Conveners
Training simulations to predict the first stars and their effect
- Jonathan Pober
Description
We are interested in regression tasks in analyzing 21 cm cosmology data. Most semi-numerical algorithms use a unique (and not always physical) parameterization of the 21 cm signal, but we can regress on well-defined phenomenological parameters. In this module, we’ll look at estimating the neutral fraction of the intergalactic medium from 21 cm signal maps.
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