FRB interests are focused on dissecting the cosmic web.

FRB interests are focused on using them to understand the formation and evolution of galaxies.

FRB interests are focused on using them as probes of the intergalactic and circumgalactic media.

FRB interests are focused on uncovering the progenitors through their host galaxy environments.

FRB interests are focused on understanding the distribution of matter in the IGM. 

FRB interests are focused on characterizing FRB hosts and constraining progenitor models.

FRB interests are constraining progenitor channels and emission mechanisms through searches for multi-wavelength counterparts.

FRB interests are focused on constraining progenitor models using multi-wavelength observations. 

FRB interests are using SED modeling of host galaxies to constrain progenitor models.

FRB interests are focused on optical follow-up and crossmatching catalogued transients and FRBs.

FRB interests are focused on understanding the DM contribution of FRB host galaxies.

FRB interests include using FRBs as a tool for probing the galaxies that lie in their sightline, allowing for the study of the distribution of matter and magnetic fields in these distant regions.

FRB interests include understanding whether and if there is a connection between neutron star merger remnants, magnetars, and FRBs to understand r-process enrichment and the maximum density of nuclear material. FRB interests also include developing next generation software and infrastructure to enable real-time, multi-messenger astronomy.

FRB interests include host galaxy characterization and data processing.

FRB interests are focused on constraining the partition of cosmic baryon between IGM and CGM, and models of galactic feedback.

FRB interests are focused on using them to probe the baryons encountered along their line of sight. 

FRB interests are polarimetry, propagation effects, probing foreground magneto-ionic material, and studying the epoch of helium reionization.

FRB interests are focused on optical follow-up and stellar population modelling.

FRB interests are focused on optical follow-up.

FRB interests are focused on morpho-cinematic analysis of FRB galaxy hosts.

FRB interests are focused on commissioning CHIME/FRB outriggers and constraining FRB progenitors through their host galaxy environments.

FRB interests are focused on determining the potential effectiveness of ground-based, adaptive optics follow-up in studying FRB hosts.

FRB interests are focused on the connection between FRB properties and host galaxy environments.

FRB interests are focused on putting limits on associated optical transients.

FRB interests are focused on optical follow up and analysis of FRB host galaxies.

FRB interests are focused on optical followup for spectral analysis of FRB host galaxies.

FRB interests are examining spectral and morphological properties of FRBs and their host galaxy.

FRB interests are focused on optical follow up using integral field spectroscopy of FRB host galaxies.

FRB interests include developing analysis software, specifically within the backend of the zdm python codebase.

FRB interests are focused on analyzing the properties of FRB host galaxies with optical integral field spectroscopy.

FRB interests include probing the IGM baryon distribution using z-DM modeling.

FRB interests include developing software and scalable inference methods to enable real-time follow-up decision making.

FRB interests are focused on exploring different methods for estimating the redshift of FRBs from their DM contributions.