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The total infrared luminosity may significantly overestimate the star formation rate of quenching and recently quenched galaxies
The total infrared (IR) luminosity is very useful for estimating the star formation rate (SFR) of galaxies, but converting the IR luminosity into an SFR relies on assumptions that do not hold for all galaxies. We test the...
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Interpreting the star formation - extinction relation with MaNGA

We investigate the resolved relation between local extinction and star formation surface density within nearby star-forming galaxies selected from the MaNGA survey. Balmer decrement measurements imply an extinction of the Hα...

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Interpreting the star formation - extinction relation with MaNGA

We investigate the resolved relation between local extinction and star formation surface density within nearby star-forming galaxies selected from the MaNGA survey. Balmer decrement measurements imply an extinction of the Hα...

Published by:
The total infrared luminosity may significantly overestimate the star formation rate of quenching and recently quenched galaxies
The total infrared (IR) luminosity is very useful for estimating the star formation rate (SFR) of galaxies, but converting the IR luminosity into an SFR relies on assumptions that do not hold for all galaxies. We test the...
Published by:
Testing the consistency of dust laws in SN Ia host galaxies
Abstract We apply BayeSN, our new hierarchical Bayesian model for the SEDs of Type Ia supernovae (SNe Ia), to analyse the griz light curves of 157 nearby SNe Ia (0.015 < z...
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