Houjun Mo spends much of his time researching Astrophysics, Astronomy, Galaxy, Halo and Dark matter halo. Dark matter, Galaxy group, Galaxy formation and evolution, Redshift and Luminosity are among the areas of Astrophysics where the researcher is concentrating his efforts. His Dark matter study combines topics in areas such as Halo occupation distribution and Galaxy cluster.
Houjun Mo focuses mostly in the field of Galaxy group, narrowing it down to topics relating to Luminosity function and, in certain cases, Field galaxy. He interconnects Cosmology and Accretion in the investigation of issues within Halo. His Dark matter halo research is multidisciplinary, incorporating elements of Galaxy rotation curve and Cold dark matter.
Houjun Mo mainly investigates Astrophysics, Galaxy, Astronomy, Halo and Dark matter. Galaxy formation and evolution, Redshift, Galaxy group, Dark matter halo and Satellite galaxy are subfields of Astrophysics in which his conducts study. Houjun Mo combines subjects such as Galaxy rotation curve and Velocity dispersion with his study of Dark matter halo.
Galaxy is closely attributed to Sky in his study. The study incorporates disciplines such as Virial theorem, Accretion, Radius and Cold dark matter in addition to Halo. His Dark matter research includes themes of Field, Halo occupation distribution, Baryon, Galaxy cluster and Structure formation.
Houjun Mo mostly deals with Astrophysics, Galaxy, Halo, Redshift and Dark matter. Houjun Mo works mostly in the field of Astrophysics, limiting it down to topics relating to Astronomy and, in certain cases, Content, as a part of the same area of interest. His Galaxy research incorporates elements of Cosmology, Spectral line, Universe and Sky.
Houjun Mo has researched Halo in several fields, including Function and Baryon. The concepts of his Dark matter study are interwoven with issues in Field and Accretion. His studies in Galaxy formation and evolution integrate themes in fields like Stars and Elliptical galaxy.
Astrophysics, Galaxy, Halo, Dark matter and Redshift are his primary areas of study. His Astrophysics study frequently links to other fields, such as Astronomy. In his research, Space and Anisotropy is intimately related to Cosmology, which falls under the overarching field of Galaxy.
His research in Luminosity focuses on subjects like Sky, which are connected to Type. Houjun Mo has included themes like Metallicity and Galaxy formation and evolution in his Elliptical galaxy study. His research in Dark matter halo intersects with topics in Mass-to-light ratio, Luminosity function, Absorption, Quasar and Velocity dispersion.
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Sloan Digital Sky Survey: Early data release
C. Stoughton;R. H. Lupton;M. Bernardi;M. R. Blanton.
web science (2002)
Sloan digital sky survey: Early data release
Chris Stoughton;Robert H. Lupton;Mariangela Bernardi;Michael R. Blanton;Michael R. Blanton.
The Astronomical Journal (2002)
The Formation of Galactic Disks
H. J. Mo;Shude Mao;Simon D. M. White.
arXiv: Astrophysics (1997)
The formation of galactic discs
H. J. Mo;Shude Mao;Simon D. M. White.
Monthly Notices of the Royal Astronomical Society (1998)
Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
Ravi K. Sheth;H. J. Mo;Giuseppe Tormen.
Monthly Notices of the Royal Astronomical Society (2001)
An analytic model for the spatial clustering of dark matter haloes
H.J. Mo;H.J. Mo;Simon D.M. White;Simon D.M. White.
Monthly Notices of the Royal Astronomical Society (1996)
Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
Xiaohu Yang;H.J. Mo;Frank C. van den Bosch;Anna Pasquali.
arXiv: Astrophysics (2007)
The size distribution of galaxies in the Sloan Digital Sky Survey
Shiyin Shen;H. J. Mo;Simon D. M. White;Michael R. Blanton.
Monthly Notices of the Royal Astronomical Society (2003)
Galaxy Formation and Evolution
Houjun Mo;Frank van den Bosch;Simon White.
Galaxy Groups in the SDSS DR4. I. The Catalog and Basic Properties
Xiaohu Yang;H. J. Mo;Frank C. van den Bosch;Anna Pasquali.
The Astrophysical Journal (2007)
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