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首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >New corroborative evidence for the overdensity of galaxies around the radio-loud quasar SDSS J0836+0054 at z=5.8
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New corroborative evidence for the overdensity of galaxies around the radio-loud quasar SDSS J0836+0054 at z=5.8

机译:在z = 5.8时射电类星体SDSS J0836 + 0054周围星系密度过大的新佐证

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摘要

Recently, Zheng et al. (2006) found evidence for an overdensity of galaxies around a radio-loud quasar, SDSS J0836+0054, at z = 5.8 (a 5 arcmin(2) field). We examined our deep optical imaging data (B, V, r', i', z', and NB816) taken with the Suprime-Cam on the Subaru Telescope. The NB816 narrow-band filter (X, 815 nm and Delta lambda = 12 nm) is suitable to search for Ly alpha emitters at z approximate to 5.7. We found a new strong Ly alpha emitter at z approximate to 5.7 close to object 13, identified by Zheng et al. (2006). Further, the non-detection of nine objects selected by Zheng et al. (2006) in our B, V, and r' images provides corroborative evidence to indicate that they are high-z objects.
机译:最近,Zheng等。 (2006年)发现了证据,表明在z = 5.8(5 arcmin(2)场)时,无线电大类星体SDSS J0836 + 0054周围的星系存在超密度。我们检查了用斯巴鲁望远镜上的Suprime-Cam拍摄的深光学成像数据(B,V,r',i',z'和NB816)。 NB816窄带滤光片(X,815 nm和Deltaλ= 12 nm)适合在z约为5.7的位置搜索Ly alpha发射器。我们发现了一个新的强Ly发射体,在z处接近物体13处的5.7,由Zheng等人识别。 (2006)。此外,Zheng等人未检测到9个物体。 (2006年)在我们的B,V和r'图像中提供了确凿的证据来表明它们是高Z对象。

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