An investigation of the star-forming main sequence considering the nebular continuum emission at low-<i>z</i>
An investigation of the star-forming main sequence considering the nebular continuum emission at low-<i>z</i>
The code FADO is the first publicly available population spectral synthesis tool that treats the contribution from ionised gas to the observed emission self-consistently. We study the impact of the nebular contribution on the determination of the star formation rate (SFR), stellar mass, and consequent effect on the star-forming main …