Takamitsu Miyaji
0000-0002-7562-485X
88 papers found
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The hard X-ray luminosity function from ASCA surveys
XMM-Newton view of the Hubble Deep Field-North and Groth-Westphal strip regions
The Chandra Deep Field North Survey. IX. Extended X-Ray Sources
Faint-Source Counts from Off-Source Fluctuation Analysis on [ITAL]Chandra[/ITAL] Observations of the Hubble Deep Field–North
XMM-Newton observation of a distant X-ray selected cluster of galaxies at $\vec{z}=\mathsf{1.26}$ with possible cluster interaction
Multiple Components of the Luminous Compact X-Ray Source at the Edge of Holmberg II Observed by [ITAL]ASCA[/ITAL] and [ITAL]ROSAT[/ITAL]
Soft X-ray AGN luminosity function from ROSAT surveys: II. Table of the binned soft X-ray luminosity function
XMM-Newton observation of the Lockman Hole: I. The X-ray data
Evolution of AGNs and a model of the X-ray back-ground
Soft X-ray AGN luminosity function from it ROSAT surveys. I. Cosmological evolution and contribution to the soft X-ray background
A Rich Cluster of Galaxies near the Quasar B2 1335+28 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 $z=1.1$ \end{document} : Color Distribution and Star Formation Properties
On the relationship between galaxy formation and quasar evolution
The large scale structure of the soft X-ray background. III. Cosmological implications
Origin of the Galactic ridge X-ray emission
The cosmic X-ray background spectrum observed with ROSAT and ASCA
ROSAT HRI observations of Selected Area 57
The cosmic X-ray background spectrum: an ASCA-ROSAT joint analysis
Sky surveys withASCA — Deep Sky Survey
The cross-correlation of faint QSOs with the cosmic X-ray background
Soft X-ray emission and optical multicolors of faint QSOs in the Selected Area 57.
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