The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Astrophysics - Astrophysics Of Galaxies
| 45
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 11
|
| Galaxies: Evolution
| 9
|
| Methods: Numerical
| 8
|
| Circumgalactic Medium
| 8
|
| Magnetohydrodynamics [S]
| 6
|
| Physics - Fluid Dynamics
| 6
|
| Hydrodynamics
| 5
|
| Physics - Plasma Physics [H]
| 5
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 5
|
| Stars: Abundances
| 5
|
| Hydrodynamical Simulations
| 5
|
| Cosmology: Theory
| 4
|
| Galaxies: Clusters: Intracluster Medium
| 4
|
| Galaxies: ISM
| 4
|
| Galaxies: Formation
| 4
|
| Galaxies: High-redshift
| 4
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 4
|
| Galaxies: Star Formation
| 3
|
| Quasars: Absorption Lines
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Active Galactic Nuclei
| 3
|
| Intergalactic Medium
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Stellar Feedback
| 3
|
| Plasma Astrophysics
| 3
|
| Dwarf Galaxies
| 2
|
| Population III Stars
| 2
|
| Primordial Galaxies
| 2
|
| Cooling Flows
| 2
|
| Quasar Absorption Line Spectroscopy
| 2
|
| Stars: Population III
| 2
|
| Galaxies: Active
| 2
|
| Supermassive Black Holes
| 2
|
| Galaxy: Halo
| 2
|
| Magnetic Fields
| 2
|
| CD
| 2
|
| Galaxy: Formation
| 2
|
| Galaxy: Evolution
| 2
|
| Reionization
| 2
|
| Theoretical Techniques
| 2
|
| Galaxies: Dwarf
| 2
|
| Galaxy Clusters
| 2
|
| Galaxies: Elliptical And Lenticular
| 2
|
| Galaxies: Halos
| 2
|
| Turbulence
| 2
|
| Active Galaxies
| 2
|
| Radiative Transfer [S]
| 2
|
| Galaxy Formation
| 2
|
| Galaxy Evolution
| 2
|
| First Stars
| 2
|
| Early Universe
| 2
|
| Dark Ages
| 2
|
| C++
| 1
|
| C
| 1
|
| Brightest Cluster Galaxies
| 1
|
| Binaries: Close
| 1
|
| Astrophysics
| 1
|
| Astrophysical Fluid Dynamics
| 1
|
| And Cluster Computing
| 1
|
| AGN Host Galaxies
| 1
|
| Adaptive Mesh Refinement
| 1
|
| Abundances
| 1
|
| X-rays: Diffuse Background
| 1
|
| X-ray Astronomy
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Photometric
| 1
|
| Surveys
| 1
|
| Stellar Kinematics
| 1
|
| Stellar Dynamics
| 1
|
| Spectroscopy
| 1
|
| Red Sequence Galaxies
| 1
|
| Radio Galaxies
| 1
|
| Quenched Galaxies
| 1
|
| Physics - Computational Physics
| 1
|
| Parallel
| 1
|
| Nucleosynthesis
| 1
|
| Nuclear Reactions
| 1
|
| Milky Way Galaxy
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Analytical
| 1
|
| Metallicity
| 1
|
| Lyman Limit Systems
| 1
|
| ISM: Structure
| 1
|
| ISM: Abundances
| 1
|
| Intracluster Medium
| 1
|
| Instabilities [H]
| 1
|
| High-velocity Clouds
| 1
|
| High-redshift Galaxies
| 1
|
| Gravitational Waves
| 1
|
| Giant Elliptical Galaxies
| 1
|
| Galaxy: Abundances
| 1
|
| Galaxy Stellar Halos
| 1
|
| Galaxy Processes
| 1
|
| Galaxy Groups
| 1
|
| Galaxy Environments
| 1
|
| Galaxy Accretion
| 1
|
| Galaxies: Kinematics And Dynamics
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies: High Redshift
| 1
|
| Galaxies: Clusters: General
| 1
|
| Galaxies
| 1
|
| Fortran
| 1
|
| Forcing
| 1
|
| Extragalactic Astronomy
| 1
|
| Energy Transfer
| 1
|
| Elliptical Galaxies
| 1
|
| Early-type Galaxies
| 1
|
| Damped Lyman-alpha Systems
| 1
|
| Cool Intergalactic Medium
| 1
|
| Computer Science - Performance
| 1
|
| Computer Science - Distributed
| 1
|
| Computational Methods
| 1
|
| Clustering
| 1
|
| X-rays: Galaxies: Clusters
| 1
|