סמינר באסטרונומיה ובאסטרופיזיקה: ML&ML reconstructions of the large scale structure of the nearby universe

Zoom: https://tau-ac-il.zoom.us/j/87185167411?pwd=FpTUyIgXaOturzOFSetA6pPVYQilen.1

Abstract:

I will show how we can use both machine-learning and maximum-likelihood techniques to map the cosmic web at low redshift. Using redshift surveys with distance-indicator catalogs, we’ll see how each method probes the density and velocity fields. Will discuss specific cases that illustrate how the two approaches are closely connected. 

מארגן הסמינר: ד"ר יהונתן שטרן