Hisanori Furusawa spends much of her time researching Astrophysics, Astronomy, Redshift, Galaxy and Hubble Deep Field. Her study in Reionization, Galaxy formation and evolution, Luminosity, Star formation and COSMIC cancer database is done as part of Astrophysics. Her Luminosity research is multidisciplinary, relying on both Line, Cosmic variance and Dark matter halo.
The Redshift study combines topics in areas such as X-shaped radio galaxy, Light curve, Supernova and Sky. Her biological study spans a wide range of topics, including Spectral line and Spectroscopy. Her study explores the link between Hubble Deep Field and topics such as Equivalent width that cross with problems in Photon and Amplitude.
Astrophysics, Galaxy, Astronomy, Redshift and Luminosity are her primary areas of study. Her study in Hubble Deep Field, Reionization, Star formation, Stars and Sky are all subfields of Astrophysics. Her Hubble Deep Field study integrates concerns from other disciplines, such as Equivalent width and Halo.
Her research in Stars focuses on subjects like Light curve, which are connected to Brightness. Her research integrates issues of Number density, Spectral line, Spectral energy distribution, Doubly ionized oxygen and Gamma-ray burst in her study of Redshift. In her study, Ram pressure and Virgo Cluster is strongly linked to Emission spectrum, which falls under the umbrella field of Luminosity.
Her scientific interests lie mostly in Astrophysics, Galaxy, Luminosity, Quasar and Astronomy. Her study in Astrophysics focuses on Reionization, Luminosity function, Light curve, Supernova and Sky. Her Galaxy research also works with subjects such as
As a part of the same scientific study, Hisanori Furusawa usually deals with the Luminosity, concentrating on Emission spectrum and frequently concerns with Line and Near-infrared spectroscopy. Her Quasar study also includes
Her primary areas of study are Astrophysics, Subaru Telescope, Astronomy, Sky and Computer graphics. Her research in the fields of Luminosity, Redshift, Kilonova and Neutron star overlaps with other disciplines such as Flux. Her research investigates the connection with Redshift and areas like Star formation which intersect with concerns in Absolute magnitude.
Hisanori Furusawa works mostly in the field of Subaru Telescope, limiting it down to topics relating to Pipeline and, in certain cases, Large Synoptic Survey Telescope, Optical imaging, Codebase, Data management and Data processing, as a part of the same area of interest. Her study on Magnitude, Brightness and Supernova is often connected to Summit and Survey research as part of broader study in Astronomy. Her research in Computer graphics tackles topics such as Field which are related to areas like Interface and Stars.
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.
Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
R. Amanullah;C. Lidman;D. Rubin;G. Aldering.
arXiv: Cosmology and Nongalactic Astrophysics (2010)
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <z< 1.12 AND THE UNION2 COMPILATION ∗
Rahman Amanullah;Chris Lidman;D. Rubin;D. Rubin;G. Aldering.
The Astrophysical Journal (2010)
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)
Subaru Prime Focus Camera — Suprime-Cam
Satoshi Miyazaki;Yutaka Komiyama;Maki Sekiguchi;Sadanori Okamura.
Publications of the Astronomical Society of Japan (2002)
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)
The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
H. Aihara;N. Arimoto;R. Armstrong;S. Arnouts.
arXiv: Instrumentation and Methods for Astrophysics (2017)
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)
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)
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