TY - JOUR
T1 - Are Two z ∼ 6 Quasars Gravitationally Lensed?
AU - Yamada, Sanae F.
AU - Shioya, Yasuhiro
AU - Taniguchi, Yoshiaki
AU - Murayama, Takashi
AU - Ajiki, Masaru
AU - Nagao, Tohru
AU - Fujita, Shinobu S.
AU - Umeda, Kazuyoshi
AU - Komiyama, Yutaka
AU - Karoji, Hiroshi
AU - Ando, Hiroyasu
AU - Iye, Masanori
AU - Kashikawa, Nobunari
AU - Kodaira, Keiichi
PY - 2003
Y1 - 2003
N2 - Several high-z (z > 5.7) quasars have been found during the course of Sloan Digital Sky Survey. The presence of such very high-z quasars is expected to put constraints on early structure formation. On one hand, it is suggested that these most luminous objects at high redshift are biased toward highly magnified objects by gravitational lensing. To clarify the effect of gravitational lensing on high-z quasars, we began an imaging survey of intervening lensing galaxies. Indeed, our previous optical image showed that SDSSp J104433.04+012502.2 at z = 5.74 is gravitationally magnified by a factor of 2. In this paper, we report our new optical imaging of two other high-z quasars, SDSSp J103027.10+052455.0 at z = 6.28 and SDSSp J130608.26+035626.3 at z = 5.99. Since we found neither an intervening galaxy nor a counter image with i′ < 25.4-25.8 around each quasar, we conclude that they are not strongly magnified regardless that a lens galaxy is dusty.
AB - Several high-z (z > 5.7) quasars have been found during the course of Sloan Digital Sky Survey. The presence of such very high-z quasars is expected to put constraints on early structure formation. On one hand, it is suggested that these most luminous objects at high redshift are biased toward highly magnified objects by gravitational lensing. To clarify the effect of gravitational lensing on high-z quasars, we began an imaging survey of intervening lensing galaxies. Indeed, our previous optical image showed that SDSSp J104433.04+012502.2 at z = 5.74 is gravitationally magnified by a factor of 2. In this paper, we report our new optical imaging of two other high-z quasars, SDSSp J103027.10+052455.0 at z = 6.28 and SDSSp J130608.26+035626.3 at z = 5.99. Since we found neither an intervening galaxy nor a counter image with i′ < 25.4-25.8 around each quasar, we conclude that they are not strongly magnified regardless that a lens galaxy is dusty.
KW - Galaxies: high-redshift
KW - Galaxies: quasars: individual (SDSSp J103027.10+052455.0, SDSSp J130608.26+035626.3)
KW - Gravitational lensing
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U2 - 10.1093/pasj/55.4.733
DO - 10.1093/pasj/55.4.733
M3 - Article
AN - SCOPUS:0242330232
SN - 0004-6264
VL - 55
SP - 733
EP - 738
JO - Publication of the Astronomical Society of Japan
JF - Publication of the Astronomical Society of Japan
IS - 4
ER -