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]
| 46
|
| X-Rays: Stars
| 39
|
| Astrophysics
| 33
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 21
|
| Stars: Pre-Main-Sequence
| 12
|
| Cataclysmic Variables
| 10
|
| Black Hole Physics
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 7
|
| ACCRETION
| 6
|
| Novae
| 6
|
| Galaxies: Active
| 6
|
| Instrumentation: Spectrographs
| 6
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 6
|
| Methods: Observational
| 6
|
| Astrophysics - Astrophysics Of Galaxies
| 6
|
| Accretion Disks
| 6
|
| X-rays: Binaries
| 6
|
| X-Rays: ISM
| 6
|
| Space Vehicles: Instruments
| 5
|
| Satellite
| 5
|
| ISM: Clouds
| 5
|
| Infrared: Stars
| 5
|
| GALAXY: CENTER
| 5
|
| Stars: Novae
| 5
|
| Stars: Formation
| 5
|
| Instrumentation: Detectors
| 4
|
| X-ray Microcalorimeter
| 4
|
| X-rays: Galaxies: Clusters
| 4
|
| Radio Continuum: ISM
| 4
|
| Stars: Early-Type
| 4
|
| X-rays: Galaxies
| 4
|
| ISM: Supernova Remnants
| 4
|
| X-ray Astronomy
| 4
|
| X-rays: Diffuse Background
| 4
|
| Stars: White Dwarfs
| 3
|
| Mass Function
| 3
|
| X-RAYS: GENERAL
| 3
|
| Be
| 3
|
| Galaxies: Seyfert
| 3
|
| Polarization
| 3
|
| Galaxies: Clusters: Intracluster Medium
| 3
|
| Cosmic Microwave Background
| 3
|
| Stars: Luminosity Function
| 3
|
| Inflation
| 3
|
| Stars: Emission-line
| 3
|
| General Relativity And Quantum Cosmology
| 2
|
| Low Temperature Detector
| 2
|
| LMC)
| 2
|
| Galaxy: Stellar Content
| 2
|
| Space Cryogenics
| 2
|
| Space Applications
| 2
|
| Stars: Variables: Other
| 2
|
| TES
| 2
|
| Galaxy: Disk
| 2
|
| ISM: Jets And Outflows
| 2
|
| X-ray Imaging And Spectroscopy Mission
| 2
|
| Galaxies: Individual (SMC
| 2
|
| Galaxies: Individual (NGC 1275)
| 2
|
| ISM: Individual: Alphanumeric: OMC-1
| 2
|
| Galaxies: Evolution
| 2
|
| Galaxies: Clusters: Individual (Perseus)
| 2
|
| Radiative Transfer [S]
| 2
|
| Digital Signal Processing
| 2
|
| X-ray Binary Stars
| 2
|
| Stars: Late-type
| 2
|
| Cryogenics
| 2
|
| XRISM
| 2
|
| Primordial Gravitational Wave
| 2
|
| Plasma Astrophysics
| 2
|
| Stars: Individual (1E 1740.7-2942)
| 2
|
| CMB
| 2
|
| ISM: HII Regions
| 2
|
| Stars: Flare
| 2
|
| ISM: H II Regions
| 2
|
| Bolometers
| 2
|
| BINARIES: GENERAL
| 2
|
| Stars: Dwarf Novae
| 2
|
| Stars: Coronae
| 2
|
| Stars: Binaries: Close
| 2
|
| Infrared: ISM
| 2
|
| Microcalorimeter
| 2
|
| Methods: Data Analysis
| 2
|
| High Energy Astrophysics
| 2
|
| Stars: Wolf-Rayet
| 2
|
| Open Clusters And Associations: Individual (Trumpler 14 And 16)
| 1
|
| Open Clusters And Associations: Individual (Pismis 24)
| 1
|
| OMT
| 1
|
| OMC-3)
| 1
|
| Molecular Processes
| 1
|
| Mission
| 1
|
| Microvibration Interference
| 1
|
| Microphonics
| 1
|
| Methods: Analytical
| 1
|
| MAGELLANIC CLOUDS
| 1
|
| Low-temperature Detector
| 1
|
| Low-mass X-ray Binary Stars
| 1
|
| Line: Formation
| 1
|
| Joule-Thomson Coolers
| 1
|
| ISM: Stars
| 1
|
| ISM: Reflection Nebulae
| 1
|
| ISM: Molecules
| 1
|
| ISM: Individual: NGC Number: NGC 6357
