Kavli Affiliate: Luis Ho | Summary:We present a spatially resolved chemical abundance analysis of 2291 star-forming galaxies at $z leq 0.1$, spanning nearly four orders of magnitude in stellar mass ($8 le rm log (M_star/M_odot) le 11.5$), by exploiting the multi-fibre spectra from the Dark Energy Spectroscopic Instrument (DESI) as a sparse integral field spectrograph. […]
Continue.. DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at $zleq0.1$