Three Dusty Star Forming Galaxies at $z\sim1.5$: Mergers and Disks on the Main Sequence

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Abstract:

The main sequence of galaxies, a correlation between the star formation rates and stellar masses of galaxies, has been observed out to $z\sim4$. Galaxies within the scatter of the correlation are typically interpreted to be secularly evolving while galaxies with star formation rates elevated above the main sequence are interpreted to be...More

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