Nobunari Kashikawa - Concepedia

Author

Nobunari Kashikawa

National Astronomical Observatory of Japan ORCID

Also Known As

Fujimoto, Seiji, Glazebrook, Karl, Habouzit, Melanie, K. Kashikawa, Kashikawa, N, Kashikawa, N., Kashikawa, Nobunari, N Kashikawa, N. Kashikawa, NOBUNARI KASHIKAWA

368

Publications

15.4K

Citations

H-Index

Concepts

All Affiliations

National Astronomical Observatory of Japan The University of Tokyo The Graduate University for Advanced Studies, SOKENDAI Kyoto University Tohoku University

About

Nobunari Kashikawa is an author at National Astronomical Observatory of Japan specializing in photometry, engineering, and physics.

Top Concepts

#	Concept	H-Index	Publications	Citations
1	Engineering	25	35	3.8K
2	Natural Sciences	7	7	1.2K
3	Applied Physics	2	2	33
4	Education	1	1	18
5	Computer Engineering	1	1	18

Nobunari Kashikawa

143

Publications

14.5K

Citations

H-Index

Page 1

	Year	Citations
THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE<i>z</i>> 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE N. Suzuki, D. Rubin, C. Lidman, The Astrophysical Journal	2012	1.7K
SPECTRA AND<i>HUBBLE SPACE TELESCOPE</i>LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <<i>z</i>< 1.12 AND THE UNION2 COMPILATION R. Amanullah, C. Lidman, D. Rubin, The Astrophysical Journal	2010	1.3K
STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS Masami Ouchi, Kazuhiro Shimasaku, Hisanori Furusawa, The Astrophysical Journal	2010	645
The Subaru/<i>XMM‐Newton</i>Deep 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 deg<sup>2</sup>Field: Luminosity Functions and AGN Masami Ouchi, Kazuhiro Shimasaku, Masayuki Akiyama, The Astrophysical Journal Supplement Series	2008	562
Subaru Deep Survey. V. A Census of Lyman Break Galaxies at<i>z</i> ≃ 4 and 5 in the Subaru Deep Fields: Photometric Properties Masami Ouchi, Kazuhiro Shimasaku, Sadanori Okamura, The Astrophysical Journal	2004	420
The End of the Reionization Epoch Probed by Lyα Emitters at<i>z</i>= 6.5 in the Subaru Deep Field Nobunari Kashikawa, Kazuhiro Shimasaku, Matthew A. Malkan, The Astrophysical Journal EngineeringSubaru Deep FieldCosmologyReionization Epoch ProbedLarge Scale Structure	2006	395
FOCAS: The Faint Object Camera and Spectrograph for the Subaru Telescope Nobunari Kashikawa, Kentaro Aoki, Ryo Asai, Publications of the Astronomical Society of Japan EngineeringSpace OpticSatellite InstrumentationSubaru TelescopeAstronomical Image Analysis	2002	322
A galaxy at a redshift z = 6.96 Masanori Iye, Kazuaki Ota, Nobunari Kashikawa, Nature Galaxy FormationPhotometryEngineeringRedshift ZLarge Scale Structure	2006	290
Lyα Emitters at <i>z</i> = 5.7 in the Subaru Deep Field Kazuhiro Shimasaku, Nobunari Kashikawa, Mamoru Doi, Publications of the Astronomical Society of Japan Galaxy FormationPhotometryLyα EmittersEngineeringPhysics	2006	285
The Type I[CLC]c[/CLC] Hypernova SN 2002[CLC]ap[/CLC] P. A. Mazzali, J. Deng, Keiichi Maeda, The Astrophysical Journal	2002	284

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