BDMWMfreq (mdr1.bdmwmfreq)

The table has 126524 rows, 32 columns.

Description

Galaxy cluster catalogue for distinct halos from the BDMW catalogue with a total mass (Mtot) above 1014 Msun/h, only for snapshots corresponding to the redshift values z = 0, 0.05, 0.1, 0.16, 0.18, 0.2, 0.27, 0.32, 0.37, 0.4, 0.47, 0.53, 0.61, 0.69, 0.78, 0.89 and 1.

Attribution

In order to properly acknowledge our efforts, we request the following paragraph to be included in the "Acknowledgements" section of any publication which makes use of the simulation data above via the CosmoSim or MultiDark database:

Acknowledgements – Database

The CosmoSim database used in this paper is a service by the Leibniz-Institute for Astrophysics Potsdam (AIP). The MultiDark database was developed in cooperation with the Spanish MultiDark Consolider Project CSD2009-00064.

Acknowledgements – Simulations

The authors gratefully acknowledge the Gauss Centre for Supercomputing e.V. (www.gauss-centre.eu) and the Partnership for Advanced Supercomputing in Europe (PRACE, www.prace-ri.eu) for funding the MultiDark simulation project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre (LRZ, www.lrz.de). The Bolshoi simulations have been performed within the Bolshoi project of the University of California High-Performance AstroComputing Center (UC-HiPACC) and were run at the NASA Ames Research Center.

More information can be found on the credit page.

Columns

Name Type UCD Unit Description
galclusterid long meta.id
meta.main

unique id for the galaxy cluster
bdmid long meta.id
meta.main

bdmId of BDMW table
snapnum short time.epoch

number of snapshot (same as in halo catalogues)
nincat int meta.id

number of galaxy cluster in original data file
x double pos.cartesian.x h-1.Mpc

(comoving) position, x-component
y double pos.cartesian.y h-1.Mpc

(comoving) position, y-component
z double pos.cartesian.z h-1.Mpc

(comoving) position, z-component
vx double phys.veloc
pos.cartesian.x 		km.s-1

(peculiar) velocity, x-component
vy double phys.veloc
pos.cartesian.y 		km.s-1

(peculiar) velocity, y-component
vz double phys.veloc
pos.cartesian.z 		km.s-1

(peculiar) velocity, z-component
np int meta.number

number of particles in halo
mvir double phys.mass h-1.solMass

halo mass - mass of bound particles within Rvir
mtot double phys.mass h-1.solMass

halo mass - mass of all particles within Rvir
rvir double phys.size.radius h-1.Mpc

virial radius
m500 double phys.mass h-1.solMass

halo mass, defined with 500 * critical density calculated from BDMW Mtot with Hu & Kravtsov (2003) method
r500 double phys.size.radius h-1.Mpc

radius for 500 * critical density boundary
t double phys.temperature keV

intra-cluster medium X-ray temperature (kBT) from Mantz et al. (2010) Tci - M500 relation
stateflag short meta.code

flag for cluster dynamical state: 0 = non-cool core cluster, 1 = cool-core cluster
rho0 double phys.density g.cm-3.h(1/2)

intra-cluster medium central gas density (at R = 0)
lx double phys.luminosity
em.X-ray 		h-2.erg.s-1

X-ray thermal bremsstrahlung luminosity within R500
yx double phys.mass
phys.temperature
arith.factor 		h(-2.5).solMass.keV

YX = Mgas * kBT parameter of Kravtsov et al. (2006) within R500, related to the total thermal energy of the ICM
sz double phys.density
phys.temperature
arith.factor 		h(-2.5).Mpc2

integrated thermal Sunyaev-Zel"dovich Compton-Y parameter (as equation 3 of Battaglia et al. 2011) within R500
radioflag short meta.code

flag for radio-loud ( = 1; 10%) and radio-quiet ( = 0; 90%) clusters
xcr double phys.pressure
arith.ratio

ratio of cosmic-ray to thermal pressure volume avarage (<PCR/Pth>) within R500
radiomhz double phys.luminosity
em.radio 		h-2.erg.s-1.Hz-1

synchrotron radio halo luminosity at 120 MHz within R500
radioghz double phys.luminosity
em.radio 		h-2.erg.s-1.Hz-1

synchrotron radio halo luminosity at 1.4 GHz within R500
gammamev double phys.luminosity
em.gamma 		h-2.photon.s-1

gamma-ray luminosity above 100 MeV within R500
gammagev double phys.luminosity
em.gamma 		h-2.photon.s-1

gamma-ray luminosity above 100 GeV within R500
ix int pos.cartesian.x

spatial index, x-direction
iy int pos.cartesian.y

spatial index, y-direction
iz int pos.cartesian.z

spatial index, z-direction
phkey int

Peano-Hilbert-key, i.e. index along the Peano-Hilbert curve