The MOSDEF survey: the dependence of H α-to-UV SFR ratios on SFR and size at z ∼ 2

We perform an aperture-matched analysis of dust-corrected H$\alpha$ and UV SFRs using 303 star-forming galaxies with spectroscopic redshifts $1.36

Keywords:

• Emission spectrum
• Physics
• Astrophysics
• Galaxy
• attenuation curve
• continuum
• Redshift

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