CORDIS Project
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This project focuses on improving the precision of distance measurements to Type Ia supernovae by utilizing near-infrared observations. By developing advanced models that integrate optical and near-infrared data, the project aims to enhance our understanding of cosmic expansion and dark energy properties.
Type Ia supernovae (SNe Ia) are used as “standardiseable candles”: their peak luminosities can be inferred from their optical light curve shapes and colours, so their distances can be estimated from their apparent brightnesses.
SN Ia distances with high precision and small systematic error are essential to accurate constraints on the cosmic expansion history, local measurements of the Hubble constant, and the properties of the dark energy driving the acceleration, in particular, its equation-of-…
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