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
| 43
|
| Stars: Formation
| 33
|
| ISM: Molecules
| 18
|
| ISM: Clouds
| 17
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 15
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 13
|
| Magellanic Clouds
| 13
|
| Radio Continuum: Galaxies
| 13
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 13
|
| RADIO LINES: ISM
| 10
|
| Astrophysics
| 10
|
| Submillimeter
| 9
|
| ISM: Supernova Remnants
| 9
|
| Stars: Protostars
| 8
|
| Site Testing
| 8
|
| ISM: Kinematics And Dynamics
| 7
|
| Dust
| 6
|
| Submillimetre: ISM
| 6
|
| Galaxies: Active
| 6
|
| Extinction
| 6
|
| Surveys
| 6
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 6
|
| Radio Continuum: ISM
| 5
|
| ISM: Structure
| 5
|
| Catalogues
| 4
|
| Techniques: Image Processing
| 4
|
| Telescopes
| 4
|
| Submillimetre: General
| 4
|
| Galaxy: Kinematics And Dynamics
| 4
|
| Galaxy: Structure
| 4
|
| ISM: Jets And Outflows
| 3
|
| Instrumentation: Miscellaneous
| 3
|
| Stars: Low-mass
| 3
|
| Radiative Transfer [S]
| 3
|
| Infrared: General
| 3
|
| Submillimeter: ISM
| 3
|
| H II Regions
| 3
|
| Galaxies: Jets
| 3
|
| Molecular Data
| 3
|
| Galaxies: General
| 3
|
| Galaxies: Evolution
| 3
|
| Galaxies: Distances And Redshifts
| 3
|
| ISM: H II REGIONS
| 3
|
| Radio Continuum: General
| 3
|
| Catalogs
| 3
|
| Atmospheric Effects
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| ISM: Abundances
| 3
|
| Dome A
| 2
|
| Supernovae: General
| 2
|
| Galaxies: Starburst
| 2
|
| INFRARED: ISM: CONTINUUM
| 2
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 2
|
| Contact Binary Stars
| 2
|
| Clouds
| 2
|
| Galaxy Clusters
| 2
|
| X-rays: General
| 2
|
| Instrumentation: Spectrographs
| 2
|
| Galaxy: Center
| 2
|
| Aurora
| 2
|
| Astrochemistry
| 2
|
| High Energy Physics - Experiment
| 2
|
| High Energy Physics - Phenomenology
| 2
|
| Infrared: Galaxies
| 2
|
| Astrophysics - Galaxy Astrophysics
| 2
|
| ISM: Lines And Bands
| 2
|
| Methods: Data Analysis
| 2
|
| Galaxies: Catalogs
| 2
|
| Radio Sources
| 2
|
| Techniques: Photometric
| 2
|
| Molecules
| 2
|
| Sky Brightness
| 2
|
| ISM: Individual Objects: DEM S5
| 1
|
| ISM: Individual (Potoroo)
| 1
|
| ISM: Individual (NGC 7129)
| 1
|
| ISM: GENERAL ISM: CLOUDS
| 1
|
| ISM: Bubbles
| 1
|
| ISM: Atoms
| 1
|
| Instruments
| 1
|
| Instrumentation: Miscellaneous -radio Lines: ISM
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation: Detectors
| 1
|
| Instrumentation
| 1
|
| Infrared: Stars
| 1
|
| Infrared: ISM
| 1
|
| IACT Technique
| 1
|
| Gamma Rays [S]
| 1
|
| Gamma Ray Experiments
| 1
|
| Galaxy: Abundances
| 1
|
| Galaxies: Structure
| 1
|
| Galaxies: NGC 7793
| 1
|
| Galaxies: NGC 55
| 1
|
| Galaxies: NGC 300
| 1
|
| Galaxies: ISM
| 1
|
| Galaxies: Individual: QSO J0443.8-6141
| 1
|
| Galaxies: Individual: LMC
| 1
|
| Galaxies: High-redshift
| 1
|
| Galaxies: Compact
| 1
|
