Masayuki Akiyama
Publications by Year
Research Areas
Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Astrophysical Phenomena and Observations, Adaptive optics and wavefront sensing, Stellar, planetary, and galactic studies
Most-Cited Works
- → Cosmological Evolution of the Hard X‐Ray Active Galactic Nucleus Luminosity Function and the Origin of the Hard X‐Ray Background(2003)1,049 cited
- → STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS(2010)650 cited
- → TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS(2014)630 cited
- → The Subaru/XMM‐NewtonDeep Survey (SXDS). IV. Evolution of Lyα Emitters from \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 $z=3.1$ \end{document} to 5.7 in the 1 deg2Field: Luminosity Functions and AGN(2008)567 cited
- → THE COSMIC BPT DIAGRAM: CONFRONTING THEORY WITH OBSERVATIONS(2013)269 cited
- → The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6(2005)250 cited
- → The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions atz∼ 1.4(2016)241 cited
- → The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6(2005)222 cited
- → A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys(2013)206 cited
- → The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field,(2003)189 cited