What is he best known for?
The fields of study he is best known for:
- Galaxy
- Astronomy
- Astrophysics
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Astronomy and Reionization.
His Astrophysics research incorporates themes from Spectroscopy and Equivalent width.
His Galaxy research includes elements of Cosmology and Emission spectrum.
His Redshift study also includes
- Quasar which is related to area like Photometry,
- Interstellar medium most often made with reference to Extinction.
His Reionization research is multidisciplinary, incorporating perspectives in Cosmic variance, Luminosity function, Nebula and Photon.
Masami Ouchi has included themes like Line and Optical depth in his Luminosity study.
His most cited work include:
- STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS* (596 citations)
- Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models (585 citations)
- 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 (571 citations)
What are the main themes of his work throughout his whole career to date?
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Astronomy and Reionization.
His work in Luminosity, Star formation, Halo, Galaxy formation and evolution and Quasar is related to Astrophysics.
His research investigates the connection between Luminosity and topics such as Sky that intersect with issues in Magnitude.
The various areas that Masami Ouchi examines in his Galaxy study include Stars and Equivalent width, Emission spectrum.
His research integrates issues of Spectroscopy, Active galactic nucleus, Spectral line, Photometry and Luminous infrared galaxy in his study of Redshift.
His Reionization study combines topics in areas such as COSMIC cancer database, Galaxy cluster and Photon.
He most often published in these fields:
- Astrophysics (135.74%)
- Galaxy (110.46%)
- Redshift (65.40%)
What were the highlights of his more recent work (between 2018-2021)?
- Astrophysics (135.74%)
- Galaxy (110.46%)
- Redshift (65.40%)
In recent papers he was focusing on the following fields of study:
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Reionization and Star formation.
As part of one scientific family, Masami Ouchi deals mainly with the area of Astrophysics, narrowing it down to issues related to the Emission spectrum, and often Line.
His Galaxy study combines topics from a wide range of disciplines, such as Stars and Nebula.
His work in Redshift tackles topics such as Millimeter which are related to areas like Submillimeter Array.
His Reionization research incorporates elements of COSMIC cancer database, Planck, Billion years and Luminosity function.
His work carried out in the field of Star formation brings together such families of science as Supernova and Galaxy cluster.
Between 2018 and 2021, his most popular works were:
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program (212 citations)
- Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O iii] 88 μm, [C ii] 158 μm, and dust continuum with ALMA (79 citations)
- Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O iii] 88 μm, [C ii] 158 μm, and dust continuum with ALMA (79 citations)
In his most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Astrophysics
His scientific interests lie mostly in Astrophysics, Galaxy, Redshift, Star formation and Halo.
His Astrophysics study frequently links to other fields, such as Spectral line.
He is involved in the study of Galaxy that focuses on Galaxy formation and evolution in particular.
His work in Redshift is not limited to one particular discipline; it also encompasses Telescope.
His study in Luminosity is interdisciplinary in nature, drawing from both Absolute magnitude and Stars.
His biological study spans a wide range of topics, including Lyman-break galaxy, Stellar mass and Nebula.
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