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
| 172
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 89
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 73
|
| ISM: Clouds
| 63
|
| ISM: Molecules
| 55
|
| Stars: Formation
| 55
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 32
|
| Interstellar Medium
| 28
|
| Star Formation
| 22
|
| Astrochemistry
| 19
|
| ISM: Abundances
| 19
|
| Radio Pulsars
| 18
|
| ISM: Structure
| 17
|
| Pulsars: General
| 16
|
| ISM: Kinematics And Dynamics
| 16
|
| Pulsars
| 16
|
| Radio Lines: ISM
| 16
|
| Radio Transient Sources
| 15
|
| Molecular Clouds
| 15
|
| Astrophysics
| 13
|
| Radio Bursts
| 13
|
| ISM: Jets And Outflows
| 13
|
| Interstellar Magnetic Fields
| 12
|
| Extinction
| 12
|
| Methods: Data Analysis
| 12
|
| Interstellar Molecules
| 12
|
| Stars: Neutron
| 12
|
| Surveys
| 12
|
| Millisecond Pulsars
| 11
|
| Polarization
| 10
|
| Methods: Statistical
| 9
|
| Star Forming Regions
| 9
|
| ISM: Atoms
| 9
|
| Interstellar Filaments
| 8
|
| Neutron Stars
| 8
|
| Methods: Numerical
| 8
|
| Dust
| 8
|
| Submillimeter: ISM
| 8
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 8
|
| Magnetic Fields
| 7
|
| Globular Star Clusters
| 7
|
| H II Regions
| 6
|
| Polarimetry
| 6
|
| ISM: Individual Objects: Taurus
| 6
|
| Radio Astronomy
| 6
|
| Evolution
| 6
|
| Pulsar
| 6
|
| Galaxies: ISM
| 6
|
| Radio Lines: Galaxies
| 6
|
| Interstellar Atomic Gas
| 5
|
| Interstellar Clouds
| 5
|
| Turbulence
| 5
|
| Star-forming Regions
| 5
|
| Binaries: General
| 5
|
| Binary Pulsars
| 5
|
| ISM: Individual Objects: Orion
| 5
|
| Collapsing Clouds
| 5
|
| Magnetars
| 5
|
| Submillimeter Astronomy
| 5
|
| FAST
| 5
|
| Radio Continuum: ISM
| 5
|
| Interstellar Absorption
| 5
|
| High Energy Physics - Phenomenology
| 5
|
| Telescopes
| 5
|
| Molecular Processes
| 4
|
| Submillimetre: ISM
| 4
|
| Gravitational Waves
| 4
|
| Stars: Protostars
| 4
|
| Galaxy Evolution
| 4
|
| ISM: Magnetic Fields
| 4
|
| Fast Radio Bursts
| 4
|
| Eclipsing Binary Stars
| 4
|
| Stars: Magnetars
| 4
|
| Dense Interstellar Clouds
| 4
|
| Chemical Abundances
| 4
|
| Astronomy Data Analysis
| 4
|
| ISM: Evolution
| 4
|
| Radio Continuum: Galaxies
| 4
|
| Submillimeter
| 3
|
| Protoclusters
| 3
|
| Stars: Low-mass
| 3
|
| ISM: Lines And Bands
| 3
|
| ISM: Globules
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Protostars
| 3
|
| Dust Continuum Emission
| 3
|
| Galaxy Quenching
| 3
|
| Galaxies: Star Formation
| 3
|
| Stars: Kinematics And Dynamics
| 3
|
| (stars:) Pulsars: General
| 3
|
| Stellar Jets
| 3
|
| Galaxies: Evolution
| 3
|
| Interstellar Dynamics
| 3
|
| Galaxies: Starburst
| 3
|
| ISM: Individual Objects: Orion A North
| 2
|
| Gamma-ray Sources
| 2
|
| Observational Astronomy
| 2
|
| Catalogues
| 2
|
| ISM: Individual Objects: Ophiuchus
| 2
|
| Brown Dwarfs
| 2
|
| Magnetospheric Radio Emissions
| 2
|
| General Relativity And Quantum Cosmology
| 2
