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.
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 for the underlying observational data used as constraints 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.
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 for the underlying observational data used as constraints 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
Star Formation Histories and Rates from 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 |
