首页> 外文期刊>The Astrophysical journal >DISCOVERY OF A z = 4.93, X-RAY-SELECTED QUASAR BY THE CHANDRA MULTIWAVELENGTH PROJECT (ChaMP)
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DISCOVERY OF A z = 4.93, X-RAY-SELECTED QUASAR BY THE CHANDRA MULTIWAVELENGTH PROJECT (ChaMP)

机译:钱德拉多波长项目(ChaMP)发现X射线选择的类比z = 4.93

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摘要

We present X-ray and optical observations of CXOMP J213945.0-234655, a high-redshift (z = 4.93) quasar discovered through the Chandra Multiwavelength Project (ChaMP). This object is the most distant X-ray-selected quasar published, with a rest-frame X-ray luminosity of L_X = 5.9 x 10~(44) ergs s~(-1) (measured in the 0.3-2.5 keV band and corrected for Galactic absorption). CXOMP J213945.0-234655 is a g′ dropout object (>26.2), with r′ = 22.87 and i′ = 21.36. The rest-frame X-ray-to-optical flux ratio is similar to quasars at lower redshifts and slightly X-ray bright relative to z > 4 optically selected quasars observed with Chandra. The ChaMP is beginning to acquire significant numbers of high-redshift quasars to investigate the X-ray luminosity function out to z ~ 5.
机译:我们将介绍通过Chandra多波长项目(ChaMP)发现的高红移(z = 4.93)类星体CXOMP J213945.0-234655的X射线和光学观察。该物体是已公布的最遥远的X射线类星体,其静止帧的X射线发光度为L_X = 5.9 x 10〜(44)ergs s〜(-1)(在0.3-2.5 keV波段和已校正银河吸收)。 CXOMP J213945.0-234655是g'丢失对象(> 26.2),r'= 22.87,i'= 21.36。相对于使用Chandra观察到的z> 4光学选择类星体,其余帧的X射线与光通量之比类似于处于较低红移且略微X射线亮的类星体。 ChaMP开始获取大量的高红移类星体,以研究z〜5的X射线光度函数。

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