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(1 - 3 of 3)
GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow
Spatially-resolved dust properties of the GRB 980425 host galaxy
The optically unbiased GRB host (TOUGH) survey. VI. radio observations at z ~ 1 and consistency with typical star-forming galaxies