APRIM2026: 2026 ASIA-PACIFIC REGIONAL IAU MEETING
TALK KEYWORD INDEX

This page contains an index consisting of author-provided keywords.

(
(Cosmology:) large-scale structure of Universe
-
- Collaboration
- Friendship
- Sustainability
2
2MASS
A
Abundances
Accessibility
Accreting binary
Accreting pulsar: XTE J1829-098
Accretion
accretion discs
Accretion disk
Accretion history
active debris removal
Active Galactic Nuclei
Active Galactic Nucleus
Active galaxies
Active Learning
Adaptive Optics
AGB
AGB stars
AGN
AGN activity
AGN Host Morphology
AGN jets
AGN luminosity function
AGN unification
AGNs
AI
AI for science
AI-based learning
Air-Bearing Spacecraft Testing Facilities
ALFALFA
ALMA
ALMA Wideband Sensitivity Upgrade (WSU)
Analog activities
angular momentum
Angular momentum of dark matter haloes
AOE (ADS Orbital Elements)
area-to-mass ratio
ARRAKIHS
Artificial Intelligence
asia
Asian telescope network
asteroid hazard problem
Asteroid regolith
Asteroids
Asteroseismology
Astro-localization
Astro-Pedagogy
Astro-tourism
Astrochemistry
Astronom surveys and time-domain astronomy
Astronomical Big Data
Astronomical facilities
astronomical facility
astronomical instrument
Astronomical Instrumentation
Astronomical Surveys
Astronomy
Astronomy Education
astronomy education and public engagement
astronomy foundation modal
Astronomy observations
Astronomy outreach
Astronomy research
Astrophysical jets
astrophysical plasmas
Astrophysics
AstroSat
astrotourism
Attenuation
Attitude Determination and Control Subsystems (ADCS)
Attitude Inversion
Automatic Identification
Autonomous Mass-Balancing
Autonomous Space Systems
Awareness Data-Driven Models
Axion-like particle
B
Barred galaxies
Batch Least Squares Estimation
Bayesian Inference
Bayesian Statistics
Big bang
Big data
big data analysis
Big surveys
binaries
binaries: close
binary
Binary pulsars
Binary star
binary stars
Binary systems
Binary/Triple star system
Biosignatures
Black Hole
black hole entropy
Black hole physics
black holes
Bootes Void
boundary spanning
BRICS
broad emission lines
broad-line region
bulges
Burstiness of Star Formation
Byurakan Astrophysical Observatory (BAO)
C
Cambodia
Cataclysmic variable
cataclysmic variables
CC-SNe central engines
central compact objects
Centre-of-Mass Alignment
CFHT
CFL EoS
Chang'e-7
Chemical Enrichment
chemical evolution
Chinese moon mission
Chinese space science
Chinese Space Station
Chinese Space Station Telescope (CSST)
Circumbinary disks
circumgalactic medium
Circumstellar disk
Circumstellar disks
circumstellar envelope
circumstellar masers
Circumstellar material
circumstellar matter
Circumstellar medium
circumstellar nebulae
citizen science
cluster
cluster membership
CMBR
CO molecule
co-evolution
coherent radio emission
Collision Warning
Color-Magnitude Diagrams
Colour super-conductivity $(\Delta)$
common envelope evolution
Community Engagement
Community-astronomy
community-based strategies
compact binaries
compact binary coalescences
Compact binary mergers
Compact object merger
compact stars
Complex organic molecules
Compliance and Commercial
Computational optics
conference
Conjunction Analysis
contextual engagement
continuous gravitational waves
coordinated campaigns
Coordination
Core-collapse supernova
core-collapse supernovae
Cosmic acceleration
cosmic chemical enrichment
cosmic dawn
Cosmic dawn and reionization
Cosmic Filaments
cosmic noon
Cosmic Ray
Cosmic Ray Acceleration
Cosmic rays
cosmic reionization
cosmic structure formation
cosmic web
cosmic-ray
Cosmological Constraints
Cosmological Foreground
Cosmological parameters (339)
Cosmological Simulation
Cosmological simulations
Cosmology
Creatunion
Critical Mass
CSPNe
CSST
CSU
CTE
Cultural Heritage & Nomenclature
D
Dark & Quiet Skies
dark ages
Dark and Quiet Skies
Dark Clouds
dark current
Dark energy
dark matter
Dark matter distribution
dark matter halo
Dark Matter Halo Mass
Dark matter halos
dark skies
Data Analysis
data cleaning
data mining
Data Release
Data Service
data visualization
