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Title: The MassiveBlack-II simulation: The evolution of haloes and galaxies to z ~ 0

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stv627· OSTI ID:1214100
 [1];  [2];  [2];  [3];  [2];  [2];  [4];  [2]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States)
  2. Carnegie Mellon Univ., Pittsburgh, PA (United States)
  3. Univ. of Sussex, Brighton (United Kingdom)
  4. The Hebrew Univ., Jerusalem (Israel)

We investigate the properties and clustering of halos, galaxies and blackholes to z = 0 in the high resolution hydrodynamical simulation MassiveBlack-II (MBII). MBII evolves a ΛCDM cosmology in a cubical comoving volume Vbox = (100Mpc/h)³. It is the highest resolution simulation of this size which includes a self-consistent model for star formation, black hole accretion and associated feedback. We provide a simulation browser web application which enables interactive search and tagging of the halos, subhalos and their properties and publicly release our galaxy catalogs to the scientific community. Our analysis of the halo mass function in MBII reveals that baryons have strong effects with changes in the halo abundance of 20–35% below the knee of the mass function (Mhalo 1013.2 M h at z = 0) when compared to dark-matter-only simulations. We provide a fitting function for the halo MF out to redshift z = 11 and discuss its limitations.

Research Organization:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC00112704
OSTI ID:
1214100
Report Number(s):
BNL-108322-2015-JA; KA2301020
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 450, Issue 2; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 232 works
Citation information provided by
Web of Science

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