INIS
filaments
100%
stars
65%
clouds
63%
magnetic fields
55%
data
46%
telescopes
40%
orientation
38%
emission
27%
density
26%
polarization
22%
space
20%
resolution
19%
algorithms
19%
dusts
19%
maps
18%
images
17%
machine learning
15%
magellanic clouds
15%
detection
15%
interstellar magnetic fields
15%
region ii
15%
region i
15%
populations
15%
balloons
12%
environment
12%
gases
11%
velocity
10%
satellites
10%
range
10%
image processing
10%
turbulence
10%
data analysis
10%
gravitation
9%
collisions
9%
dynamics
9%
astronomy
8%
sky
7%
european space agency
7%
junctions
7%
surveys
7%
rolling
7%
milky way
6%
neural networks
6%
galaxies
5%
protostars
5%
distribution
5%
wavelengths
5%
labelling
5%
center-of-mass system
5%
Keyphrases
Planck
42%
Relative Orientation
38%
Star Formation
30%
Filamentary Structure
30%
Column Density
30%
Big Data
30%
ISM
26%
Molecular Clouds
22%
Magnetic Field
22%
Space Telescope
22%
Interstellar Medium
22%
Statistical Analysis
19%
Herschel
15%
Balloon-borne
15%
Background Magnetic Field
15%
Interstellar Magnetic Fields
15%
Parametrization
15%
Galactic
15%
Machine Learning
15%
Lineament Detection
15%
Dense Core
15%
Magnetic Filaments
15%
Evolutionary Stages
11%
Magnetic Field Direction
11%
European Space Agency
11%
Astronomy
11%
Hough Transform
7%
Observatory
7%
High Angular Resolution
7%
Identification Algorithm
7%
Mask R-CNN
7%
Data Combination
7%
Formation Process
7%
Turbulence
7%
Density Contrast
7%
Condensation
7%
Neural Network Model
7%
Training Samples
7%
Neural Network Training
7%
All-sky Survey
7%
U-Net
7%
Limited Training Data
7%
Low Contrast
7%
Best Model
7%
User-dependent
7%
Sampling Methods
7%
Orientation Angle
7%
Atomic Hydrogen
7%
Neural Network Method
7%
Molecular Lines
6%
Physics
Magnetic Field
75%
Star Formation
62%
Molecular Clouds
62%
Star Forming Regions
34%
Interstellar Matter
32%
Big Data
30%
Space Telescope
23%
Image Processing
18%
Large Magellanic Cloud
15%
Interstellar Magnetic Field
15%
Milky Way
15%
Neural Network
15%
Interstellar Dust
15%
Machine Learning
15%
Center of Mass
15%
Ground Telescopes
8%
Protostars
7%
Line Spectra
6%
High Resolution
5%
Condensation
5%
Astronomical Map
5%
Convolutional Neural Network
5%
Sky Surveys
5%