)\nDwarf sph
 eroidal (dSph) satellites of the Milky Way (MW) are the\nmostly dark matte
 r (DM) dominated systems. Their dynamical parameters\nsuch as line-of-sigh
 t (LOS) velocities are measured very accurately\, so they\nare very good p
 robes of DM properties. We have constructed nearly\nself-consistent stars-
 halo model of the dSph Fornax galaxy using \nSchwarzschild orbit-superposi
 tion code of the AGAMA software library. \nThis is a step forward after pr
 evious studies\nof this object based on more approximate Jeans equation ap
 proach.\nThe code fits Gauss–Hermite (GH) expansion coefficients of the 
 LOS velocity\ndistribution for each apperture of the galaxy to their obser
 vational estimates. \nWe use the latest data on the stellar velocities and
  their probability \nmembership to estimate the GH coefficients of the obs
 ervational data\nby the AGAMA code.\n\nhttps://indico.particle.mephi.ru/ev
 ent/436/contributions/4138/
LOCATION: Moskvorechye 1
URL:https://indico.particle.mephi.ru/event/436/contributions/4138/
END:VEVENT
END:VCALENDAR