Probing the Star-Formation Epoch with the Wilkinson Microwave Anisotropy Probe (WMAP) Data and High-Redshift QSOs

Yokoyama Juna€?Ichi

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Probing the Star-Formation Epoch with the Wilkinson Microwave Anisotropy Probe (WMAP) Data and High-Redshift QSOs

机译：用威尔金森微波各向异性探测器（WMAP）数据和高红移QSO探测恒星形成时代

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UsingthevaluesofthecosmologicalparametersobtainedfromtheWilkinsonMicrowaveAnisotropyProbe(WMAP)andthecosmologicalchemicalclockobservedfromhigh-redshiftquasars,itisshownthattheformationepochofprecursorsoftypeIasupernovaeshouldhavestartedataredshiftof$$z_{mathrm{F}}gt9.5$$$$z_{mathrm{F}}gt9.5$$,andthat$$z_mathrm{F}$$issensitiveonlyto$$Omega_{mathrm{m0}},h^2$$inflat$$Lambda$$CDMcosmology.

机译：UsingthevaluesofthecosmologicalparametersobtainedfromtheWilkinsonMicrowaveAnisotropyProbe（WMAP）andthecosmologicalchemicalclockobservedfromhigh-redshiftquasars，itisshownthattheformationepochofprecursorsoftypeIasupernovaeshouldhavestartedataredshiftof $$ Z_ {mathrm {F}} gt9.5 $$$$ Z_ {mathrm {F}} gt9.5 $$，andthat $$ z_mathrm {F} $$ issensitiveonlyto $$ Omega_ {mathrm {m0}}，h ^ 2 $ inflat $$ Lambda $$ CDMcosmology。

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《PASJ: Publications of the Astronomical Society of Japan》 |2003年第3期|共页
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Yokoyama Juna€?Ichi;
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Probing the Star-Formation Epoch with the Wilkinson Microwave Anisotropy Probe (WMAP) Data and High-Redshift QSOs

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