todo.txt

- hubble flow:
   - few examples
   - yhteenvetoplotti
   - 

- velocity dispersion
   - good, neljä plottia erikseen hyvä

- anisotropy mollweide
   - multiple plots (9?) with different volumes
   - absolute velocities too (see filaments etc)

- grouping
   - no need to repeat mollweide for multiple simulations
   - show same volume with multiple eps and ms
   - eps and ms in one 3d plot

- include error bars on new plots (H0 vs r0, LG mass cs r0)

Meeting after these:
[X] H0 and r0 distributions, their correlation?
[X] LG mass vs r0 where LG mass is either MW+A or everything within r0

- citation style either from ApJ or another journal

For meeting:
-


5.1 introduction, selection
5.2 zeroth order stuff
   hubble flow, local H0, zero-point, H0 within shells, is this consistent with what went into the simulation, number of subhaloes within some radius, kinematics of LGs
HUOM JÄRJESTYS
5.4 anisotropies
   H0 as a function of different things, esim suunta
   clustering: relation of number of groups and linking length, relevanssi keskimääräiseen etäisyyteen, laske ehkä sufrace densities, groups with massive members, hubble flow and zero points measurements for unbound and clustered haloes (ehkä myös ne clusterist joissa massive halo erikseen)
5.3 scatter
   isotropic + random motions, anisotropy alone (tietty aina scatter myös)
5.5 LG mass
   arvioi massaa edellä esitettyjen perusteella: principal component analysis