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首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21a€‰cm-line fluctuations
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Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21a€‰cm-line fluctuations

机译:21a€?cm-线红移中具有方差和偏度的电离时代模型的预期约束

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Theredshifted21a€‰cm-linesignalfromneutralhydrogenintheintergalacticmedium(IGM)givesadirectprobeoftheepochofreionization(EoR).Inthispaper,weinvestigatethepotentialofthevarianceandskewnessoftheprobabilitydistributionfunctionofthe21a€‰cmbrightnesstemperatureforconstrainingEoRmodels.Thesestatisticalquantitiesaresimple,easytocalculatefromtheobservedvisibility,andthussuitablefortheearlyexplorationoftheEoRwithcurrenttelescopessuchastheMurchisonWidefieldArray(MWA)andLOwFrequencyARray(LOFAR).Weshow,byperformingFisheranalysis,thatthevarianceandskewnessatz=7a€“9arecomplementarytoeachothertoconstraintheEoRmodelparameterssuchastheminimumvirialtemperatureofhaloswhichhostluminousobjects,ionizingefficiency,andmeanfreepathofionizingphotonsintheIGM.Quantitatively,theconstrainingpowerhighlydependsonthequalityoftheforegroundsubtractionandcalibration.Wegiveabestcaseestimateoftheconstraintsontheparameters,neglectingthesystematicsotherthanthethermalnoise.
机译:Theredshifted21a€‰厘米-linesignalfromneutralhydrogenintheintergalacticmedium(IGM)givesadirectprobeoftheepochofreionization(EOR).Inthispaper,weinvestigatethepotentialofthevarianceandskewnessoftheprobabilitydistributionfunctionofthe21a€‰cmbrightnesstemperatureforconstrainingEoRmodels.Thesestatisticalquantitiesaresimple,easytocalculatefromtheobservedvisibility,andthussuitablefortheearlyexplorationoftheEoRwithcurrenttelescopessuchastheMurchisonWidefieldArray(MWA)andLOwFrequencyARray(LOFAR).Weshow,byperformingFisheranalysis,thatthevarianceandskewnessatz = 7A€“9arecomplementarytoeachothertoconstraintheEoRmodelparameterssuchastheminimumvirialtemperatureofhaloswhichhostluminousobjects,ionizingefficiency,andmeanfreepathofionizingphotonsintheIGM.Quantitatively因此,约束力在很大程度上取决于前减法和校准的质量。最好不要估算参数的约束条件,而忽略热噪声以外的系统参数。

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