Nobunari Kashikawa mostly deals with Astrophysics, Galaxy, Astronomy, Redshift and Luminosity. His work in Astrophysics is not limited to one particular discipline; it also encompasses Spectroscopy. In his work, Computer graphics and Image quality is strongly intertwined with Stars, which is a subfield of Galaxy.
His work carried out in the field of Redshift brings together such families of science as Sky, COSMIC cancer database, Spectral line, Emission spectrum and Photometry. His work on Luminosity function as part of general Luminosity research is frequently linked to Flux, bridging the gap between disciplines. Nobunari Kashikawa has researched Hubble Deep Field in several fields, including Optical imaging and Cosmology.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Astronomy and Quasar. His study in Luminosity, Hubble Deep Field, Star formation, Reionization and Galaxy formation and evolution is carried out as part of his studies in Astrophysics. His Luminosity research incorporates themes from Line and Extinction.
His Galaxy study combines topics from a wide range of disciplines, such as Stars, Spectroscopy and Emission spectrum. The Redshift study combines topics in areas such as Equivalent width, Sky, Supernova, Active galactic nucleus and Spectral line. His research integrates issues of Supermassive black hole, Black hole and Sigma in his study of Quasar.
His primary areas of investigation include Astrophysics, Galaxy, Quasar, Luminosity and Redshift. His Reionization, Star formation, COSMIC cancer database, Luminosity function and Intergalactic medium investigations are all subjects of Astrophysics research. Nobunari Kashikawa focuses mostly in the field of Galaxy, narrowing it down to matters related to Equivalent width and, in some cases, Radiative transfer.
Nobunari Kashikawa combines subjects such as Accretion, Supermassive black hole, Black hole and Sigma with his study of Quasar. His Luminosity research integrates issues from Spectral energy distribution, Sky, Line, Absolute magnitude and Universe. His studies in Redshift integrate themes in fields like Stars and Emission spectrum.
Nobunari Kashikawa mainly focuses on Astrophysics, Galaxy, Luminosity, Quasar and Reionization. The Astrophysics study which covers Emission spectrum that intersects with Line. His work on Star formation, Stellar mass and Halo as part of general Galaxy research is often related to Systematic search, thus linking different fields of science.
Nobunari Kashikawa interconnects Doubly ionized oxygen, Cosmology, Active galactic nucleus and Stars in the investigation of issues within Luminosity. His Reionization research is multidisciplinary, incorporating perspectives in COSMIC cancer database and Intergalactic medium. Nobunari Kashikawa has included themes like Galaxy formation and evolution and Sigma in his Redshift study.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample
N. Suzuki;N. Suzuki;D. Rubin;D. Rubin;C. Lidman;G. Aldering.
The Astrophysical Journal (2012)
Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models
Masami Ouchi;Kazuhiro Shimasaku;Hisanori Furusawa;Tomoki Saito.
arXiv: Cosmology and Nongalactic Astrophysics (2010)
The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
Masami Ouchi;Kazuhiro Shimasaku;Masayuki Akiyama;Chris Simpson.
arXiv: Astrophysics (2007)
STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS*
Masami Ouchi;Kazuhiro Shimasaku;Hisanori Furusawa;Tomoki Saito.
The Astrophysical Journal (2010)
The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z = 3.1 to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN*
Masami Ouchi;Kazuhiro Shimasaku;Masayuki Akiyama;Chris Simpson.
Astrophysical Journal Supplement Series (2008)
Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 - 7.213: Demographics of Lyman-Alpha Emission in z ~ 7 Galaxies
Yoshiaki Ono;Masami Ouchi;Bahram Mobasher;Mark Dickinson.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
The End of the Reionization Epoch Probed by Lyα Emitters at z = 6.5 in the Subaru Deep Field* **
Nobunari Kashikawa;Kazuhiro Shimasaku;Matthew A. Malkan;Mamoru Doi.
The Astrophysical Journal (2006)
Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties*
Masami Ouchi;Kazuhiro Shimasaku;Kazuhiro Shimasaku;Sadanori Okamura;Sadanori Okamura;Hisanori Furusawa.
The Astrophysical Journal (2004)
The Hyper Suprime-Cam SSP Survey: Overview and survey design
Hiroaki Aihara;Nobuo Arimoto;Nobuo Arimoto;Robert Armstrong;Stéphane Arnouts.
Publications of the Astronomical Society of Japan (2018)
Large Area Survey for z = 7 Galaxies in SDF and GOODS-N: Implications for Galaxy Formation and Cosmic Reionization
Masami Ouchi;Masami Ouchi;Bahram Mobasher;Kazuhiro Shimasaku;Henry C. Ferguson;Henry C. Ferguson.
The Astrophysical Journal (2009)
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