Appendix B: Science Keywords

Keywords to be used in APT when submitting a proposal.

The Tables in this Appendix list the Scientific Keywords that are valid for use in the proposal template. 

Within a panel, proposals are assigned to individual reviewers based on the reviewers' expertise and based partly on the keywords given in the proposal and partly on analysis of the proposal text. Generally, the more keywords the proposer selects the better the match to reviewers' expertise. Proposals can designate both a Science Category and an Alternate Category. Designating an Alternate Category enables usage of keywords from multiple categories. The Science Mission Office at STScI reserves the right to re-classify proposals.

For additional information on the proposal sorting into each panel, see HST Proposal Selection Procedures. The HST Scientific Categories and Keywords were developed using the Unified Astronomy Thesaurus beginning in Cycle 28.


Solar System Astronomy:

Asteroids

Astronomical models

Astronomical simulations

Atmospheric composition

Atmospheric variability

Binary systems / Multiple systems

Biomarkers

Centaurs

Chemical composition

Comets

Inner planets

Irregular satellites

Main belt asteroids

Minor planets

Natural satellites

Near-Earth objects

Occultation

Orbits

Outer planets

Planetary atmospheres

Planetary rings

Planetary surfaces

Small solar system bodies

Space weather

Surface composition

Surface ices

Surface processes

Surface variability

Trans-Neptunian objects

Transits

Trojan asteroids

Zodiacal cloud


Stellar Physics and Stellar Types:

Astrometry
Astronomical models
Astronomical simulations
Binary stars / Trinary stars
Black holes
Brown dwarfs
Circumstellar disks
Circumstellar matter
Cosmological parameters
Cosmology
Early-type stars
Evolved stars
Gamma-ray bursts
Gravitational wave sources
H II regions
High contrast techniques
Hubble constant
Interacting binary stars
Intermediate-type stars
Interstellar dust
Interstellar medium
Late-type stars
Low mass stars
Main sequence stars
Massive stars
Molecular clouds
Neutron stars
Planetary nebulae
Pre-main sequence stars
Pulsars
Radiative transfer
Stellar abundances
Stellar accretion disks
Stellar atmospheres
Stellar distance
Stellar evolution
Stellar jets
Stellar mergers
Stellar phenomena
Stellar structures
Supernovae
Transient sources
Variable stars
White dwarf stars
Young stellar objects


Galaxies:

Astronomical models
Astronomical simulations
Balmer break
Chemical abundances
Cosmic dawn
Cosmic infrared background
Cosmic noon
Cosmological parameters
Cosmology
Dark energy
Dark matter distribution
Disk galaxies
Dwarf galaxies
Elliptical galaxies
Emission line galaxies
Extragalactic legacy and deep fields
Galaxy bulges
Galaxy clusters
Galaxy dark matter halos
Galaxy disks
Galaxy environments
Galaxy groups
Galaxy kinematics
Galaxy mergers
Galaxy spheroids
Galaxy stellar halos
Galaxy structure
Gravitational lensing
High-redshift galaxies
Hubble constant
Infrared photometry
Interacting galaxies
Interstellar dust
Irregular galaxies
Large-scale structure of the universe
Local Group
Luminous infrared galaxies
Lyman-break galaxies
Magellanic Clouds
Molecular gas
Nearby galaxies
Polycyclic aromatic hydrocarbons
Population III stars
Post-starburst galaxies
Protoclusters
Protogalaxies
Quenched galaxies
Reionization
Scaling relations
Spectral energy distribution
Star clusters
Star formation
Starburst galaxies
Stellar populations
Ultraluminous infrared galaxies


Exoplanets and Exoplanet Formation:

Astronomical models
Astronomical simulations
Biomarkers
Brown Dwarfs
Chemical composition
Circumstellar disks
Circumstellar dust
Circumstellar gas
Debris disks
Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanet atmospheric variability
Exoplanet detection methods
Exoplanet dynamics
Exoplanet structure
Exoplanet surfaces
Exoplanet systems
Extrasolar gaseous giant planets
Extrasolar ice giants
Extrasolar rocky planets
Extrasolar sub-Neptunes
Free floating planets
High contrast techniques
Natural satellites (Extrasolar)
Planet hosting stars
Protoplanetary disks (Extrasolar)
Radial velocity
Space weather
Stellar accretion disks
Transits
White dwarf stars


Stellar Populations and the Interstellar Medium:

Astrochemistry
Astrometry
Astronomical models
Astronomical simulations
Chemical abundances
Cosmological parameters
Cosmology
Dwarf galaxies
Early-type stars
Elliptical galaxies
Galactic center
Galaxy bulges
Galaxy evolution
Galaxy halos
Galaxy spheroids
Globular star clusters
Gravitational microlensing
H II regions
Hertzsprung Russell diagram
High-mass star formation
Hubble constant
Initial mass function
Intermediate-type stars
Interstellar atomic gas
Interstellar dust
Interstellar ices
Interstellar medium
Irregular galaxies
Late-type stars
Local Group
Low metallicity stars
Low-mass star formation
Magellanic Clouds
Molecular clouds
Molecular gas
Open star clusters
Planetary nebulae
Polycyclic aromatic hydrocarbons
Population I stars
Population II stars
Population III stars
Red giant tip
Resolved stellar populations
Star clusters
Star formation
Star formation histories
Stellar distance
Stellar kinematics
Stellar population synthesis
Young stellar objects


Supermassive Black Holes and Active Galaxies:

AGN host galaxies
Astronomical models
Astronomical simulations
Blazars
Broad-absorption line quasar
Emission line galaxies
Galaxy jets
Galaxy winds
High contrast techniques
High-luminosity active galactic nuclei
LINER galaxies
Low-luminosity active galactic nuclei
M-sigma relation
Markarian galaxies
Quasars
Quenched galaxies
Radio cores
Reverberation mapping
Seyfert galaxies
Stellar accretion disks
Stellar feedback
Supermassive black holes
X-ray active galactic nuclei



Intergalactic Medium and Circumgalactic Medium:

Astronomical models
Astronomical simulations
Circumgalactic medium
Cooling flows
Damped Lyman-alpha systems
Gunn-Peterson effect
Intergalactic dust clouds
Intergalactic medium
Intracluster medium
Lyman-alpha forest
Metal line absorbers
Reionization
Warm-hot intergalactic medium