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首页> 外文期刊>The Astrophysical Journal. Letters >SDSS J013127.34?032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z = 5.18 WITH EXTREMELY HIGH LUMINOSITY
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SDSS J013127.34?032100.1: A NEWLY DISCOVERED RADIO-LOUD QUASAR AT z = 5.18 WITH EXTREMELY HIGH LUMINOSITY

机译:SDSS J013127.34?032100.1:z = 5.18时新发现的无线电量极大的类星体,具有极高的发光度

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摘要

Very few of the z>5 quasars discovered to date have been radio-loud, with radio-to-optical flux ratios (radioloudness parameters) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34?032100.1 (J0131?0321 in short), at z = 5.18± 0.01 using the Lijiang 2.4 m and Magellan telescopes. J0131?0321 has a spectral energy distribution consistent with that of radio-loud quasars.With an i-band magnitude of 18.47 and a radio flux density of 33 mJy, its radio-loudness parameter is ~100. The optical and nearinfrared spectra taken by Magellan enable us to estimate its bolometric luminosity to be L_(bol) ~ 1.1 × 10~(48) erg s~(~(?1)), approximately 4.5 times greater than that of the most distant quasar known to date. The black hole mass of J0131?0321 is estimated to be 2.7 × 10~9M_⊙, with an uncertainty up to 0.4 dex. Detailed physical properties of this high-redshift, radio-loud, potentially super-Eddington quasar can be probed in the future with more dedicated and intensive follow-up observations using multi-wavelength facilities.
机译:迄今为止,发现的z> 5类星体中只有极少数是无线电大声的,无线电波与光通量之比(辐射声度参数)高于10。这里我们报告发现了光学发光的无线电大声类星SDSS J013127。 34?032100.1(简称J0131?0321),使用丽江2.4 m和麦哲伦望远镜在z = 5.18±0.01处。 J0131?0321的光谱能量分布与无线电类星体的光谱能量分布一致。i波段幅度为18.47,无线电通量密度为33 mJy,其无线电响度参数为〜100。麦哲伦拍摄的光学和近红外光谱使我们能够估计其辐射热度为L_(bol)〜1.1×10〜(48)erg s〜(〜(?1)),约为最远距离的4.5倍。迄今为止已知的类星体。 J0131?0321的黑洞质量估计为2.7×10〜9M_⊙,不确定度最高为0.4 dex。将来可以使用多波长设备,通过更专门,更深入的后续观察,来探究这种高红移,无线电响,可能是超爱丁顿类星体的详细物理特性。

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