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首页> 外文期刊>The Astrophysical Journal. Letters >THE FAINTEST RADIO SOURCE YET: EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE GRAVITATIONAL LENS SDSS J1004+4112
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THE FAINTEST RADIO SOURCE YET: EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE GRAVITATIONAL LENS SDSS J1004+4112

机译:最微弱的无线电源:扩展了非常大的阵列观测的引力透镜SDSS J1004 + 4112

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摘要

We present new radio observations of the large-separation gravitationally lensed quasar SDSS J1004+4112, taken in a total of 6 hr of observations with the Expanded Very Large Array. The maps reach a thermal noise level of approximately 4μJy. We detect four of the five lensed images at the 15–35μJy level, representing a source of intrinsic flux density, after allowing for lensing magnification, of about 1μJy, intrinsically probably the faintest radio source yet detected. This reinforces the utility of gravitational lensing in potentially allowing us to study nJylevel sources before the advent of the Square Kilometre Array. In an optical observation taken three months after the radio observation, image C is the brightest image, whereas the radio map shows flux density ratios consistent with previous optical observations. Future observations separated by a time delay will give the intrinsic flux ratios of the images in this source.
机译:我们呈现出大型重力透镜Quasar SDSS J1004 + 4112的新型无线电观察,总共6小时与膨胀的非常大的阵列一起观察。 地图达到大约4μJY的热噪声水平。 我们在15-35μJY水平下检测五个镜头图像中的四个,代表内在磁通密度的源,在允许镜头倍率之后,约1μJY,本质上可能是尚未检测到的最微量的无线电源。 这加强了引力透镜的效用,潜在允许我们在平方公里阵列的出现前研究Njylevel来源。 在无线电观察之后三个月拍摄的光学观察中,图像C是最亮的图像,而无线电映射显示与先前的光学观察一致的磁通密度比。 通过时间延迟分离的未来观察将提供该来源中图像的内在通量比率。

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