See also the review of simulation methods and codes at https://arxiv.org/abs/1909.07976, "Cosmological simulations of Galaxy Formation," a review paper by Vogelsberger, Marinacci, Torrey and Puchwein.
Galaxy and some other Mock Catalogues available online
Our mock catalog is based on SHAM, highly relying on the S82-MGC
catalog and the Rockstar subhalo catalog in the Multidark N-body
simulation (currently we are using MDR1 ). We prepare ascii (.txt)
and FITS (.fits) files, and explanations for each column can be
found in the header in the ascii file or in the header comments in
the primary HDU in the FITS file. In case you need other halo
properties not included in the mock catalog, you may find them in
the Multidark database by refering to the HALO_ID or ask Shun Saito.
has stellar mass,
CMASSFLAG,X,Y,Z, V_PEAK,
M_VIR,HALO_ID,distinct halo
CAMELS contains 4,233 simulations: 2,049 N-body simulations and 2,184 hydrodynamic simulations.
The CAMELS simulations can be organized in three different suites:
IllustrisTNG. This suite contains 1,092 hydrodynamic simulations that have been run with the AREPO code employing the same subgrid physics as the original IllustrisTNG simulations.
SIMBA. This suite contains 1,092 hydrodynamic simulations that have been run with the GIZMO code employing the same subgrid physics as the original SIMBA simulation.
N-body. This suite contains 2,049 N-body simulation. For each CAMELS hydrodynamic simulation there is an N-body simulation with the same cosmology and value of the initial random seed as its hydrodynamic counterpart.
Release paper https://arxiv.org/abs/2010.00619, The CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations
Results from 3 simulation suites, MultiDark, Bolshoi and CLUES
Dark matter catalogues of various sizes and resolutions (MultiDark, Bolshoi)
MultiDark release paper
, with 3 SAMS added to dark matter halos for 1 Gpc/h^3 and mass resolution 1.5 e9 M_o/h mass resolution
and 126 time steps from z=17 to 0, Planck cosmology.
Galacticus added,SAG added, and SAGE added.
Properties include SFR, M*, SDSS bands, bulge, black hole, etc properties.
Constrained 64 Mpc/h side box simulations of the local universe, with and without gas (CLUES)
A mass limited complete volume sample of resimulated objects at high-z (from z ~ 3 to 6). To this end, we have simulated a cubic box 200 h-1 Mpc with different resolutions and physics, ranging from 5123 to 20483 particles. These simulations of the whole box have been used to identify the objects of interest in order to generate the initial conditions for the resimulations.
2 with dark matter only, (512,1024)3 particles, one with sph+rad physics+sfr+winds (1024)3 + (1024)3 particles
LSST-DESC
The LSST DESC catalog and simulated sky survey from the DESC Data Challenge 2 (DC2) based on the HACC Outer Rim simulation are here:
https://lsstdesc-portal.nersc.gov/
Data products are publicly available from HACC simulations. The main site is:
https://cosmology.alcf.anl.gov/
Results are available from a subset of the Mira-Titan simulation suite (subset of 11 cosmologies out of 110+), and the Outer Rim, QContinuum, Last Journey, and Farpoint simulations. The associated papers are:
The first, TNG100, is a "re-do" of Illustris, using the same initial conditions and with the new TNG model for galaxy formation physics. TNG300 (~300 Mpc) is the large-volume, with ~20x more objects in any given mass range (including ~300 clusters above 10^14).
Please find more information here:
Gas and Dark matter, and Dark matter only, AREPO code, WMAP9 cosmology,
106.5 Mpc side boxes with different resolution.
properties of gas (per cell), dark matter particles, wind/stars particles, tracers, black holes, galaxies (with sunrise, stellar images, 13 redshifts), morphologies, stellar mass histories, black hole histories, etc, see list here.
models include halo/galaxy merger trees and rich list of galaxy properties, depending on particular model choice (includes intrinsic properties such as halo spin, central/sat, etc and observables including sdss bands, dust, plus many other things)
The mockFactory is a collection of public code to help create mock
galaxy catalogs for BOSS (and other surveys). This includes
populating simulation halo catalogs (galaxy bias) and adding survey
realism. Data at NERSC and generally available.
43100 full N-body simulations spanning more than 7000 cosmological models in the {Omega_m,Omega_b,h,ns,sigma_8,M_nu,w} hyperplane
At a single redshift the simulations contain more than 8.5 trillions of particles over a combined volume of 43100 (Gpc/h)3
Billions of dark matter halos and cosmic voids have been identified in the simulations
Release of the Petabyte of data generated, comprising hundreds of thousands of simulation snapshots at multiple redshifts, halo and void catalogs, together with millions of summary statistics such as power spectra, bispectra, correlation functions, marked power spectra, and estimated probability density functions.
This is a simulation of the extragalactic sky including clustering based on empirical prescriptions. The method used to build this simulated catalog is described in Bethermin, Wu, Lagache, et al. , (sub. to A&A). Please refer to this paper if you use this catalog.
Based on Bolshoi (DM, in below), lightcone 1.4deg x 1.4deg from 0 < z < 10, comoving volume of 0.17 Gpc3
Includes ra, dec, mhalo, mstar, sfr, magnification from lensing, and what is found in a wide range of various filters for each halo.
>800 independent N-body simulations ran with CUBEP3M,
each post-processed into 100 sq.deg. light-cones. Many observables
available including:
mock weak lensing galaxy catalogues
spectroscopic galaxy surveys catalogues
lensing maps reconstructed from the cosmological microwave background.
Also available on request: mass maps, shear maps and dark matter halo catalogues,
as well as some two-point correlation function measurements such as
P(k,z=0), xi+/-, C_ell^kappa, w(theta), Delta(Sigma).
The 21cm Simulated Signal Database is a publicly available repository of 21cm signal lightcones produced with a number of large radiative-hydrodynamics simulations.
The simulations are described in 21SSD: a public database of simulated 21-cm signals from the epoch of reionization, Semelin, Eames, Bolgar and Caillat, 2017. https://arxiv.org/abs/1707.02073.
Mocks of nside=2048 of CIB (in MJy/sr) intensity, Compton-y, CMB lensing convergence, and lensed and unlensed CMB temperature, all from the same 8192^3 16 Gpc simulation. The minimum halo mass used was 2.62e13 M200,M.
Higher resolution maps and different frequencies are available upon request.
Please email jcohn@berkeley.edu
to add correct/references. Thank you to M. Alvarez, S. Habib and M. White for suggestions.