New corroborative evidence for the overdensity of galaxies around the radio-loud quasar SDSS J0836+0054 at z=5.8

被引:12
作者
Ajiki, Masaru [1 ]
Taniguchi, Yoshiaki
Murayama, Takashi
Shioya, Yasuhiro
Nagao, Tohru
Sasaki, Shunji S.
Hatakeyama, Yuichiro
Morioka, Taichi
Yokouchi, Asuka
Takahashi, Mari I.
Koizumi, Osamu
机构
[1] Tohoku Univ, Inst Astron, Grad Sch Sci, Aoba Ku, Sendai, Miyagi 9808578, Japan
[2] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
[3] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan
关键词
cosmology : early universe; cosmology : observations; galaxies : evolution; galaxies : formation;
D O I
10.1093/pasj/58.3.499
中图分类号
P1 [天文学];
学科分类号
0704 ;
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.
引用
收藏
页码:499 / 502
页数:4
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