text: 451,41,1407963590515118083,1140222123006472194,Kasper Elm Heintz,"New paper on @arxiv_org today, lead by W. Fong @FongGroup at: <LINK> Here 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: <LINK>) with a potential hot MIR dust component contributing ~10-30% to the SED. <LINK> 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. <LINK>",https://arxiv.org/abs/2106.11993,"We present the Australian Square Kilometre Array Pathfinder (ASKAP) localization and follow-up observations of the host galaxy of the repeating fast radio burst (FRB) source, FRB20201124A, the fifth such extragalactic repeating FRB with an identified host. From spectroscopic observations using the 6.5-m MMT Observatory, we derive a redshift of $z=0.0979 \pm 0.0001$, a star formation rate inferred from H$\alpha$ emission of SFR(H$\alpha$) $\approx 2.1 M_{\odot}$ yr$^{-1}$, and a gas-phase metallicity of 12+log(O/H)$\approx 9.0$. By jointly modeling the 12-filter optical-mid-infrared (MIR) photometry and spectroscopy of the host, we infer a median stellar mass of $\approx 2 \times 10^{10} M_{\odot}$, internal dust extinction of $A_V\approx 1-1.5$ mag, and a mass-weighted stellar population age of $\approx 5-6$ Gyr. Connecting these data to the radio and X-ray observations, we cannot reconcile the broad-band behavior with strong AGN activity and instead attribute the dominant source of persistent radio emission to star formation, likely originating from the circumnuclear region of the host. The modeling also indicates a hot dust component contributing to the MIR luminosity at a level of $\approx 10-30\%$. We model the host galaxy's star formation and mass assembly histories, finding that the host assembled $>90\%$ of its mass by 1 Gyr ago and exhibited a fairly constant SFR for most of its existence, with no clear evidence of past star-burst activity. ","Chronicling the Host Galaxy Properties of the Remarkable Repeating FRB