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 - High Energy Astrophysical Phenomena [S]
| 45
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 15
|
| X-rays: ISM
| 14
|
| Astrophysics - Astrophysics Of Galaxies
| 14
|
| ISM: Supernova Remnants
| 10
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| X-ray Astronomy
| 8
|
| X-rays: Galaxies: Clusters
| 6
|
| X-rays: General
| 6
|
| Atomic Data
| 6
|
| Shock Waves
| 5
|
| Plasma Astrophysics
| 4
|
| Line: Identification
| 4
|
| High Energy Physics - Phenomenology
| 4
|
| Extinction
| 4
|
| Dark Matter
| 4
|
| Stars: Mass-loss
| 4
|
| Dust
| 4
|
| Hydrodynamics
| 4
|
| X-rays: Diffuse Background
| 3
|
| Circumstellar Matter
| 3
|
| Radio Continuum: General
| 3
|
| Atomic Spectroscopy
| 3
|
| Supernova Remnants
| 3
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 3
|
| Galaxy Clusters
| 3
|
| X-rays: Galaxies
| 3
|
| High Resolution Spectroscopy
| 2
|
| Molecular Clouds
| 2
|
| Supermassive Black Holes
| 2
|
| X-rays: Binaries
| 2
|
| Methods: Numerical
| 2
|
| Radiation Mechanisms: General
| 2
|
| Methods: Data Analysis
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Galaxies: Clusters: Intracluster Medium
| 2
|
| Large-scale Structure Of Universe
| 2
|
| Quasars: Absorption Lines
| 2
|
| Galaxies: Active
| 2
|
| Event Horizons
| 2
|
| Elementary Particles
| 2
|
| EHT
| 2
|
| ISM: Individual Objects: W49B
| 2
|
| Plasmas
| 2
|
| Type Ia Supernovae
| 2
|
| ISM: Bubbles
| 2
|
| ISM: Abundances
| 2
|
| Physics - Atomic Physics
| 2
|
| Black Hole Physics
| 2
|
| Atomic Processes
| 2
|
| Turbulence
| 2
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 2
|
| Scattering
| 2
|
| NgEHT
| 2
|
| Acceleration Of Particles
| 2
|
| ISM: Clouds
| 1
|
| Intergalactic Medium
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Detectors
| 1
|
| Informal Learning; Science Communication: Theory And Models; Visual Communication
| 1
|
| Hubble Constant
| 1
|
| Hot Spot
| 1
|
| High Energy Physics - Theory
| 1
|
| Globular Clusters: Individual: Terzan 2
| 1
|
| Gamma Rays: ISM
| 1
|
| Galaxy: Halo
| 1
|
| Galaxy Distances
| 1
|
| Galaxy Dark Matter Halos
| 1
|
| Galaxies: Starburst
| 1
|
| Galaxies: Seyfert
| 1
|
| Galaxies: Individual: M82
| 1
|
| Galaxies: Individual: A3112
| 1
|
| Galaxies: Elliptical And Lenticular
| 1
|
| Galaxies: Clusters: Individual: Perseus Cluster
| 1
|
| Galaxies: Clusters: Individual: A3112
| 1
|
| Galaxies: Clusters: Individual: A1750
| 1
|
| Galaxies: Clusters: General
| 1
|
| Galaxies
| 1
|
| Elliptical Galaxies
| 1
|
| Dynamical Image Reconstruction
| 1
|
| Distance Indicators
| 1
|
| Diffuse Radiation
| 1
|
| Cosmology: Observations
| 1
|
| Cosmic Rays
| 1
|
| Cosmic EUV
| 1
|
| Computer Science - Human-Computer Interaction
| 1
|
| Circumgalactic Medium
| 1
|
| CD
| 1
|
| Binaries: Eclipsing
| 1
|
| Atomic Physics
| 1
|
| Atomic Data Benchmarking
| 1
|
| Asymptotic Giant Branch Stars
| 1
|
| Astrophysics
| 1
|
| Astroparticle Physics
| 1
|
| X-rays: Individuals: Cygnus X-3
| 1
|
| X-rays: Individual: Cyg X-2
| 1
|
| X-rays: Individual (Crab)
| 1
|
| X-ray Telescopes
| 1
|
| X-ray Spectroscopy
| 1
|
| X-ray Detectors
| 1
|
| White Dwarf Stars
| 1
|
| Warm-hot Intergalactic Medium
| 1
|
| Time-variability
| 1
|
| The Milky Way
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Interferometric
| 1
|
| Supernovae: Individual: SN 2013ej
| 1
|
| Supernovae: Individual: SN 2012aw
| 1
|
| Supernovae: Individual: SN 2011ja
| 1
|
| Supernovae: Individual: SN 2004dj
| 1
|
| Supernovae: General
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Stellar Distance
| 1
|
| Stellar Accretion
| 1
|
| StarWarps
| 1
|
| Starburst Galaxies
| 1
|
| Spectrometers
| 1
|
| Abundances
| 1
|
| Sgr A*
| 1
|
| Science And Media; Public Perception Of Science And Technology; Representations Of Science And Technology
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Quasars: Individual: PG 1211+143
| 1
|
| Quasars: Individual: H 1821+643
| 1
|
| Publicly Available Software
| 1
|
| Protoplanetary Disks
| 1
|
| Proper Motions
| 1
|
| Polarization
| 1
|
| Plasma Composition
| 1
|
| Physics - Physics Education
| 1
|
| Observational Cosmology
| 1
|
| Nucleosynthesis
| 1
|
| Nuclear Reactions
| 1
|
| Nonthermal Radiation Sources
| 1
|
| Neutrinos
| 1
|
| Mira Variable Stars
| 1
|
| Methods: Statistical
| 1
|
| Methods: Laboratory: Atomic
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| M87*
| 1
|
| Large Magellanic Cloud
| 1
|
| Laboratory Astrophysics
| 1
|
| ISM: Structure
| 1
|
| ISM: Molecules
| 1
|
| ISM: Individual Objects: W49B: G43.3-0.2
| 1
|
| ISM: Individual Objects: SN 1572 Tycho's SNR
| 1
|
| ISM: Individual Objects: RCW 86
| 1
|
| ISM: Individual Objects: G290.1-0.8
| 1
|
| Solar Wind [H]
| 1
|