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The fraction of clumpy star-forming galaxies in nearby galaxies from CLAUDS and HSC-SSP
Massive, star-forming clumps are regions of intensive star-formation that are commonly observed in high-redshift ($z > 1$) galaxies. Observations of low-redshift clumpy galaxy analogues are rare but the availability of wide-field galaxy survey data makes the detection of large clumpy galaxy samples
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