| Galaxies: Clusters: General
| 1
|
| Evolution
| 1
|
| Event-based Camera (EBC)
| 1
|
| Electrical Engineering And Systems Science - Signal Processing
| 1
|
| Electrical Engineering And Systems Science - Image And Video Processing
| 1
|
| DEM S23
| 1
|
| Dark Matter Theory
| 1
|
| Dark Matter Experiments
| 1
|
| Cosmology: Observations
| 1
|
| Cosmic Rays
| 1
|
| Cherenkov Telescopes
| 1
|
| Binaries: Eclipsing
| 1
|
| Astronomy
| 1
|
| (ISM:) HII Regions
| 1
|
| X-rays: Individual (CXOU J163802.6-471358)
| 1
|
| X-ray Astronomy
| 1
|
| Winterover Scientists
| 1
|
| Turbulence
| 1
|
| Transient Detection
| 1
|
| THE LAGOON NEBULA
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Interferometric
| 1
|
| Techniques: Spectroscopic
| 1
|
| Sunyaev-Zeldovich Effect
| 1
|
| Submillimetre
| 1
|
| Submillimeter: Galaxies
| 1
|
| Stellar Mergers
| 1
|
| Stars: Winds
| 1
|
| Stars: Pre-main-sequence
| 1
|
| Stars: Pre-main Sequence
| 1
|
| Stars: Pre-main
| 1
|
| Stars: Mass-loss
| 1
|
| Stars: Low Mass
| 1
|
| Stars: Evolution
| 1
|
| Spiral
| 1
|
| Space Vehicles: Instruments
| 1
|
| Space Situational Awareness (SSA)
| 1
|
| Space Imaging
| 1
|
| Solar Neighbourhood
| 1
|
| Sky Transparency
| 1
|
| Sequence Stars:protostars
| 1
|
| Scattering
| 1
|
| Radio Sources: Lines
| 1
|
| Radio Continuum
| 1
|
| Radio Active Galactic Nuclei
| 1
|
| Radiation Mechanisms: General
| 1
|
| Radiation Mechanism: Non-thermal Radio Continuum: ISM
| 1
|
| Pulsars: Individual (PSR J1638-4713)
| 1
|
| Pulsars: General
| 1
|
| Photometry
| 1
|
| Outflows
| 1
|
| Orbital Elements
| 1
|
| Open Clusters And Associations: General
| 1
|
| Neuromorphic
| 1
|
| Monte Carlo Simulations
| 1
|
| Molecular Processes
| 1
|
| MOLECULAR CLOUDS
| 1
|
| Methods: Statistical
| 1
|
| M8
| 1
|
| Low Mass Stars
| 1
|
| ISO
| 1
|
| ISM: Reflection Nebulae
| 1
|
| ISM: Individual: Taurus
| 1
|
| ISM: Individual: Name: Orion B
| 1
|
| ISM: Individual: Name: Carina Nebula
| 1
|
| ISM: Individual: Messier Number: M8
| 1
|
| ISM: Individual: Lupus
| 1
|
| ISM: Individual Objects: ρ Oph A
| 1
|
| ISM: Individual Objects: W3
| 1
|
| ISM: Individual Objects: SNR J0530
| 1
|
| ISM: Individual Objects: SNR J0453-6829
| 1
|
| ISM: Individual Objects: Sgr A
| 1
|
| ISM: Individual Objects: SBN70
| 1
|
| ISM: Individual Objects: Sagittarius B2
| 1
|
| ISM: Individual Objects: RX J0046.5‑7308
| 1
|
| ISM: Individual Objects: Rho Oph A
| 1
|
| ISM: Individual Objects: Orion KL
| 1
|
| ISM: Individual Objects: Orion A
| 1
|
| ISM: Individual Objects: N 103B
| 1
|
| ISM: INDIVIDUAL OBJECTS: M8
| 1
|
| ISM: Individual Objects: Lupus V And VI
| 1
|
| ISM: Individual Objects: L1689
| 1
|
| ISM: Individual Objects: L1688
| 1
|
| ISM: Individual Objects: G308.3-1.4
| 1
|
| ISM: INDIVIDUAL OBJECTS: EAGLE NEBULA
| 1
|
| Astrobiology
| 1
|
| Airglow
| 1
|
| Active Galactic Nuclei
| 1
|
| Abundances
| 1
|
| X-rays: ISM
| 1
|