Databases
day-time asteroids
DBSCAN Clustering
Debris detection
debris removal
decameter asteroids
Decaying Dark Matter
Deep learning
Deep synoptic array-2000 (DSA-2000)
Democratization of Science
DESI
Development
Diffuse X-ray background
Diffusive Shock Acceleration
Digital adaptive optics
Digital Literacy
Direct imaging
Disks
Disposal orbits
Distance
distance scale
Distance scales
Distributed SSA
Diverse ionization
Diverse Motion Characteristics
double black holes
double white dwarfs
DSL project
Dust
Dust attenuation
Dust polarization
Dwarf galaxies
Dwarf galaxy
E
Early Universe
Early universe cosmology
Early-type galaxies
early-type stars
eclipsing binaries
Economic Trade Offs
ecosystem
education
Educational Card Game
Educational Content Development
Einstein Probe
Electron precipitation
Emission line
Emission lines
emission spectra
Emission-line galaxies
engagement development
entrepreneurship
Environment
Environmental effects on galaxy formation
Environmental Influence
EP-FXT Source Catalog
equatorial sky
ESA F-Mission
escape fraction
exomoon
Exoplanet
Exoplanet atmosphere
Exoplanet migration
Exoplanet systems
Exoplanets
External Shear
Extinction
Extrasolar planets
Extreme Universise
Extremenly Large Telescope
F
Facilities
Faint Object Extraction
fallback accretion
FASHI
FAST
fast radio bursts
Fast radio bursts (FRBs)
Fast X-ray transient
feedback
flagship
flight schemes
Flipbook Animation
fluorine nucleosynthesis (HF)
Formation of interdisciplinary competencies
Fractal turbulence MR
Framework Ontology
FRB
FRB progenitor models
Fullerenes
future facilities
G
Gaia
Gaia DR3
galactic bars
Galactic Center
Galactic feedback
galactic outflows
Galaxies
galaxies: active
galaxies: clusters: general
galaxies: clusters: intracluster medium
Galaxies: distances and redshifts
Galaxies: evolution
galaxies: individual (Milky Way)
galaxies: interactions
galaxies: jets
Galaxies: kinematics
galaxy cluster
Galaxy Clustering
galaxy clusters
Galaxy Coevolution
Galaxy dynamics
Galaxy environment
Galaxy environments
galaxy evolution
Galaxy formation
Galaxy formation and evolution
Galaxy group
galaxy merger
Galaxy mergers
galaxy morphology
Galaxy Overdensities
Galaxy properties
Galaxy Redshift Distributions
Galaxy structure
galaxy structures
Galaxy survey
Galaxy: centre
Galaxy: halo
Galaxy: kinematics and dynamics
Galaxy: stellar content
Gamification
gamma ray bursts
Gamma-ray
Gamma-ray burst
Gamma-ray bursts
Gamma-ray sources
gamma-rays
gas phase metallicity gradients
General relativity
general – pulsars
Generative AI
Geodesy
geostationary orbit
Giant Magellan Telescope (GMT)
girls
GLAO
global citizenship education
Global Hub
Global-Local (Glocal) STEM Strategies
globular clusters
globular clusters: individual: M49
GNSS
governance
GPU-based Digital Spectrometer
Gravitation
gravitational lensing
Gravitational recoil
Gravitational Wave Astronomy
gravitational waves
Gravitational-wave Astronomy
Gravitational-wave observation
gravitational-waveform
gravity-assist maneuvers
GRB 220426A
GRB 230812B
Ground-based astronomy
Ground-based Observatory
ground-based optical astronomy
GW190521
H
Halo Spin
Hamiltonian approach
Hands-on Learning
Hanle Dark Sky Reserve HDSR
Hapke model
Herbig Ae/Be stars
Herbig-Haro Objects
heritage protection
HI galaxy
HI line absorption
High cadence
High energy astrophysics
high redshift
High redshift galaxies
High resolution spectroscopy
High schools
High-energy
High-energy astrophysics
High-frequency radio observations
High-redshift
high-redshift galaxies
High-redshift galaxy clusters
High-redshift Universe
High-Resolution Real-time Processing
high-speed solar wind
High-z Galaxy
Higher dimension
HII regions
Hong Kong SAR
Hongmeng Project
horizon mass
Host-galaxy environments
host-galaxy of Type Ia supernovae
Hot ISM
hot subdwarf
HPC
Hubble constant
Hubble constant (758)
Hydrocarbons
Hydrodynamic-magnetodynamic-kinetic evolution
Hydrodynamical Simulation
Hydrodynamical simulations
Hydrodynamical simulations25
I
IAU CPS
IAU Regional Offices
