The halo catalogues are created using the ROCKSTAR halo finder and it contains also information from the Merger Trees outputs. They are written in HDF5 format.
We provide halo catalogues for Uchuu, mini-Uchuu and micro-Uchuu. Shin-Uchuu is coming soon.
For Uchuu the number of files per snapshot is 100 with a total size ~1TB. The total data set is ~36TB.
- How to download the data
- Code to read the Halo Catalogue files
- Analysis scripts (examples)
Column# |
Name |
Type |
Unit |
Description |
0 |
scale |
float |
scale factor, same as in snapshot-redshifts table |
|
1 |
id |
int64 |
unique ID for the halo |
|
2 |
desc_scale |
float |
scale factor of the descendant halo, if applicable |
|
3 |
desc_id |
int64 |
ID of the descendant halo, if applicable |
|
4 |
num_prog |
int64 |
number of progenitors |
|
5 |
pid |
int64 |
ID of least massive host halo (-1 if
distinct halo) |
|
6 |
upid |
int64 |
ID of most massive host halo (different
from pid when the halo is within two or more larger
halos) |
|
7 |
desc_pid |
int64 |
pid
of the descendant halo, if applicable |
|
8 |
phantom |
int64 |
flag for phantom halos, nonzero for halos interpolated
across timesteps |
|
9 |
sam_Mvir |
float |
Msun/h |
halo mass, smoothed across accretion history; always
greater than the sum of halo masses of contributing progenitors; only for use
with selected semi-analytic models |
10 |
Mvir |
float |
Msun/h |
halo mass (within virial radius) |
11 |
Rvir |
float |
kpc/h |
halo radius (comoving) |
12 |
rs |
float |
kpc/h |
scale radius (comoving) |
13 |
vrms |
float |
km/s |
velocity dispersion (physical) |
14 |
mmp |
boolean |
flag indicating whether the halo is the most massive
progenitor or not |
|
15 |
scale_of_last_MM |
float |
scale factor of the last major merger (Mass ratio > 0.3) |
|
16 |
vmax |
float |
km/s |
maximum circular velocity (physical) |
17 |
x |
float |
Mpc/h |
halo position (comoving) |
18 |
y |
float |
Mpc/h |
halo position (comoving) |
19 |
z |
float |
Mpc/h |
halo position (comoving) |
20 |
vx |
float |
km/s |
halo velocity (physical, peculiar) |
21 |
vy |
float |
km/s |
halo velocity (physical, peculiar) |
22 |
vz |
float |
km/s |
halo velocity (physical, peculiar) |
23 |
Jx |
float |
(Msun/h)* (Mpc/h)* km/s |
halo angular momentum (physical) |
24 |
Jy |
float |
(Msun/h)* (Mpc/h)* km/s |
halo angular momentum (physical |
25 |
Jz |
float |
(Msun/h)* (Mpc/h)* km/s |
halo angular momentum (physical |
26 |
Spin |
float |
halo spin parameter |
|
27 |
Breadth_first_ID |
int64 |
ID for breadth-first ordering of halos
within a tree |
|
28 |
Depth_first_ID |
int64 |
ID for depth-first ordering of halos
within a tree |
|
29 |
Tree_root_ID |
int64 |
ID of the halo at the last time-step in
the tree |
|
30 |
Orig_halo_ID |
int64 |
original halo ID from halo finder |
|
31 |
Snap_idx |
int64 |
Index of snapshot (in the original
snapshot list) from which halo originated |
|
32 |
Next_coprogenitor_ depthfirst_ID |
int64 |
depthfirst
ID of next coprogenitor |
|
33 |
Last_progenitor_ depthfirst_ID |
int64 |
depthfirst
ID of last progenitor |
|
34 |
Last_mainleaf_ depthfirst_ID |
int64 |
depthfirst
ID of last progenitor on main progenitor branch |
|
35 |
Tidal_Force |
float |
|
Strongest tidal field from any nearby
halo, in dimensionless units (Rhalo / Rhill). Here "nearby" means within 25 Mpc/h comoving
distance. This is applied only for Uchuu. mini- and micro-Uchuu do not have this limitation. |
36 |
Tidal_ID |
int64 |
|
ID of halo exerting strongest tidal force |
37 |
Rs_Klypin |
float |
scale radius determined using Vmax
and Mvir (see Rockstar
paper) |
|
38 |
Mvir_all |
float |
Msun/h |
Mass enclosed within the specified overdensity, including unbound particles |
39 |
M200b |
float |
Msun/h |
Mass enclosed within overdensity
200*rho_b |
40 |
M200c |
float |
Msun/h |
Mass enclosed within overdensity
200*rho_crit |
41 |
M500c |
float |
Msun/h |
Mass enclosed within overdensity
500*rho_crit |
