CORDIS Project
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The PHOLOS project aims to improve methods for identifying and analyzing lensed supernovae to measure the Hubble constant accurately. It involves developing techniques to find candidates and modeling the mass distribution of lensing galaxies, ultimately enhancing cosmological inference.
Lensed supernovae offer promising tools for cosmology with the upcoming revolutionary LSST survey, however the current techniques to both find these systems and to properly use them to infer the Hubble constant (H0) are severely underdeveloped.
In this fellowship, I propose PHOLOS (Probing H0 with Lensing Of Supernovae), a three-part project to make lasting contributions to all steps of this process. I will first solve the longstanding problem of finding and prioritising lensed supernovae, by s…
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