text:   20201124A",3,"['New paper on @arxiv_org today, lead by W. Fong @FongGroup at: <LINK>\n\nHere we identify and characterize the host galaxy of the repeating, super-bursting FRB 20201124A <LINK>', 'We found that the galaxy is a dusty, relatively modest star-formning galaxy (in good agreement with last weeks result by Vikram Ravi and collaborators: https://t.co/KZLlitr5fm) with a potential hot MIR dust component contributing ~10-30% to the SED. https://t.co/eEClt2bb3T', 'Perhaps most intriguing, is that we could constrain the star-formation history of the galaxy finding that &gt;90% of its mass (and thus likely the progenitor star/object) was formed 1 Gyr ago, putting strong constraints on the likely progenitor channels of this FRB. https://t.co/QJAutE2fBF']",21,06,686