FIVE NEW HIGH-REDSHIFT QUASAR LENSES FROM THE SLOAN DIGITAL SKY SURVEY

被引:34
作者
Inada, Naohisa [1 ]
Oguri, Masamune [2 ]
Shin, Min-Su [3 ]
Kayo, Issha [4 ,5 ]
Strauss, Michael A. [3 ]
Morokuma, Tomoki [6 ]
Schneider, Donald P. [7 ]
Becker, Robert H. [8 ,9 ]
Bahcall, Neta A. [3 ]
York, Donald G. [10 ,11 ]
机构
[1] RIKEN, Cosm Radiat Lab, Wako, Saitama 3510198, Japan
[2] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA
[3] Princeton Univ Observ, Princeton, NJ 08544 USA
[4] Nagoya Univ, Dept Phys & Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[5] Univ Tokyo, Inst Phys & Math Universe, Chiba 2778582, Japan
[6] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan
[7] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[8] IGPP LLNL, Livermore, CA 94550 USA
[9] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[10] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[11] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
gravitational lensing; quasars: individual (SDSS J081959.79+535624.3; SDSS J125418.95+223536.5; SDSS J125819.24+165717.6; SDSS J133907.13+131039.6; SDSS J140012.77+313454.1); SPECTROSCOPIC TARGET SELECTION; 3RD DATA RELEASE; 5TH DATA RELEASE; GRAVITATIONAL LENS; CANDIDATE SELECTION; GALAXY STRUCTURE; SAMPLE; SEARCH; CONSTRAINTS; DISCOVERY;
D O I
10.1088/0004-6256/137/5/4118
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of five gravitationally lensed quasars from the Sloan Digital Sky Survey (SDSS). All five systems are selected as two-image lensed quasar candidates from a sample of high-redshift (z > 2.2) SDSS quasars. We confirmed their lensing nature with additional imaging and spectroscopic observations. The new systems are SDSS J0819+5356 (source redshift z(s) = 2.237, lens redshift z(l) = 0.294, and image separation theta = 4 ''.04), SDSS J1254+2235 (z(s) = 3.626, theta = 1 ''.56), SDSS J1258+1657 (z(s) = 2.702, theta = 1 ''.28), SDSS J1339+1310 (z(s) = 2.243, theta = 1 ''.69), and SDSS J1400+3134 (z(s) = 3.317, theta = 1 ''.74). We estimate the lens redshifts of the latter four systems to be z(l) = 0.2-0.8 from the colors and magnitudes of the lensing galaxies. We find that the image configurations of all systems are well reproduced by standard mass models. Although these lenses will not be included in our statistical sample of z(s) < 2.2 lenses, they expand the number of lensed quasars which can be used for high-redshift galaxy and quasar studies.
引用
收藏
页码:4118 / 4126
页数:9
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