| 1
|
| ISM: Individual: Name: Orion Nebula
| 1
|
| ISM: Individual: Name: Carina Nebula
| 1
|
| ISM: Individual: Alphanumeric: W49A
| 1
|
| ISM: Individual: Alphanumeric: OMC-3
| 1
|
| ISM: Individual: Alphanumeric: L1551
| 1
|
| ISM: Individual: Alphanumeric: HH 154
| 1
|
| ISM: Individual Objects: NGC 7538
| 1
|
| ISM: Individual Objects (N 132 D)
| 1
|
| ISM: Individual Objects (G21.5-0.9)
| 1
|
| ISM: Individual (ρ Ophiuchi Cloud)
| 1
|
| ISM: Individual (Sgr D)
| 1
|
| ISM: Individual (Sagittarius C)
| 1
|
| ISM: INDIVIDUAL (SAGITTARIUS B2)
| 1
|
| ISM: Individual (rho Ophiuchi Cloud)
| 1
|
| ISM: Individual (OMC-2
| 1
|
| ISM: Individual (Monoceros R2)
| 1
|
| ISM: Individual (M 17)
| 1
|
| ISM: Individual (Crab Nebula)
| 1
|
| ISM: Individual (Cepheus Molecular Cloud)
| 1
|
| ISM: Individual (Carina Nebula)
| 1
|
| ISM: Herbig-Haro Objects
| 1
|
| ISM: Dust
| 1
|
| ISM: Bubbles
| 1
|
| ISM: Abundances
| 1
|
| Ionization
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Institution
| 1
|
| Infrared: Planetary Systems
| 1
|
| Infrared Submillimeter Wave Microwave And Radiowave Receivers And Detectors
| 1
|
| Infrared Radiation
| 1
|
| High-performance Computing
| 1
|
| High Energy Physics - Phenomenology
| 1
|
| High Energy Physics - Experiment
| 1
|
| He II Systems
| 1
|
| HD 110432)
| 1
|
| Gate Valve
| 1
|
| Gamma-ray Bursts
| 1
|
| Galaxy: Structure
| 1
|
| Galaxy: Open Clusters: Individual (Arches Cluster)
| 1
|
| Galaxy: Open Clusters And Associations: Individual: Name: Orion Nebula Cluster
| 1
|
| Galaxy: Open Clusters And Associations: Individual: Name: Orion
| 1
|
| Galaxy: Open Clusters And Associations: Individual: Name: Cepheus OB3
| 1
|
| Galaxy: Open Clusters And Associations: Individual: Alphanumeric: Westerlund 2
| 1
|
| Galaxy: Bulge
| 1
|
| GALAXY: ABUNDANCES
| 1
|
| Galaxies: Starburst
| 1
|
| Galaxies: Radio Galaxy
| 1
|
| 07.20.Fw
| 1
|
| Galaxies: Magellanic Clouds
| 1
|
| Galaxies: Individual: M 51 NGC 4490 NGC 4485
| 1
|
| Galaxies: Individual (IRAS 13224-3809)
| 1
|
| Galaxies: Clusters: Individual: A426
| 1
|
| Galaxies: Clusters: Individual (Perseus Cluster)
| 1
|
| Extinction
| 1
|
| Evolution
| 1
|
| Electromagnetic Interference
| 1
|
| Detector Noise
| 1
|
| Dark Matter
| 1
|
| Cryogenic Detector
| 1
|
| Cosmology
| 1
|
| Cosmic Microwave Background Radiation
| 1
|
| Cosmic Inflation
| 1
|
| Cooperation
| 1
|
| CMBR Polarisation
| 1
|
| CMBR Experiments
| 1
|
| CMBR Detectors
| 1
|
| Clusters Of Galaxies
| 1
|
| Chemical Evolution
| 1
|
| Calorimetry
| 1
|
| Calorimeters
| 1
|
| Brown Dwarfs
| 1
|
| Bragg Diffraction
| 1
|
| Bolometer
| 1
|
| Black Holes
| 1
|
| Binaries: Close
| 1
|
| Beryllium
| 1
|
| B-mode Polarization
| 1
|
| B-mode
| 1
|
| Atomic Spectroscopy
| 1
|
| Astrostatistics Tools
| 1
|
| Astrostatistics
| 1
|
| Astrophysics - Galaxy Astrophysics
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 1
|
| Astronomy
| 1
|
| Astrometry
| 1
|
| ASTRO-H
| 1
|
| Ark 564
| 1
|
| Adiabatic Demagnetization