IAU-OAD
IGSO
ILRS
Image Processing
immersive Learning
In-Orbit Sensing
inclusion and diversity
Inclusive Astronomy
Inclusive Teaching
Indian Astronomical Observatory IAO
Indian Institute of Astrophysics IIA
indigenous astronomical knowledge preservation
Indigenous lands and communities
indigenous peoples’ rights
industrial robots
Infalling Envelope
Inflation
infrared
Infrared Spectroscopic Survey
infrastructure
initial mass function
innovation
Insight-HXMT
Instrumentation
Instruments
Insurance
Integral Field Spectroscopy
integral field units
Integrated Testing
Inter-regional collaboration
Interacting binary system
Interdisciplinary learning
interferometric data analysis
Interferometric observations
intergalactic medium
Intermediate-mass Black Holes
International Astronomy Policy
international cooperation
International partnerships
interplanetary medium
interplanetary parameters
Interstellar atomic gas
Interstellar Clouds
Interstellar dust
Interstellar filaments
Interstellar magnetic fields
Interstellar Media
interstellar medium
Interstellar Medium (ISM)
intracluster medium
irreducible mass
ISM
ISRU
IVS
J
Jet
jets
jets and outflows
JWST
JWST observations
K
k1
k2
k3
Keplerian rotation
Kerr black hole
KH Coder
Kinematics
Kinematics and star formation
Kinetic energy
Knowledge Graph
Korea
Korea Astronomical Society
Korea Microlensing Telescope Network (KMTNet)
kuiper belt
kw1
kw2
kw3
L
Laboratory astrophysics
Lagrangian Points
large aperture mirror
Large Area telescopes
large scale structures
large science model
large-scale structure
large-scale structure of Universe
Large-scale structures
Late Stage Stellar Evolution
lensed transients
LEO
LEO statatites
LHAASO
Lie group theoretic method
light curve
light curves
light pollution
Light Pollution Awareness
Light scattering
Light-curve Modeling
lightcurve photometry
lightcurves
LIGO
LIGO-India
Little Red Dots (LRDs)
Local Universe galaxies
long-term sustainability
Low Frequency
low frequency radio astronomy
Low Mass X-ray binary (LMXB)
low surface brightness galaxies
Low-Earth Orbit LEO
LRDs
luminosity function
luminosity functions
Lumme Bowell model
lunar-based astronomy
Lyman alpha emitters
Lyman Continuum Leakers
Lyman-alpha Emitter
Lyman-alpha galaxies
M
Machine Learning
machine learning – conditional diffusion
machine-learning
Mageprojects
magnetar
Magnetic Field
magnetic fields
magneticfield
Magnetohydrodynamical simulations
Magnetospheric radio emissions
Manufacturing
Mars
Mass
Mass accretion
mass loss
mass transfer
mass-loss
Mass-loss rate
massive star
Massive star evolution
massive stars
Maunakea
Maximum mass
MeerKAT
MegaCam
megaconstellations
MEO
Merger
Merger of compact binary
Metal Dilution
methods: statistical
MHD
MHD simulations
Microlensing
microstructures
Mid-Infrared
Milky Way dynamics
Millimeter astronomy
Millimeter interferometry
Millimeter/Submillimeter Wave Astronomy
Millisecond pulsars
missing satellite problem
mission
Mission design
mm and submm interferometer
Model Comparison
Modelling
Modified gravity
Molecular clouds
molecular gas and dust grains
molecular hydrogen
Molecular outflows
Molecular spectroscopy
Molecular Vibrations
Molecules
moment of inertia
multi wavelength
Multi-Agent System
multi-band receiver
Multi-class classification
Multi-component-isotope-abundance SEPs
multi-epoch spectroscopy
Multi-messenger Astronomy
Multi-probe cosmology
Multi-wavelength
Multi-wavelength and multi-messenger constraints
Multi-wavelength and multi-mode observation
MultiDark(Planck)
multimessenger
Multimodal data
multimodal pedagogy
Multiple Object Tracking
MUSE/VLT
N
n-body simulation
NARIT
Narrative
National Standard
NEA
near-Earth asteroids
Near-infrared
Near-infrared spectroscopy
nearby galaxies
nebular spectroscopy
Nested Sampling
Neural Networks
Neutrino astronomy
neutrinos
neutron star
neutron star X-rays binaries
neutron stars
New multi-purpose Facility
Night aky
Nitric oxide
No-hair Theorem
Non-metricity gravity
non-thermal radiation
Nonthermal Emissions
Norms