|
| Giant Molecular Clouds
| 2
|
| Masers
| 2
|
| Scattering
| 2
|
| Techniques: Image Processing
| 2
|
| Massive Stars
| 2
|
| X-rays: Binaries
| 2
|
| Quasars: Absorption Lines
| 2
|
| Stars
| 2
|
| Radiative Transfer [S]
| 2
|
| Techniques: Spectroscopic
| 2
|
| Infrared Dark Clouds
| 2
|
| Radio Continuum Emission
| 2
|
| ASTRONOMY; PHYSICS
| 2
|
| Radio Telescopes And Instrumentation
| 2
|
| ISM: Individual (Taurus)
| 2
|
| Astronomical Object Identification
| 2
|
| Stellar Feedback
| 2
|
| (ISM:) Dust
| 2
|
| Astrobiology
| 2
|
| Radio Telescope
| 2
|
| Radio Continuum: General
| 2
|
| Survey
| 2
|
| ISM: Dust
| 2
|
| Instrumentation: Miscellaneous
| 2
|
| Galaxies: Dwarf
| 2
|
| Galaxies: Active
| 2
|
| Transients: Fast Radio Bursts
| 2
|
| Stellar Winds
| 2
|
| Galaxies: General
| 2
|
| Galaxies: Interactions
| 2
|
| Line: Identification
| 2
|
| Exoplanets
| 2
|
| ISM: Bubbles
| 2
|
| Line: Profiles
| 2
|
| Stars: Magnetic Field
| 2
|
| Galaxy Formation
| 2
|
| Pulsar Timing Method
| 2
|
| Interstellar Line Emission
| 2
|
| Accretion
| 2
|
| Dark Interstellar Clouds
| 2
|
| Low Mass Stars
| 2
|
| Search For Extraterrestrial Intelligence
| 2
|
| Magellanic Clouds
| 2
|
| ISM: Individual Objects: Orion KL
| 2
|
| Gamma-ray Burst: General
| 2
|
| Radio Continuum: Transients
| 2
|
| Pulsar Simulation
| 2
|
| Interstellar Abundances
| 1
|
| Intergalactic Medium
| 1
|
| Intercloud Medium
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation: Detectors
| 1
|
| Infrared: Stars
| 1
|
| Infrared: ISM
| 1
|
| Infrared: Galaxies
| 1
|
| Individual
| 1
|
| Imaging
| 1
|
| I.6.1
| 1
|
| Hydroxyl Sources
| 1
|
| Hydrodynamics
| 1
|
| HII Regions
| 1
|
| High Energy Physics - Theory
| 1
|
| HI Regions And 21-cm Lines
| 1
|
| HI 21cm Line
| 1
|
| H I Line Emission
| 1
|
| Gravitational-wave Cosmology
| 1
|
| Gravitational-wave Astronomy
| 1
|
| Gravitational Wave
| 1
|
| Gravitational Collapse
| 1
|
| Gravational Waves
| 1
|
| General Pulsars
| 1
|
| Gamma-ray Bursts
| 1
|
| Gamma Rays: ISM
| 1
|
| Galaxy: Evolution
| 1
|
| Galaxy: Centre
| 1
|
| Galaxy: Abundances
| 1
|
| Galaxy Structure
| 1
|
| Galaxy Bulges
| 1
|
| Galaxies: Nuclei
| 1
|
| Galaxies: Luminosity Function
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies: Intergalactic Medium
| 1
|
| Galaxies: Individual: Triangulum
| 1
|
| Galaxies: Individual: Andromeda
| 1
|
| FRBs
| 1
|
| FRB20190520B
| 1
|
| FRB 20190520B
| 1
|
| FRB 20121102
| 1
|
| FRB
| 1
|
| Five-hundred-meter Aperture Spherical Radio Telescope
| 1
|
| Fast Radio Burst
| 1
|
| Errata
| 1
|
| Early-type Stars
| 1
|
| Early Stellar Evolution
| 1
|
| Dwarf Galaxies
| 1
|
| Distance Measure
| 1
|
| Diffuse Molecular Clouds
| 1
|
| Database
| 1
|
| Data Analysis
| 1
|
| Cosmology: Observations
| 1
|
| Cosmic Rays
| 1
|
| Control Systems
| 1
|
| Condensed Matter - Statistical Mechanics
| 1
|
| Cold Neutral Medium
| 1
|
| Clouds
| 1
|
| Circumstellar Matter
| 1
