These  files include  the most  of the  data shown  in the  Figures of
Weinmann  et al.  (2013)  on  the circular  velocity  of galaxies  and
haloes.

For questions please e-mail: weinmann@strw.leidenuniv.nl

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Fig. 1c: 
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fig1c_w13.dat
Average density vs. radius from Fig. 1c  
1: radius in kpc
2: density in Msun/kpc^3 at z=0
3: at z=1
4: at z=2
5: at z=3
6: at z=4

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Fig. 3
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fig3_xx_w13.dat
Numbers 67, 52 etc. indiciate the snapshot in the MS-II simulation.
67: z=0
52: z=0.508 (not used in plot)
45: z=0.988  (denoted z=1)
36: z=2.07  (denoted z=2)
31: z=3.06 (denoted z=3)
28: z=3.86 (denoted z=4)

1: log(halo) mass in M_sun
2: v: log(velocity) in km/s
3: number density in dex^{-1}h^3Mpc^{-3}, halo mass
4: number density in dex^{-1}h^3Mpc^{-3}, v=v_vir
5: number density in dex^{-1}h^3Mpc^{-3}, v=v_20 (DM only)
6: number density in dex^{-1}h^3Mpc^{-3}, v=v_max

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Fig. 4
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average_history_xx.dat
1: redshift
2: m200 [msun]
3: v_20 [km/s]
4: vvir [km/s]
5: vmax [km/s]
6: sigma_20, b, AC [km/s] (needs to be multiplied by sqrt(2) to get v_20, b, AC)

xx in the file names indicate different halo mass bins at z=0, with 10 lowest and 3500 highest, 
expressed in units of the MS-II particle mass.

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Fig. 5 lower panels (cumulative)
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cumulative_v20_w13.dat: only DM
cumulative_v20_bar_ac_w13.dat: including the effects of baryons + AC

1: log(v20) [km/s] 
2: log(N) [h^3Mpc^-3] at z=0 
3: at z=0.508
4: at z=0.988
5: at z=2.07
6: at z=3.06
7: at z=3.86

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Fig. 5 upper panels (differential)
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diff_xx_w13.dat
xx indicating snapshots, see above

1: log(velocity) in km/s
2: number density in dex^{-1}h^3Mpc^{-3}, v20, DM only [needs to be divided by sqrt(2) to get sigma. Also, this is the same
qunatity as in fig3_xx_w13.dat, column 5]
3: number density in dex^{-1}h^3Mpc^{-3}, v20 including baryons [needs to be divided by sqrt(2) to get sigma]
4: number density in dex^{-1}h^3Mpc^{-3}, v20 including baryons+AC [needs to be divided by sqrt(2) to get sigma]



