Wide-Field Optical Variability Survey for Low-Luminosity AGN with Suprime-Cam

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作者
Morokuma, Tomoki [1 ,2 ]
Doi, Mamoru [2 ]
Yasuda, Naoki [3 ]
Akiyama, Masayuki [4 ]
Sekiguchi, Kazuhiro [1 ]
Furusawa, Hisanori [4 ]
Kashikawa, Nobunari [1 ]
Nagao, Tohru [1 ]
Ueda, Yoshihiro [5 ]
Totani, Tomonori [5 ]
Oda, Takeshi [5 ]
Murayama, Takashi [6 ]
Ouchi, Masami [7 ]
Watson, Mike G. [8 ]
机构
[1] Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[2] Univ Tokyo, Inst Astron, Mitaka, Tokyo 1818588, Japan
[3] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[4] NAOJ, Subaru Telescope, Hilo, HI 96720 USA
[5] Kyoto Univ, Dept Astron, Kyoto 6068502, Japan
[6] Tohoku Univ, Inst Astron, Sendai, Miyagi 9808578, Japan
[7] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[8] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present our optical variability survey for low-luminosity active galactic nuclei (AGN) with Subaru Suprime Cam. We found that a significant fraction of variable AGN are not detected in deep x-ray data and about half of them can be low-luminosity AGN at z similar to 0.5. We also show a strong potential of optical variability as a tracer of high-z low-luminosity faint quasars.
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页码:417 / +
页数:2
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