42 |
M2500c |
float |
Msun/h |
Mass enclosed within overdensity
2500*rho_crit |
43 |
Xoff |
float |
Kpc/h |
Offset of density peak from average
particle position (comoving) |
44 |
Voff |
float |
km/s |
Offset of density peak from average
particle velocity (physical) |
45 |
Spin_Bullock |
float |
Bullock spin parameter (J/(sqrt(2)*GMVR)) |
|
46 |
b_to_a |
float |
ratio of second largest shape ellipsoid axes to largest
shape ellipsoid axis (dimensionless); shapes determined by method in Allgood et al. (2006) |
|
47 |
c_to_a |
float |
ratio of smallest shape ellipsoid axes to largest shape
ellipsoid axis (dimensionless) ); shapes determined by method in Allgood et al. (2006) |
|
48 |
A_x |
float |
Kpc/h |
largest shape ellipsoid axis (comoving) |
49 |
A_y |
float |
Kpc/h |
largest shape ellipsoid axis (comoving) |
50 |
A_z |
float |
Kpc/h |
largest shape ellipsoid axis (comoving) |
51 |
b_to_a_500c |
float |
as above but only for particles within overdensity 500*rho_crit
(dimensionless) |
|
52 |
c_to_a_500c |
float |
as above but only for particles within overdensity 500*rho_crit
(dimensionless) |
|
53 |
A_x_500c |
float |
Kpc/h |
as above but only for particles within overdensity 500*rho_crit (comoving) |
54 |
A_y_500c |
float |
Kpc/h |
as above but only for particles within overdensity 500*rho_crit (comoving) |
55 |
A_z_500c |
float |
Kpc/h |
as above but only for particles within overdensity 500*rho_crit (comoving) |
56 |
T_U |
float |
ratio of kinetic to potential energies |
|
57 |
M_pe_Behroozi
|
float |
Msun/h |
Pseudo-evolution corrected masses (very
experimental) |
58 |
M_pe_Diemer |
float |
Msun/h |
Pseudo-evolution corrected masses (very
experimental) |
59 |
Halfmass_Radius |
float |
Kpc/h |
Radius within which 1/2 of Mvir is enclosed |
60 |
rvmax |
float |
Kpc/h |
Radius at Vmax |
61 |
Macc |
float |
Msun/h |
halo mass at accretion |
62 |
Mpeak |
float |
Msun/h |
peak mass over accretion history |
63 |
Vacc |
float |
Vmax at accretion |
|
64 |
Vpeak |
float |
peak Vmax over accretion history |
|
65 |
Halfmass_Scale |
float |
scale factor at which the most massive progenitor (mmp) reaches 0.5*Mpeak |
|
66 |
Acc_Rate_Inst |
float |
Msun/h/yr |
instantaneous halo mass accretion rate |
67 |
Acc_Rate_100Myr |
float |
Msun/h/yr |
halo mass accretion rate averaged over past 100 Myr |
68 |
Acc_Rate_1_Tdyn |
float |
Msun/h/yr |
halo mass accretion rate averaged over past 1*virial dynamical time |
69 |
Acc_Rate_2_Tdyn |
float |
Msun/h/yr |
halo mass accretion rate averaged over past 2*virial dynamical time |
70 |
Acc_Rate_Mpeak |
float |
Msun/h/yr |
growth rate of Mpeak, averaged from
current z to z+0.5 |
71 |
Acc_Log_Vmax _Inst |
float |
Msun/h/yr |
Instantaneous growth rate of Log10(Vmax) |
72 |
Acc_Log_Vmax _1_Tdyn |
float |
Msun/h/yr |
growth rate of Log10(Vmax),
averaged over past 1*virial dynamical time |
73 |
Mpeak_Scale |
float |
scale factor at which Mpeak was
reached |
|
74 |
Acc_Scale |
float |
scale factor at which satellites were (last) accreted |
|
75 |
First_Acc_Scale |
float |
scale factor at which current and former satellites first
passed through a larger halo |
|
76 |
First_Acc_Mvir |
float |
Msun/h |
Mvir at First_Acc_scale |
77 |
First_Acc_Vmax |
float |
km/s |
Vmax at First_Acc_scale |
78 |
Vmax_Mpeak |
float |
km/s |
halo Vmax at the scale at which Mpeak was reached |
79 |
Tidal_Force_Tdyn |
float |
Dimensionless tidal force averaged over
past dynamical time |
|
80 |
Log_Vmax_Vmax_ _max_Tdyn_Tmpeak |
float |
Log10 of Vmax_now
over Vmax@(Tdyn ago) OR Vmax@Mpeak (if and only if Mpeak
happened > 1Tdyn ago) |
|
81 |
Time_to_future _merger |
float |
Gyr |
Time (in Gyr)
until the given halo merges into a larger halo. (-1 if no future merger happens) |
82 |
Future_merger_ MMP_ID |
int64 |
most-massive progenitor of the halo into which the given
halo merges. (-1 if the main progenitor of the future merger halo does not
exist at the given scale factor.) |