新的高红移GPS候选源

T. Mufakharov, A. Mikhailov, M. Mingaliev, Y. Sotnikova
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引用次数: 0

摘要

GHz峰值频谱(GPS)对象是紧凑而强大的射电源(星系和类星体),其无线电频谱的最大值在数百MHz到几GHz之间。这些源作为射电星系的前体很有趣,在高红移时,它们也是早期宇宙的活动星系核。利用RATAN-600射电望远镜于2017-2020年在6个频率(1.2-22.3 GHz)对101个高红移类星体(通量密度大于100 mJy,频率为1.4 GHz)样本进行监测,发现几乎一半(47%)的天体的无线电频谱在GHz频率处最大。我们研究了它们的无线电特性,并根据它们的估计峰值频率、低变异性和文献中的无线电形态确定了10个新的GPS候选源。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
New GPS sources candidates at high redshifts
GHz-peaked spectrum (GPS) objects are compact and powerful radio sources (galaxies and quasars) that have a maximum in the radio spectrum in the range from hundreds of MHz to several GHz. These sources are interesting as precursors of radio galaxies and, at high redshifts, also as active galactic nuclei of the early Universe. A monitoring of a sample of 101 bright (with a flux density of more than 100 mJy at a frequency of 1.4 GHz) quasars at high redshifts ( 𝑧 > 3) with the RATAN-600 radio telescope in 2017–2020 at six frequencies (1.2-22.3 GHz) has revealed that almost half of the objects (47%) have a radio spectrum with the maximum at GHz frequencies. We studied their radio properties and determined 10 new candidates for GPS sources based on their estimated peak frequencies, low variability, and radio morphology from the literature.
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