novae
nucleosynthesis
numerical
Numerical Simulation
Numerical simulations
NuSTAR
O
obscured galaxy populations
observation
Observational astronomy
observational cosmology
Observational Performance
observatory
occultation events
Occultation observations
off-nuclear AGN
OIR Instrumentation
OIR Telescope
Open clusters
Operator
Operator Impact Model
Optical
Optical and infrared astronomy
Optical and Radio Astronomy
optical astronomy
optical manufacturing
Optical Observation
optical telescope
Optical Tracking
Orbit Determination
Orbit Maneuver Criteria
Orbit modelling
orbital dynamics
Orbital Traffic Management
Out-of-plane
Outer space
outflows
outreach
P
parameter-estimation
Particle Acceleration
particle transport
PCA
Perseus Star-Forming Region
photometry
PID Control
Pitch angle distribution
planet
Planet nine
planetarium
Planetary alignment
planetary defense
planetary exploration
Planetary Nebulae
planetary radio emission
Planetary system formation
Plasma astrophysics
plasma nonlinear phenomena
Plasma physics
polarisation
Polarization (Dust and Synchrotron)
polycyclic aromatic hydrocarbons
population synthesis
Population synthesis and survey biases
Porosity
Post-AGB stars
pre-main sequence stars
Primordial gravitational-wave background
Protocluster
protoplanetary disks
Protostars
protostellar disks
Protostellar Jet
public engagement
Public Event
Public Outreach
Pulsar
pulsar surveys
pulsar timing
pulsar wind nebula
Pulsar wind nebulae
pulsars
pulsars: individual (AR Sco)
pulsating star
Pusat Astronomi Borneo
PWV
Q
QCD correction factor $(c_{cor})$
Quantum gravity phenomenology
quasar
quasars
Quasi-periodic Oscillations
quenching
Quick-Look Database
R
Radial velocity
radiation mechanisms: thermal
radiation: dynamics – radiative transfer
radiative process
radiative transfer
Radio
Radio Astronomy
Radio Astronomy facilities
Radio bursts (1339)
radio continuum
Radio continuum emission (1340)
Radio Frequency Interference
Radio galaxies
radio interferometry
Radio lines
Radio pulsars
Radio Quiet Zone
radio rebrightening
Radio Relics
Radio sources (1358)
Radio survey
Radio Telescope
radio telescopes
radio transients
radio-selected AGNs
Random Forest
real-time source search
receivers
Red giants
Red supergiants
Redshift Evolution of AGN
Reflectance
Regional collaboration
Regulation
Reionization
Reissner-Nordström metric
Relativistic hybrid Particle-in-Cell Lattice Boltzmann Method
Relativistic jets
relativistic processes
Research
Research-to-Classroom (R2C) Framework
resident space objects
resonant orbits
Retarded Gravity
retrieval technique
reverberation mapping
Ringdown
Risk Mitigation Cost
Robotic Operations
Robotic Telescopes
rotation
Rubin-LSST
S
s-process
SAGE
San Pedro Martir Observatory
satellite
Satellite Collision Avoidance
Satellite Constellations
satellite interference
Satellite Maneuver
Satellite tracking
Satellite-to-Satellite Observation
Satellites
Scattering effect
Schools
Science Commissioning
Science Communication & Public Outreach
Science Delivery
science education
science engagement
science literacy
science public engagement
Science Verification
Scientific Impact
scientific reasoning
sdb
SDSS
search pipeline
Second-generation planet formation
secular evolution
Secular perturbations
segmented telescope
SEL1 Lagrange point
Self-gravitating ideal gas
Self-interacting dark matter (SIDM)
Semi-analytical model
Seyfert galaxies
shadow time predictions
Shock wave in rotating medium
shock waves
Shocks
Signal Extraction
Simulation
simulation-based inference
simulations
Single-dish observations
Site Suitability Analysis
Site testing
size-mass relation
SKA
SKA Observatory
SKAO
sky brightness
Sky Survey
Sky surveys
slitless spectroscopy
Small satellite
SMBH
SN 2023aew
Snapshot spectroscopy
Social and societal reponsibility of astronomy
software development
solar activity
Solar Eclipse
solar energetic particles
solar magnetic field
solar polar orbit spacecraft
Solar radiation pressure
solar radio burst
solar system
source localization