|
| Candidate Selection
| 1
|
| Black Hole Physics
| 1
|
| Binaries: Eclipsing
| 1
|
| Binaries: Close
| 1
|
| Binaries
| 1
|
| Big Data
| 1
|
| Barred Spiral Galaxies
| 1
|
| Automated Flagging
| 1
|
| Astrostatistics Strategies
| 1
|
| Astrophysics - Galaxy Astrophysics
| 1
|
| Astronomy Databases
| 1
|
| Astronomical Observations
| 1
|
| Astronomical Instrumentation
| 1
|
| Artificial Intelligence
| 1
|
| Applied Computing - Astronomy
| 1
|
| Algorithms And Implementation
| 1
|
| Addenda
| 1
|
| Active Main Reflector
| 1
|
| Active Galactic Nuclei
| 1
|
| Accretion Discs
| 1
|
| Abundance Ratios
| 1
|
| 20190520B
| 1
|
| (transients:) Fast Radio Bursts
| 1
|
| (stars:) Pulsars: Individual (PSR J1909+0122)
| 1
|
| (stars): Pulsars: General
| 1
|
| Young Stellar Objects
| 1
|
| Young Massive Clusters
| 1
|
| X-rays: Galaxies
| 1
|
| X-ray Binary Stars
| 1
|
| Warm Neutral Medium
| 1
|
| Transients: Supernovae
| 1
|
| Transients
| 1
|
| Transient
| 1
|
| Time Series Analysis
| 1
|
| Time Domain Astronomy
| 1
|
| The Milky Way
| 1
|
| Telescopes: FAST
| 1
|
| Technosignatures
| 1
|
| Techniques: Miscellaneous
| 1
|
| Techniques: Interferometric
| 1
|
| T Tauri Stars
| 1
|
| Supernovae: General
| 1
|
| Supernovae
| 1
|
| Supernova Remnants
| 1
|
| Stellar-interstellar Interactions
| 1
|
| Stellar Wind Bubbles
| 1
|
| Stellar Flares
| 1
|
| Stellar Abundances
| 1
|
| Statistical And Correlative Studies Of Properties
| 1
|
| Statistical
| 1
|
| Stars: Winds
| 1
|
| Stars: Rotation
| 1
|
| Stars: Pulsars: General
| 1
|
| Stars: Pre-main-sequence
| 1
|
| Stars: Pre-main Sequence
| 1
|
| Stars: Neutron < Stars
| 1
|
| Stars: Massive
| 1
|
| Stars: Mass Loss
| 1
|
| Stars: Kinematics And Dynamics; ISM: H Ii Regions; ISM: Clouds
| 1
|
| Stars: Individual: Constellation Name: W Hydrae
| 1
|
| Stars: Individual: Constellation Name: VY Canis Majoris
| 1
|
| Stars: Individual: Constellation Name: NML Cygni
| 1
|
| Stars: Individual (Orion)
| 1
|
| Stars: Individual (FRB 20201124A)
| 1
|
| Stars: Flare
| 1
|
| Stars: Circumstellar Matter
| 1
|
| Starlight Polarization
| 1
|
| Star-planet Interactions
| 1
|
| Star Formation: Kinematics And Dynamics
| 1
|
| Star Formation Rate
| 1
|
| Spectral Index
| 1
|
| Spectral Energy Distribution
| 1
|
| Space Vehicles: Instruments
| 1
|
| Software: Simulations
| 1
|
| Soft Gamma-ray Repeaters
| 1
|
| Sky Surveys
| 1
|
| Sensitivity
| 1
|
| Security And Privacy - Cryptography
| 1
|
| Rotation Powered Pulsars
| 1
|
| Repeaters
| 1
|
| Relativistic Jets
| 1
|
| Radio Wave Receivers
| 1
|
| Radio Telescopes
| 1
|
| Radio Sources
| 1
|
| Radio Jets
| 1
|
| Radio Frequency Interference
| 1
|
| Radio Emission Lines
| 1
|
| Radio Astronomy Instrumentation
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Quasars
| 1
|
| Pulsars: Individual: Subpulse Drifting-micropulses
| 1
|
| Pulsars: Individual: PSR J2016+3711
| 1
|
| Pulsars: Individual: PSR J1926-0652
| 1
|
