The scientist’s investigation covers issues in Astrophysics, Galaxy, Astronomy, Redshift and Luminosity. Astrophysics and Flux are two areas of study in which Yuichi Matsuda engages in interdisciplinary research. In his research, Dark matter is intimately related to Equivalent width, which falls under the overarching field of Galaxy.
When carried out as part of a general Astronomy research project, his work on Galaxy formation and evolution, Cosmology, Galaxy merger and Lenticular galaxy is frequently linked to work in Field, therefore connecting diverse disciplines of study. His Redshift study also includes
His main research concerns Astrophysics, Galaxy, Astronomy, Redshift and Star formation. His research in Submillimeter Array, Luminosity, Galaxy formation and evolution, Hubble Deep Field and Millimeter are components of Astrophysics. His Galaxy research is multidisciplinary, incorporating perspectives in Stars and Emission spectrum.
His Redshift research incorporates elements of Spectral energy distribution, Subaru Telescope, Initial mass function and Sky. His work carried out in the field of Star formation brings together such families of science as Accretion and Universe. His research investigates the connection with Reionization and areas like Continuum which intersect with concerns in Interstellar medium.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Star formation and Submillimeter Array. His Continuum, Nebula, Galaxy formation and evolution, Reionization and Luminosity study are his primary interests in Astrophysics. His research in Galaxy intersects with topics in Stars and Doubly ionized oxygen, Emission spectrum.
His Redshift study contributes to a more complete understanding of Astronomy. His Star formation research is multidisciplinary, relying on both Milky Way, Line-of-sight and Supercluster. His studies examine the connections between Submillimeter Array and genetics, as well as such issues in Millimeter, with regards to Hubble Deep Field, Spatially resolved and Supernova.
Yuichi Matsuda mainly focuses on Astrophysics, Galaxy, Redshift, Star formation and Primary aldosteronism. His study in Galaxy formation and evolution, Submillimeter Array, Continuum, Nebula and Cosmic web falls within the category of Astrophysics. His Galaxy study incorporates themes from Doubly ionized oxygen and Emission spectrum.
His Redshift study introduces a deeper knowledge of Astronomy. In his study, Hubble Deep Field and Initial mass function is strongly linked to Universe, which falls under the umbrella field of Star formation. Within one scientific family, Yuichi Matsuda focuses on topics pertaining to Retrospective cohort study under Primary aldosteronism, and may sometimes address concerns connected to Diabetes mellitus, Renal function, Adrenalectomy and Hypokalemia.
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 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)
A galaxy at a redshift z = 6.96
Masanori Iye;Masanori Iye;Kazuaki Ota;Nobunari Kashikawa;Hisanori Furusawa.
Nature (2006)
Lyα Emitters at z = 5.7 in the Subaru Deep Field
Kazuhiro Shimasaku;Nobunari Kashikawa;Mamoru Doi;Chun Ly.
Publications of the Astronomical Society of Japan (2006)
A Subaru Search for Lyα Blobs in and around the Protocluster Region At Redshift z = 3.1
Yuichi Matsuda;Toru Yamada;Tomoki Hayashino;Hajime Tamura.
The Astronomical Journal (2004)
A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS
David Sobral;Ian Smail;Philip N. Best;James E. Geach.
Monthly Notices of the Royal Astronomical Society (2013)
Completing the Census of Ly-alpha Emitters at the Reionization Epoch
Nobunari Kashikawa;Kazuhiro Shimasaku;Yuichi Matsuda;Eiichi Egami.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6
Yoshiaki Taniguchi;Masaru Ajiki;Tohru Nagao;Tohru Nagao;Yasuhiro Shioya.
Publications of the Astronomical Society of Japan (2005)
Subaru Deep Survey. II. Luminosity Functions and Clustering Properties of Lyα Emitters at z = 4.86 in the Subaru Deep Field*
Masami Ouchi;Kazuhiro Shimasaku;Hisanori Furusawa;Masayuki Miyazaki.
The Astrophysical Journal (2003)
Star formation at z=1.47 from HiZELS: An H{lpha}+[OII] double-blind study
David Sobral;Philip Best;Yuichi Matsuda;Ian Smail.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
The Reionization and Galaxy Evolution Probed by z=7 Lyman Alpha Emitters
Kazuaki Ota;Masanori Iye;Nobunari Kashikawa;Kazuhiro Shimasaku.
arXiv: Astrophysics (2007)
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