Mapping the low-surface brightness Universe in the UV band with Lyα emission from IGM filaments

Keyphrases

• Intergalactic Medium 100%
• Ultraviolet Band 100%
• Low Surface Brightness 100%
• Galaxies 50%
• Space-based 50%
• Emission Lines 25%
• Cooling Method 25%
• Baryons 25%
• Ultraviolet Wavelength 25%
• Direct Detection 25%
• Spatial Distribution 25%
• Emissivity 25%
• Density Fluctuations 25%
• Recombination 25%
• Density Field 25%
• Halo 25%
• Ionization State 25%
• Thermal State 25%
• Excitation Process 25%
• Helium Gas 25%
• Intensity Fluctuation 25%
• N-body Simulations 25%
• Lyman-alpha 25%
• Dark Matter Density 25%
• Special Regions 25%
• Hydrogen Gas 25%
• Circumgalactic Medium 25%
• Collisional Excitation 25%
• Spatial Fluctuations 25%
• Particle Dark Matter 25%

Physics

• Intergalactic Medium 100%
• Baryon 25%
• Spatial Distribution 25%
• Emissivity 25%
• Dark Matter 25%
• N-Body Simulations 25%
• Dark Matter Density 25%