Radio-based SFR estimates assign 84% of SN Ia hosts to the same SFR-M* regions as FIR-constrained SED fitting, produce consistent standardization parameters, and confirm region-dependent variations in nuisance parameters.
C., Ciesla L., Ilbert O., Magnelli B., Jiménez-Andrade E
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Modeling indicates AME is negligible for distant galaxies at ~10 GHz but may bias single-frequency SFR estimates in resolved nearby galaxies depending on beam size and column density.
citing papers explorer
-
Applications of 1.4 GHz diagnostics to Type Ia Supernova host galaxies
Radio-based SFR estimates assign 84% of SN Ia hosts to the same SFR-M* regions as FIR-constrained SED fitting, produce consistent standardization parameters, and confirm region-dependent variations in nuisance parameters.
-
Impact of Anomalous Microwave Emission (AME) on Radio Spectral Energy Distributions: SKA Observations of Galaxies Near and Far
Modeling indicates AME is negligible for distant galaxies at ~10 GHz but may bias single-frequency SFR estimates in resolved nearby galaxies depending on beam size and column density.