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 - Cosmology And Nongalactic Astrophysics
| 176
|
| Cosmology: Observations
| 95
|
| Cosmic Background Radiation
| 92
|
| Astrophysics - Astrophysics Of Galaxies
| 69
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 52
|
| Methods: Data Analysis
| 51
|
| Large-scale Structure Of Universe
| 36
|
| Galaxies: Clusters: General
| 32
|
| Cosmological Parameters
| 31
|
| Surveys
| 29
|
| Polarization
| 23
|
| Submillimeter: ISM
| 23
|
| Astrophysics
| 22
|
| Extinction
| 20
|
| Dust
| 20
|
| Methods: Statistical
| 19
|
| Cosmic Microwave Background
| 18
|
| ISM: General
| 18
|
| Space Vehicles: Instruments
| 16
|
| Instrumentation: Detectors
| 16
|
| Cosmology: Theory
| 15
|
| Catalogs
| 14
|
| Radio Continuum: ISM
| 13
|
| Cosmology
| 12
|
| Galaxies: Clusters: Intracluster Medium
| 12
|
| Gravitational Lensing: Weak
| 12
|
| Cosmology: Cosmic Microwave Background
| 11
|
| ISM: Clouds
| 10
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 10
|
| Radiation Mechanisms: General
| 10
|
| Galaxy: General
| 10
|
| ISM: Magnetic Fields
| 10
|
| X-rays: Galaxies: Clusters
| 9
|
| Inflation
| 9
|
| Early Universe
| 9
|
| Submillimeter: General
| 8
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 8
|
| Galaxies: Active
| 8
|
| Infrared: ISM
| 8
|
| ISM: Structure
| 8
|
| Dark Energy
| 7
|
| Instrumentation: Polarimeters
| 6
|
| 98.70.Vc
| 6
|
| BL Lacertae Objects: General
| 6
|
| Diffuse Radiation
| 6
|
| Radio Continuum: General
| 6
|
| Local Insterstellar Matter
| 6
|
| Background Radiations
| 6
|
| Submillimeter: Galaxies
| 6
|
| Galaxies: Evolution
| 6
|
| Radio Continuum: Galaxies
| 5
|
| High Energy Physics - Phenomenology
| 5
|
| Quasars: General
| 5
|
| Galaxies: Star Formation
| 5
|
| General Relativity And Quantum Cosmology
| 5
|
| Galaxies: Distances And Redshifts
| 5
|
| Balloons
| 4
|
| Techniques: Photometric
| 4
|
| Dark Matter
| 4
|
| Galaxies: ISM
| 4
|
| Reionization
| 4
|
| High Energy Physics - Theory
| 4
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 4
|
| Stars: Formation
| 4
|
| Bolometers
| 4
|
| Gravitation
| 4
|
| Techniques: Image Processing
| 4
|
| Methods: Numerical
| 4
|
| Galaxies: Photometry
| 4
|
| Relativistic Processes
| 3
|
| Radio Microwave
| 3
|
| Galaxies: General
| 3
|
| Radiation Mechanisms: Non-thermal
| 3
|
| Galaxies
| 3
|
| First Stars
| 3
|
| Errata
| 3
|
| Dark Ages
| 3
|
| Cosmology: Cosmological Parameters
| 3
|
| Cosmic Rays
| 3
|
| ISM:
| 3
|
| Telescopes
| 3
|
| Instrumentation: Photometers
| 3
|
| Physics - Instrumentation And Detectors
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Infrared: Galaxies
| 3
|
| Infrared: Diffuse Background
| 3
|
| Addenda
| 3
|
| High-redshift Galaxies
| 3
|
| 98.80.-k
| 3
|
| 95.85.Bh
| 3
|
| Gamma-rays: Galaxies
| 2
|
| Quasars: Emission Lines
| 2
|
| Evolution
| 2
|
| Radiation
| 2
|
| Background Radiation
| 2
|
| B-modes
| 2
|
| Magnetic Fields
| 2
|
| Transition Edge Sensors
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Galaxies: High-redshift
| 2
|
| Methods: Analytical
| 2
|
| Galaxies: Jets
| 2
|
| Space Vehicles
| 2
|
| Galaxies: Statistics
| 2
|
| Galaxies: Structure
| 2
|
| Submillimeter: Diffuse Background
| 2
|
| Radiofrequency Cosmic Radiation
| 2
|
| Gamma Rays: Galaxies
| 2
|
| 98.80.Es
| 2
|
| Observational Cosmology
| 2
|
| CMB
| 2
|
| X-rays: Galaxies
| 2
|
| Polarimetry
| 2
|
| Clouds
| 2
|
| Turbulence
| 2
|
| CMBR Experiments
| 2
|
| Cosmic
| 2
|
| Reference Systems
| 2
|
| Stratospheric Balloons
| 2
|
| Techniques: Miscellaneous
| 2
|
| Planetary Nebulae: General
| 2
|
| Astronomical Observations
| 1
|
| Astronomical Instruments
| 1
|
| Asteroids: General
| 1
|
| Ariel
| 1
|
| Antarctic Astronomy
| 1
|
| Active Or Peculiar Galaxies Objects And Systems
| 1
|
| 98.80.Cq
| 1
|
