Trinity Model for Supermassive Black Holes in Galaxies
See Haowen Zhang's Trinity Data/Code repository here.
UniverseMachine Data Release 1 + NeutralUniverseMachine
JWST lightcones (0<z<15) covering all CANDELS fields are available here.
Data Release 1 statistics and constraints available here (213 MB). Most recent release: 7/26/2019. Includes observational constraints (SMFs, UVLFs, SSFRs, CSFRs, UVSM relations, correlation functions, and central environment-dependent quenched fractions) as well as derived constraints (e.g., SMHM relation, SFR(Mh,z), star formation histories, quenched fractions, correlation function/weak lensing predictions, etc.). Those wishing just for the underlying observations behind the empirical constraints above can download a smaller dataset here (60K).
The UniverseMachine code is publicly available here, including a README for use of the constraints above and catalogs below. This is constantly updated; the code used to generate Data Release 1 is frozen here.
Catalogs (ASCII and binary) and star formation histories generated for Bolshoi-Planck are also available. Lightcones for Bolshoi-Planck (best for z<10) for all CANDELS fields are available here. Base files to generate new catalogs for Bolshoi-Planck are available here. Finally, a movie is available here.
Gas masses from the NeutralUniverseMachine paper by Hong Guo are available for Bolshoi-Planck here.
Binary UniverseMachine catalogs for the MDPL2 (1000 Mpc/h), the SMDPL (400 Mpc/h), and the VSMDPL (160 Mpc/h) high-resolution simulations are available here: MDPL2, SMDPL, VSMDPL.
Comparison with past results from Behroozi, Wechsler, Conroy (2013) is available here. An interactive map of joint parameter distributions is available here.
Data Release 1 statistics and constraints available here (213 MB). Most recent release: 7/26/2019. Includes observational constraints (SMFs, UVLFs, SSFRs, CSFRs, UVSM relations, correlation functions, and central environment-dependent quenched fractions) as well as derived constraints (e.g., SMHM relation, SFR(Mh,z), star formation histories, quenched fractions, correlation function/weak lensing predictions, etc.). Those wishing just for the underlying observations behind the empirical constraints above can download a smaller dataset here (60K).
The UniverseMachine code is publicly available here, including a README for use of the constraints above and catalogs below. This is constantly updated; the code used to generate Data Release 1 is frozen here.
Catalogs (ASCII and binary) and star formation histories generated for Bolshoi-Planck are also available. Lightcones for Bolshoi-Planck (best for z<10) for all CANDELS fields are available here. Base files to generate new catalogs for Bolshoi-Planck are available here. Finally, a movie is available here.
Gas masses from the NeutralUniverseMachine paper by Hong Guo are available for Bolshoi-Planck here.
Binary UniverseMachine catalogs for the MDPL2 (1000 Mpc/h), the SMDPL (400 Mpc/h), and the VSMDPL (160 Mpc/h) high-resolution simulations are available here: MDPL2, SMDPL, VSMDPL.
Comparison with past results from Behroozi, Wechsler, Conroy (2013) is available here. An interactive map of joint parameter distributions is available here.
Bolshoi-Planck, Small MultiDark-Planck, and MultiDark-Planck2 Catalogs and Merger Trees
Simulation Sizes: 250 Mpc/h (Bolshoi-Planck), 1 Gpc/h (MultiDark-Planck2), 400 Mpc/h (Small MultiDark-Planck)
Bolshoi-Planck: Halo Catalogs and Merger Trees
SMDPL: Halo Catalogs and Merger Trees
MDPL2: Halo Catalogs and Merger Trees
Bolshoi-Planck: Halo Catalogs and Merger Trees
SMDPL: Halo Catalogs and Merger Trees
MDPL2: Halo Catalogs and Merger Trees
Behroozi et al. (2013):
Star formation histories and rates for z=0 to z=8. Also includes stellar mass to halo mass relationships. Most recent release: 5/29/2013. For 2D density plots of the parameter space, click here.
All results from Behroozi, Wechsler, & Conroy 2013a and 2013b. Important note about clusters: BCG masses are very sensitive to profile fitting, BCG/ICL separation, and background subtraction. Please contact us to make sure the stellar mass definition is consistent if you are comparing to other cluster results.
All results from Behroozi, Wechsler, & Conroy 2013a and 2013b. Important note about clusters: BCG masses are very sensitive to profile fitting, BCG/ICL separation, and background subtraction. Please contact us to make sure the stellar mass definition is consistent if you are comparing to other cluster results.
| sfh_z0_z8.tar.gz |
The compiled observational constraints (stellar mass functions, cosmic star formation rates, and specific star formation rates) are also available here:
| observational-data.tar.gz |