| 1
|
| X-rays: Spectra
| 1
|
| X-rays: Individuals: G21.5-0.9
| 1
|
| X-rays: Individual: 1H 0707--495
| 1
|
| X-rays: Individual (PKS 2155‑304)
| 1
|
| X-rays: Individual (N 132 D)
| 1
|
| X-rays: Individual (Cygnus X-1)
| 1
|
| X-rays: Individual (Crab)
| 1
|
| X-rays: Bursts
| 1
|
| X-Rays
| 1
|
| X-ray Transmission
| 1
|
| X-ray Spectrometer
| 1
|
| X-ray Microcalorimeters
| 1
|
| X-ray Detector
| 1
|
| X-ray CCDs
| 1
|
| X-ray Calorimeter
| 1
|
| X-ray
| 1
|
| Warm-hot Intergalactic Medium
| 1
|
| V458 Vulpeculae)
| 1
|
| V2672 Ophiuchi)
| 1
|
| V2491 Cygni)
| 1
|
| Telescopes
| 1
|
| Telescope
| 1
|
| Techniques: Photometric
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| SXP 523)
| 1
|
| Supernova Remnants-- X-rays: ISM
| 1
|
| Stirling
| 1
|
| Stellar Mass Loss
| 1
|
| Stellar Flares
| 1
|
| Stellar Coronae
| 1
|
| Stellar Activity
| 1
|
| Stellar Accretion Disks
| 1
|
| Stars: Pulsars: Individual (Suzaku J0102.8-7204
| 1
|
| Stars: Pulsars: General
| 1
|
| Stars: Pre-main Sequence
| 1
|
| Stars: Planetary Systems: Protoplanetary Disks
| 1
|
| STARS: NEUTRON
| 1
|
| Stars: Magnetic Fields
| 1
|
| Stars: Low-Mass
| 1
|
| Stars: Individual: ρ Oph
| 1
|
| Stars: Individual: V458 Vul
| 1
|
| Stars: Individual: U Scorpii
| 1
|
| Stars: Individual: Nova Cygni 2008 Number 2 V2491 Cygni
| 1
|
| Stars: Individual: Elias 29
| 1
|
| Stars: Individual: Alphanumeric: ROX 31
| 1
|
| Stars: Individual: Alphanumeric: ROX 21
| 1
|
| Stars: Individual: Alphanumeric: DoAr 21
| 1
|
| Stars: Individual (π Aquarii)
| 1
|
| Stars: Individual (η Carinae)
| 1
|
| Stars: Individual (γ Cassiopeiae
| 1
|
| Stars: Individual (Z Camelopardalis)
| 1
|
| Stars: Individual (XSSJ 12270-4859)
| 1
|
| Stars: Individual (XSS J12270-4859)
| 1
|
| Stars: Individual (SuzakuJ0105-72)
| 1
|
| Stars: Individual (Orion Molecular Cloud 2/3)
| 1
|
| Stars: Individual (Nova Vulpeculae 2007 Number 1
| 1
|
| Stars: Individual (Nova Ophiuchi 2009
| 1
|
| Stars: Individual (Nova Cygni 2008 Number 2
| 1
|
| Stars: Individual (L1448)
| 1
|
| Stars: Individual (IGR J16318-4848)
| 1
|
| Stars: Individual (HD161084)
| 1
|
| Stars: Individual (GRS 1915+105)
| 1
|
| Stars: Individual (CXOGC J174645.3-281546
| 1
|
| Stars: Binaries: General
| 1
|
| Stars: Abundances
| 1
|
| Spectroscopy
| 1
|
| Space Plasmas [H]
| 1
|
| Source Population Study
| 1
|
| Signal Processing Electronics
| 1
|
| Sensitivity
| 1
|
| Scattering
| 1
|
| ROSCA
| 1
|
| Resolve
| 1
|
| Refrigerators Low-temperature Detectors And Other Low-temperature Equipment
| 1
|
| Radio Continuum: Stars
| 1
|
| Quantum Gravity
| 1
|
| Pulsars: Individual (PSR J1833-1034)
| 1
|
| Pulsars: Individual (B0531+21)
| 1
|
| PULSARS: INDIVIDUAL (AX J0058-7203)
| 1
|
| PULSARS: INDIVIDUAL (AX J0051-733)
| 1
|
| PULSARS: INDIVIDUAL (AX J0049-729)
| 1
|
| Pulsars: General
| 1
|
| Physics - Instrumentation And Detectors
| 1
|
| Peer Selection
| 1
|
| 2XMMp J174645.2-281547)
| 1
|
| 07.57.Kp
| 1
|
| 07.20.Mc
| 1
|
| Galaxies: Nuclei
| 1
|