South West and Central Asian Regional Office of Astronomy for Development (SWCA ROAD)
southeast asia
space astronomy
Space Astrophysics Mission
space debris
Space Debris Detection
Space Debris Laser Ranging
Space Debris Mitigation
Space economy
Space mission
Space missions
Space object Detection
space observatory
space robotics
space science
Space Science Mission
Space Situation Awareness
Space Situational
space situational awareness
Space Sustainability
space technology
space telescope
Space Traffick Management
space weather
Sparse Measurements
Speckle interferometry
Spectral surveys
spectral width
Spectroscopic Survey
spectroscopy
Spectrum Management
Spektr-UF
Spektr-UF (WSO UV) space telescope
SPHEREx
Spherical accretion
spider pulsars
spiral galaxies
SRCNet
SSA
ssc1
SSC2
ssc3
Stability
Stable Hot Gas Halo
Standard Model
star and planet formation
Star formation
Star Formation History
star formation in galaxies
star formation rate
Star Forming History
star-formation
Star-forming regions
Starburst
Starburst Galaxies
Starfishing
Starlight polarization
Stars
stars: abundances
stars: activity
stars: emission mechanisms: non-thermal
stars: evolution
stars: flare
stars: kinematics and dynamics
stars: late-type
stars: magnetic field
stars: neutron
stars: population III
stars: rotation
stars: statistics
stars: winds outflows
Stellar abundances
stellar astrophysics
Stellar atmosphere
Stellar cores
stellar evolution
Stellar initial mass function
stellar jet
stellar nucleosynthesis
Stellar parameters
Stellar physics
Stellar populations
Stellar Rotation
Stellar spots
Stellar streams
Stellar Wind
Stellar winds
Stellar-to-total Mass Ratio
STEM
STEM Education Facilities
STEM Engagement
Stephen Hawking
Sterile neutrino
stripped-envelope supernovae
Strong Gravitational Lensing
Structural Growth of Galaxies
structure and evolution of galaxies
Structure formation
Student Engagement
Student Research
sub-/mm-observations
subdwarfs
submillimeter spectroscopy and ISS technology
Super Massive Black Holes
supercomputer
supermassive binary black holes
Supermassive black holes
supernova
Supernova host galaxies
Supernova Remnants
supernovae
superstations
Survey
Survey Camera
Surveys
Sustainable Development Goals
sustainable space
Synthetic data generation
System Dynamics
Sérsic Index
T
targeted transient survey
Teacher development
Teacher Education
Teacher Training
Teacher Training Workshop for International Audiences
techniques: polarimetric
Telescope
Telescope capabilities
Telescope Facility
Telescope images
Telescopes
Tension Quantification
TeV photons
Text Analysis
The "Dark Matter" Problem
theoretical models
theory of gravitational radiation
thermal diffusion
Tianguan Einstein Probe
Tidal disruption
Time domain astronomy
Time Domain Astrophysics
Time-domain Astronomy
time-domain surveys
ToO observation
Tracklet identification
training
Transient
Transient astronomy
Transient Phenomena
transients
Transit
transit observation
translational-rotational motion
transmission spectroscopy
Transneptunian objects
Trasient searches
Trumpler 14
Tully-Fisher relation
Turbulence
Type Ia Supernovae
Type Ic supernovae
type Ic-BL supernova
Type IIb supernovae
U
UIEs
ultra-diffuse galaxies
ultralong wavelength astronomy
Ultraviolet
ultraviolet observatory
Ultraviolet range
ultraviolet spectra
Ultraviolet spectroscopy
unipolar induction
universe
Urban Astronomy & Outreach
Urban Astronomy Education
User Support
User tools
V
Variable star classification
Venus
Very Ling Baseline Interferometry
Very Long Baseline Interferometry
Very Long Baseline Interferometry (VLBI)
very-long baseline radio interferometry
VGOS
Virtual Observatory (VO) network
VLBI
Void Galaxies
W
weak gravitational lensing
weak lensing
White Dwarf
white dwarfs
Wide field
Wide field imagery
winds
WIRCam
Wolf-Rayet star
Wolf-Rayet Stars
Workshop
Workshops
X
X-ray
X-ray binaries
X-ray binary stars
X-ray ISM
X-ray spectroscopy
X-ray transient sources
X-rays
X-rays: galaxies
Xray
XRB
Y
Young Stellar Objects