Optical Identification of theASCALynx Deep Survey: An Association of Quasi‐Stellar Objects and a Supercluster at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=1.3$ \end{document} ?-Reference-Cited by-同舟云学术

Optical Identification of theASCALynx Deep Survey: An Association of Quasi‐Stellar Objects and a Supercluster at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=1.3$ \end{document} ?

Published:2003-11-20 Issue:1 Volume:598 Page:210-215
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Ohta Kouji,Akiyama Masayuki,Ueda Yoshihiro,Yamada Toru,Nakanishi Kouichiro,Dalton Gavin B.,Ogasaka Yasushi,Kii Tsuneo,Hayashida Kiyoshi

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/598/i=1/a=210/pdf

Reference34 articles.

1. A Candidate of a Type 2 Quasi‐stellar Object atz = 0.9: Large X‐Ray Absorption with a Strong Broad Hα Emission Line

2. Optical Identification of the ASCA Medium Sensitivity Survey in the Northern Sky: Nature of Hard X‐Ray–Selected Luminous Active Galactic Nuclei

3. Optical Identification of theASCALarge Sky Survey

4. An abuttable CCD imager for visible and X-ray focal plane arrays

5. ChandraStudy of an Overdensity of X‐Ray Sources around Two Distant (z ∼ 0.5) Clusters

Cited by 5 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Two close large quasar groups of size ∼ 350 Mpc at;Monthly Notices of the Royal Astronomical Society;2011-11-03

2. The luminosity dependence of the type 1 active galactic nucleus fraction;Monthly Notices of the Royal Astronomical Society;2005-06-21

3. The discovery of a type II quasar at = 1.65 with integral-field spectroscopy;Monthly Notices of the Royal Astronomical Society: Letters;2005-03-01

4. X-ray source overdensities in Chandra distant cluster fields: A new probe to map the cosmic tapestry?;Astronomy & Astrophysics;2005-01

5. Detection of 20–30 h$\mathsf{^{-1}}$ Mpc-scale galaxy structures embedded in 100 h$\mathsf{^{-1}}$ Mpc-scale structures of quasars and MgII absorbers at $\textit{z}\simeq\mathsf{0.8}$ and $\textit{z} \simeq\mathsf{1.2}$;Astronomy & Astrophysics;2004-06-11