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Quasar Absorbing Galaxies at z ≤1: Deep Imaging and Spectroscopy in the Field of 3C 336

机译:z≤1的类星体吸收星系:3C 336领域的深度成像和光谱学

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摘要

There are several other galaxies with redshifts near that of 3C 336, suggesting that the QSO is situated in an overdense region, perhaps a galaxy cluster. Previously published reports of a cluster around 3C 336 were largely misled by the presence of many foreground galaxies seen in projection near the QSO. It is possible that a reported measurement of weak shear gravitational lensing in this field may be produced by the QSO cluster itself, since there appear to be no other groups or clusters in the foreground. We find no evidence for a normal, bright QSO host galaxy, although there are several faint objects very close to the quasar and at similar redshift that might either be companions or part of a disorganized QSO host.
机译:还有其他一些星系,它们的红移接近3C 336的星系,这表明QSO位于超稠密区域,也许是一个星系团。先前发表的有关3C 336附近星团的报告很大程度上被QSO附近投影中看到的许多前景星系的存在所误导。 QSO群集本身可能会报告该领域中的弱剪切重力透镜的测量结果,因为前景中似乎没有其他组或群集。我们没有找到正常,明亮的QSO主机星系的证据,尽管有一些微弱的物体非常接近类星体,并且处于类似的红移状态,可能是同伴或者是混乱的QSO主机的一部分。

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