Finite Resolution Deconvolution of Multi-Wavelength Imaging of 20,000 Galaxies in the COSMOS Field: The Evolution of Clumpy Galaxies Over Cosmic Time

Compact star-forming clumps observed in distant galaxies are often suggested to play a crucial role in galaxy assembly. In this paper, we use a novel approach of applying finite resolution deconvolution on ground-based images of the COSMOS field to resolve 20,185 star-forming galaxies (SFG) at 0.5

Keywords:

• Galaxy
• Stellar mass
• Instability
• Astrophysics
• Deconvolution
• Redshift
• Surface brightness
• Physics
• Angular resolution
• Star formation

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