CMB-S4 Virtual 2020
instructors:
ACTPol DR4: Virtual 2020
instructors:
ACTPol: Princeton 2019
instructors: Jo Dunkley, Renee Hlozek, Jeff McMahon, Mat Madhavacheril, Alex van Engelen
ACTPol: Michigan 2016
instructors: Renee Hlozek, Jeff McMahon
La Serena 2015
instructors: Jeff McMahon (as part of the La Serena data science summer school)
In this module you will learn to simulate realizations of the CMB starting from a theoretical power spectrum.
In this module you learn to simulate maps of point sources and SZ clusters starting from statistical distributions and a cluster profile.
In this module you learn to simulate a ground based instrument by including the impact of diffraction (the beam), white noise, 1/f noise, and atmospheric noise
In this module you learn to estimate the power spectrum and its error bars starting from a map and knowledge about the instrument.
In this module you learn to find cluster and point source candidates using the matched filter technique.
In this module you work with public ACT data. A version using ACTPol data will soon be available.
In this module you simulate maps of the CMB's polarization including TE correlation, and work with B-mode estimators that minimize E-B leakage.
In this module you model time ordered data (TODs) and work with maximum likelihood mapping code.
In this module you simulate the lensing of the CMB and work with a quadratic estimator to recover the lensing convergence.