Mar 18, 2024 - 11:00 am to 12:00 pm
Location
Campus, Varian 355
Speaker
Noah Sailer (UC Berkeley) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Zoom info: https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
In this talk, I will present ongoing work from which we constrain the amplitude of large-scale structure using the DESI Luminous Red Galaxy sample and its cross-correlation with CMB lensing maps reconstructed from the latest ACT and Planck data. I will pay close attention to potential sources of systematic errors (in the data, modeling, and statistical inference) and our approaches for mitigating them when necessary. Along the way I’ll highlight several subtitles that are peculiar to CMB cross-correlation analyses in a pedagogical fashion. Finally, I will discuss how preliminary results from this analysis weigh in on the S8 “tension.”