Open aphearin opened 7 months ago
As a first pass, I compared the peculiar velocity distributions in cosmoDC2 and roman_rubin_v1.1.2_elais (in a singlr healpixel). Here are 2 plots: the first looks at all non synthetic galaxies, the second shows galaxies with log_10(M*) > 9.5. Apart from having more galaxies in roman-rubin, the distributions are similar.
And now with the distributions separated by centrals and satellites: Again, they look very similar.
These velocities are in comoving units.
As reported by Rick Kessler, our peculiar velocities are suspiciously high. In the plot below, a cut on stellar mass logsm>9.5 was made. The typical velocity is a bit north of 500 km/s, which is a bit uncomfortably high. The very first check would be to repeat this measurement separately for host halos and satellites.