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SXDFa€“ALMA 2-arcmin2 deep survey: 1.1-mm number counts

机译:SXDFa –“ ALMA 2-arcmin2”深层调查:1.1毫米计数

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Wereport1.1-mmnumbercountsrevealedwiththeAtacamaLargeMillimeter/submillimeterArray(ALMA)intheSubaru/XMM-NewtonDeepSurveyField(SXDF).TheadventofALMAenablesustorevealmillimeter-wavelengthnumbercountsdowntothefaintendwithoutsourceconfusion.However,previousstudiesarebasedontheensembleofserendipitouslydetectedsourcesinfieldsoriginallytargetingdifferentsourcesandcouldbebiasedduetotheclusteringofsourcesaroundthetargets.Wederivenumbercountsinthefluxrangeof0.2a€“2a€‰mJybyusing23(a‰¥4??)sourcesdetectedinacontinuous2.0-arcmin2areaoftheSXDF.Thenumbercountsareconsistentwithpreviousresultswithinerrors,suggestingthatthecountsderivedfromserendipitouslydetectedsourcesarenotsignificantlybiased,althoughtherecouldbefield-to-fieldvariationduetothesmallsurveyarea.Byusingthebest-fittingfunctionofthenumbercounts,wefindthata??40%oftheextragalacticbackgroundlightat1.1a€‰mmisresolvedatS1.1mm0.2a€‰mJy.
机译:Wereport1.1-mmnumbercountsrevealedwiththeAtacamaLargeMillimeter / submillimeterArray(ALMA)intheSubaru / XMM-NewtonDeepSurveyField(SXDF).TheadventofALMAenablesustorevealmillimeter-wavelengthnumbercountsdowntothefaintendwithoutsourceconfusion.However,previousstudiesarebasedontheensembleofserendipitouslydetectedsourcesinfieldsoriginallytargetingdifferentsourcesandcouldbebiasedduetotheclusteringofsourcesaroundthetargets.Wederivenumbercountsinthefluxrangeof0.2a€“2A€‰mJybyusing23(一个‰¥4?)sourcesdetectedinacontinuous2.0-arcmin2areaoftheSXDF。该数量计数与先前的错误结果一致,这表明从小巧的测量区域来看,应该认为源于偶然发现的偶然发现的来源的计数没有显着偏差。通过使用最佳的1.1系数的最佳拟合函数,我们可以计算出1.1%的最佳拟合度为1的百分之二十。

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