J/ApJS/100/281ivo://CDS.VizieR/J/ApJS/100/281doi:10.26093/cds/vizier.21000281CDSSugiyama N.1998-03-05T21:10:08Z1998-03-05T22:10:04ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frstellar-evolutionary-modelsCosmic microwave background (CMB) anisotropies and density fluctuations are calculated for flat cold dark matter (CDM) models with a wide range of parameters, viz., {OMEGA}_0,h_, and {OMEGA}_B_, for standard recombination and for various epochs of reionization. Tables of the power spectrum of CMB anisotropies in the form of C_l_ values as a function of l are presented. Although the Harrison-Zeldovich initial spectrum is assumed in these tables, we present simple approximations for obtaining the C_l_ values corresponding to a tilted spectrum from those with a Harrison-Zeldovich spectrum. Values of {sigma}_8_ are derived for the matter density spectrum, with {sigma}(10deg), fixed Q_(rms-PS) and COBE Differential Microwave Radiometer (DMR) 2yr normalizations. Simple modifications of the fitting formula for the density transfer function are given which are applicable for models with high baryon density. By using both numerical results and these fitting formulae, we calculate the relation between {sigma}_8_ and Q_(rms-PS) and find good agreement. In addition, the velocity fields are calculated.1995ApJS..100..281Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/100/281CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/100/281https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/100/281http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/100/281https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/100/281https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/100/281http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/100/281GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/100/281/table110^10^xl(l+1)C_l_/2{pi} for h=0.3 and {OMEGA}_0_=1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBs_10Standard recombination, {OMEGA}_B_=0.10stat.paramfloatOBs_14Standard recombination, {OMEGA}_B_=0.14stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatOBr_10Reionization (tau=1), {OMEGA}_B_=0.10stat.paramfloatOBr_14Reionization (tau=1), {OMEGA}_B_=0.14stat.paramfloatJ/ApJS/100/281/table210^10^xl(l+1)C_l_/2{pi} for h=0.5 and {OMEGA}_0_=1lModel parameter, lstat.paramintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_05Standard recombination, {OMEGA}_B_=0.05stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBs_10Standard recombination, {OMEGA}_B_=0.10stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_05Reionization (tau=1), {OMEGA}_B_=0.05stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatOBr_10Reionization (tau=1), {OMEGA}_B_=0.10stat.paramfloatJ/ApJS/100/281/table310^10^xl(l+1)C_l_/2{pi} for h=0.8 and {OMEGA}_0_=1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_02Standard recombination, {OMEGA}_B_=0.02stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBs_10Standard recombination, {OMEGA}_B_=0.10stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_02Reionization (tau=1), {OMEGA}_B_=0.02stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatOBr_10Reionization (tau=1), {OMEGA}_B_=0.10stat.paramfloatJ/ApJS/100/281/table410^10^xl(l+1)C_l_/2{pi} for h=0.5, {OMEGA}_0_=0.1 and {lambda}=0.9recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_05Standard recombination, {OMEGA}_B_=0.05stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_05Reionization (tau=1), {OMEGA}_B_=0.05stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table510^10^xl(l+1)C_l_/2{pi} for h=0.5, {OMEGA}_0_=0.2 and {lambda}=0.8recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_05Standard recombination, {OMEGA}_B_=0.05stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_05Reionization (tau=1), {OMEGA}_B_=0.05stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table610^10^xl(l+1)C_l_/2{pi} for h=0.5, {OMEGA}_0_=0.3 and {lambda}=0.7recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_05Standard recombination, {OMEGA}_B_=0.05stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_05Reionization (tau=1), {OMEGA}_B_=0.05stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table710^10^xl(l+1)C_l_/2{pi} for h=0.5, {OMEGA}_0_=0.4 and {lambda}=0.6recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_05Standard recombination, {OMEGA}_B_=0.05stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_05Reionization (tau=1), {OMEGA}_B_=0.05stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table810^10^xl(l+1)C_l_/2{pi} for h=0.8, {OMEGA}_0_=0.1 and {lambda}=0.9recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_02Standard recombination, {OMEGA}_B_=0.02stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_02Reionization (tau=1), {OMEGA}_B_=0.02stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table910^10^xl(l+1)C_l_/2{pi} for h=0.8, {OMEGA}_0_=0.2 and {lambda}=0.8recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_02Standard recombination, {OMEGA}_B_=0.02stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_02Reionization (tau=1), {OMEGA}_B_=0.02stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table1010^10^xl(l+1)C_l_/2{pi} for h=0.8, {OMEGA}_0_=0.3 and {lambda}=0.7OBs_02Standard recombination, {OMEGA}_B_=0.02stat.paramfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_02Reionization (tau=1), {OMEGA}_B_=0.02stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table1110^10^xl(l+1)C_l_/2{pi} for h=0.8, {OMEGA}_0_=0.4 and {lambda}=0.6recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOBs_01Standard recombination, {OMEGA}_B_=0.01stat.paramfloatOBs_02Standard recombination, {OMEGA}_B_=0.02stat.paramfloatOBs_03Standard recombination, {OMEGA}_B_=0.03stat.paramfloatOBs_06Standard recombination, {OMEGA}_B_=0.06stat.paramfloatOBr_01Reionization (tau=1), {OMEGA}_B_=0.01stat.paramfloatOBr_02Reionization (tau=1), {OMEGA}_B_=0.02stat.paramfloatOBr_03Reionization (tau=1), {OMEGA}_B_=0.03stat.paramfloatOBr_06Reionization (tau=1), {OMEGA}_B_=0.06stat.paramfloatJ/ApJS/100/281/table1210^10^xl(l+1)C_l_/2{pi} for {OMEGA}_0_.h approx. 0.25 and Omega_B_.h^2^=0.125recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramintOs_02Std recombination, {OMEGA}_0_=0.2, h=1.0stat.paramfloatOs_03Std recombination, {OMEGA}_0_=0.3, h=0.833stat.paramfloatOs_04Std recombination, {OMEGA}_0_=0.4, h=0.625stat.paramfloatOs_05Std recombination, {OMEGA}_0_=0.5, h=0.5stat.paramfloatOr_02Reion. (tau=1), {OMEGA}_0_=0.2, h=1.0stat.paramfloatOr_03Reion. (tau=1), {OMEGA}_0_=0.3, h=0.833stat.paramfloatOr_04Reion. (tau=1), {OMEGA}_0_=0.4, h=0.625stat.paramfloatOr_05Reion. (tau=1), {OMEGA}_0_=0.5, h=0.5stat.paramfloatJ/ApJS/100/281/table1310^10^xl(l+1)C_l_/2{pi} for h=0.5, {OMEGA}_0_=1 and {OMEGA}_B_=0.05tau_05Tau=0.5stat.paramfloattau_08Tau=0.8stat.paramfloattau_15Tau=1.5stat.paramfloattau_20Tau=2.0stat.paramfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlModel parameter, lstat.paramint