| 98.54.-h
| 1
|
| Zodiacal Dust
| 1
|
| X-rays: General
| 1
|
| Unbiased Estimator
| 1
|
| Transition-edge Sensors
| 1
|
| TESs
| 1
|
| Telescopes: Balloon-Borne
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Polarimetric
| 1
|
| TDM
| 1
|
| T Dwarfs
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Submillimetre: ISM
| 1
|
| Submillimetre: Diffuse Background
| 1
|
| Structure Of Universe
| 1
|
| Structure
| 1
|
| Stratosphere
| 1
|
| Strategy
| 1
|
| Stokes Polarimeter
| 1
|
| Stellar Masses
| 1
|
| Stars: Protostars
| 1
|
| Stars: Abundances
| 1
|
| Solar Neighborhood
| 1
|
| Site Testing
| 1
|
| Satellite
| 1
|
| Radiotelescopes
| 1
|
| Radioastronomy
| 1
|
| Quasars: Individual: 4C +49.22
| 1
|
| Quasars
| 1
|
| Primordial Nucleosynthesis
| 1
|
| Primordial Gravitational Wave
| 1
|
| Polarisation
| 1
|
| Planets And Satellites: General
| 1
|
| Planets And Satellites: Dynamical Evolution And Stability
| 1
|
| Planets And Satellites: Detection
| 1
|
| Physics - Atmospheric And Oceanic Physics
| 1
|
| Photometry
| 1
|
| Photoconductors And Bolometers
| 1
|
| Particle-theory And Field-theory Models Of The Early Universe
| 1
|
| Parameter Estimation
| 1
|
| Opacity
| 1
|
| OLIMPO
| 1
|
| Observations
| 1
|
| Observation And Data Reduction Techniques
| 1
|
| Noise
| 1
|
| Multi-moded Optics
| 1
|
| Mm/sub-mm Astronomy
| 1
|
| Missions
| 1
|
| Minor Planets
| 1
|
| Methods: Observational
| 1
|
| Mechanisms: General
| 1
|
| Mass-to-light Ratio
| 1
|
| Magellanic Clouds
| 1
|
| Lyman-break Galaxies
| 1
|
| Likelihood Function
| 1
|
| LEKIDs
| 1
|
| Large-scale
| 1
|
| ISM: Supernova Remnants
| 1
|
| ISM: Molecules
| 1
|
| ISM: Magnetic
| 1
|
| ISM: Individual Objects: Taurus-Auriga Molecular Cloud
| 1
|
| ISM: HII Regions
| 1
|
| ISM: Bubbles
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interferometry
| 1
|
| Interferometer
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instrumentation
| 1
|
| Infrared: General
| 1
|
| Infrared Submillimeter Wave Microwave And Radiowave Receivers And Detectors
| 1
|
| Infrared Spectra
| 1
|
| HII Regions
| 1
|
| High Energy Physics - Experiment
| 1
|
| Ground Segment
| 1
|
| Gravitational Waves And CMBR Polarization
| 1
|
| Gravitational Waves
| 1
|
| Gravitational Wave Detectors And Experiments
| 1
|
| Gravitational Lensing: Strong
| 1
|
| Gamma Rays: ISM
| 1
|
| Galaxy: Nucleus
| 1
|
| Galaxy: Halo
| 1
|
| Galaxy: Formation
| 1
|
| Galaxy: Disk
| 1
|
| Galaxy: Center
| 1
|
| Galaxy Spectroscopy
| 1
|
| Galaxies: Quasars: General
| 1
|
| Galaxies: Nuclei
| 1
|
| Galaxies: Individual: Messier 31
| 1
|
| Galaxies: Halos
| 1
|
| Galaxies: Fundamental Parameters
| 1
|
| Galaxies: Clusters: Interacluster Medium
| 1
|
| Galaxies: Clusters: Individual: Virgo
| 1
|
| Galaxies: Clusters: Individual: PLCKG214.6+37.0
| 1
|
| Galaxies: Clusters: Individual: Coma Cluster
| 1
|
| Galaxies: Clusters: Individual: 1ES0657-556
| 1
|
| Galaxies:
| 1
|
| Fourier Transform Optics
| 1
|
| Fields
| 1
|
| Exoplanets
| 1
|
| Data Management
| 1
|
| Data Analysis - Methods
| 1
|
| Data Analysis
| 1
|
| Cryogenic Detectors
| 1
|
| 04.80.Nn
| 1
|
| Cosmology: Clusters Of Galaxies
| 1
|
| Cosmological Parameters From CMBR
| 1
|
| Cosmic Background
| 1
|
| Computer Modeling And Simulation
| 1
|
| CMBR Polarisation
| 1
|
| Clusters: Intracluster Medium
| 1
|
| Clusters Of Galaxies
| 1
|
| Celestial Mechanics
| 1
|
| Calibration
| 1
|
| Bolometric Interferometer
| 1
|
| Bolometer
| 1
|
| Blackbody Radiation
| 1
|
| BL Lacertae Objects: Individual: PKS 0537-441
| 1
|
| Atomic Data
| 1
|
| Atmospheric Effects
| 1
|
| Astrophysics - Galaxy Astrophysics
| 1
|
| Astronomy Image Processing
| 1
|
| 95.85.-e
| 1
|
| 95.75.Kk
| 1
|
| 95.75.Hi
| 1
|
| 95.75.-z
| 1
|
| 95.55.Rg
| 1
|
| 33.20.Ea
| 1
|
| 07.57.Kp
| 1
|
| Cosmology: Miscellaneous
| 1
|