About this document

Galaxy Morphology and Emission Lines Analysis by aryan mehata is a document available to read on EtoBox.

The document discusses the features learned by a SFNet model trained to predict optical emission lines and their correlation with morphological characteristics in galaxies. It highlights specific features that indicate different physical interpretations related to star formation and metallicity. The findings suggest that CNNs can effectively predict spectroscopic tracers of galaxy evolution based on morphological data.

Author

aryan mehata

Language

EN