Physics
Active Galactic Nuclei
10%
Atmospherics
11%
Bl Lacertae Object
9%
Black Holes
9%
Canary Island
15%
Carbon Star
21%
Chemical Abundances
10%
Chemical Evolution
8%
Cold Gas
18%
Color-Magnitude Diagram
10%
Coma Cluster
8%
Data Transmission
7%
Early-Type Galaxies
58%
Extremely large telescope
7%
Field of View
38%
Galactic Evolution
19%
Galaxy Clusters
21%
Galaxy Evolution
17%
Hertzsprung-Russell Diagram
9%
High Resolution
28%
Hubble Space Telescope
9%
Initial Mass Function
34%
Interstellar Matter
13%
Ionized Gas
16%
Lenticular Galaxies
7%
LOFAR
23%
Magellanic Clouds
9%
Metallicity
57%
Milky Way
11%
Molecular Gas
13%
Near Infrared
34%
Photometry
11%
Physics
10%
Planetary Atmosphere
6%
Red Giant Branch
9%
Redshift Surveys
10%
RR Lyrae Variable Stars
19%
Sky Surveys
16%
Spectra
9%
Spectral Energy Distribution
7%
Spectrographs
91%
Spectroscopic Telescopes
9%
Spiral Galaxy
9%
Star Formation
40%
Star Formation Rate
19%
Stellar Mass
28%
Stellar Populations
100%
Stellar Spectra
7%
Ultraviolet Spectra
9%
Very Large Telescope
18%
Keyphrases
Absorption System
6%
Ancient Metals
6%
Atmospheric Parameters
5%
Carbon Stars
9%
Cluster Survey
6%
Cold Gas
10%
Colour-magnitude Diagrams
6%
Dimensionality Reduction
6%
Early-type Galaxies
13%
Formation Model
10%
Gaia
9%
Galactic Chemical Evolution
6%
Galaxies
46%
Galaxy Clusters
9%
Galaxy Formation
9%
Halo
5%
Hierarchical Formation
6%
High-resolution
6%
Initial Mass Function
10%
Integral Field Unit
7%
Interstellar Medium
5%
John Herschel
15%
Local Universe
9%
Low-mass
10%
Massive Stars
6%
Metallicity
20%
Molecular Gas
6%
Multi-object
5%
Near-infrared
11%
Near-infrared Spectrum
5%
Prime Focus Corrector
6%
Red Supergiants
6%
RR Lyrae Stars
5%
Semi-analytic Model
9%
Spectral Energy Distribution
6%
Spectral Library
38%
Spectrograph
15%
Star Formation
6%
Star Formation Rate
9%
Star-forming Galaxies
7%
Stellar Masses
12%
Stellar Populations
26%
Synthesis Model
8%
Ultra-diffuse Galaxies
6%
Ultraviolet Spectrum
6%
Wavelength Range
10%
Wide-field
13%
X-Shooter
36%
