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Predictions for deep galaxy surveys with JWST from ΛCDMAddressing the too big to fail problem with baryon physics and sterile neutrino dark matterProperties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologiesShaken and stirred: the Milky Way's dark substructuresSize matters: abundance matching, galaxy sizes, and the Tully–Fisher relation in EAGLEThe effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulationThe Copernicus Complexio: a high-resolution view of the small-scale UniverseThe chosen few: the low-mass haloes that host faint galaxiesThe Copernicus Complexio: statistical properties of warm dark matter haloesFormation ofin situstellar haloes in Milky Way-mass galaxiesBaryon effects on the internal structure of ΛCDM haloes in the EAGLE simulationsBent by baryons: the low-mass galaxy-halo relationCreating mock catalogues of stellar haloes from cosmological simulationsMilky Way mass constraints from the Galactic satellite gapSubhalo statistics of galactic haloes: beyond the resolution limitThe StEllar Counterparts of COmpact high velocity clouds (SECCO) surveyToo small to succeed: the difficulty of sustaining star formation in low-mass haloesnIFTy galaxy cluster simulations – IV. Quantifying the influence of baryons on halo propertiesHow robust are predictions of galaxy clustering?Small-scale galaxy clustering in the eagle simulation
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description
article
@en
im März 2013 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 2013
@uk
name
The abundance of (not just) dark matter haloes
@en
The abundance of
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type
label
The abundance of (not just) dark matter haloes
@en
The abundance of
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prefLabel
The abundance of (not just) dark matter haloes
@en
The abundance of
@nl
P2093
P2860
P50
P356
P1476
The abundance of (not just) dark matter haloes
@en
P2093
Carlos S. Frenk
Jesus Zavala
Till Sawala
P2860
P304
P356
10.1093/MNRAS/STT259
P407
P577
2013-03-09T00:00:00Z
P818
P819
2013MNRAS.431.1366S