| Pulsars: Individual: PSR J1906+0746
| 1
|
| Pulsars: Individual: PSR J1023+0038
| 1
|
| Pulsars: Individual: PSR J0250+5854
| 1
|
| Pulsars: Individual: PSR B1957+20
| 1
|
| Pulsars: Individual: PSR B1642-03
| 1
|
| Pulsars: Individual: PSR B0919+06
| 1
|
| Pulsars: Individual: PSR B0329+54
| 1
|
| Pulsars: Individual: AXP1E2259+586
| 1
|
| Pulsars - Computational Methods
| 1
|
| Pulsar Surveys Simulation
| 1
|
| Pulsar Surveys
| 1
|
| PSR B0531 + 21 (the Crab Pulsar)
| 1
|
| Plasmas
| 1
|
| Physical Data And Processes
| 1
|
| Photon-dominated Region: PDR
| 1
|
| Photon-dominated Region
| 1
|
| Photodissociation Region (PDR)
| 1
|
| Period Search
| 1
|
| Outflows
| 1
|
| Orion
| 1
|
| Optical Observation
| 1
|
| Open Clusters And Associations: Individual: Vela
| 1
|
| Open Clusters And Associations: Individual: Orion
| 1
|
| Opacity
| 1
|
| OMC1
| 1
|
| OH Megamaser
| 1
|
| Numerical Relativity
| 1
|
| Nuclear Astrophysics
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Neutron Star Cores
| 1
|
| Neutron Star
| 1
|
| Neutron
| 1
|
| Neural Networks
| 1
|
| Multi-structural
| 1
|
| Molecular Gas
| 1
|
| Molecular Data
| 1
|
| Middle Infrared
| 1
|
| Methods: Observational
| 1
|
| Methods And Techniques
| 1
|
| Methods
| 1
|
| Metallicity
| 1
|
| Mass Function
| 1
|
| Low-luminosity Active Galactic Nuclei
| 1
|
| Local Group
| 1
|
| Large-scale Structure Of Universe
| 1
|
| Large Magellanic Cloud
| 1
|
| L-band
| 1
|
| K.8.1
| 1
|
| Jets
| 1
|
| J.2
| 1
|
| ISM: Supernova Remnants
| 1
|
| ISM: Molecules.
| 1
|
| ISM: Individual: Taurus
| 1
|
| ISM: Individual: Saggitarius B2
| 1
|
| ISM: Individual: Orion
| 1
|
| ISM: Individual: Name: ρ Ophiuchi Cloud
| 1
|
| ISM: Individual: Name: Orion
| 1
|
| ISM: Individual Objects:ρOph A SM 1
| 1
|
| ISM: Individual Objects: ρ Ophiuchi Molecular Cloud Complex
| 1
|
| ISM: Individual Objects: Taurus Molecular Cloud
| 1
|
| ISM: Individual Objects: Orion A
| 1
|
| ISM: Individual Objects: Ophiuchi
| 1
|
| ISM: Individual Objects: NGC 2024
| 1
|
| ISM: Individual Objects: MMS-7
| 1
|
| ISM: Individual Objects: IC348-SMM2
| 1
|
| ISM: Individual Objects: IC 5146
| 1
|
| ISM: Individual Objects: GM Tau 2MASS J04141188+2811535 2MASS J04381486+2611399
| 1
|
| ISM: Individual Objects: G19.61 – 0.23
| 1
|
| ISM: Individual Objects: G034.43+00.24
| 1
|
| ISM: Individual Objects: CTB 87 (G74.9+1.2)
| 1
|
| ISM: Individual Objects: Barnard 1
| 1
|
| ISM: Individual (Saggitarius B2)
| 1
|
| ISM: Individual (hydrogen)
| 1
|
| ISM: General
| 1
|
| ISM: Clouds-stars: Mass Function
| 1
|
| ISM: Abundance
| 1
|
| ISM
| 1
|
| Interstellar Scintillation
| 1
|
| Interstellar Scattering
| 1
|
| Interstellar Emissions
| 1
|
| Interstellar Dust Extinction
| 1
|
| (434); Protostars
| 1
|
| (371); Interstellar Medium (847)
| 1
|
| (2050); Multiple Stars
| 1
|
| (1569); Early Stellar Evolution
| 1
|
| (1302); Low Mass Stars
| 1
|
| (1081); Dense Interstellar Clouds
| 1
|