Differences and similarities of stellar populations in LAEs and LBGs at $z\sim$ 3.4 - 6.8

The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burst-like models for a sample of 1,558 sources at $3.4

Keywords:

• Galaxy formation and evolution
• Low Mass
• Astrophysics
• Astronomy
• Spectral line
• Stellar mass
• Star formation
• Galaxy
• Cosmic time
• the other
• Physics

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