Radio Cosmology: Imaging the Cosmic Dawn
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Location
Campus, Varian 355
Speaker
Emma Tolley (EPFL) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Cosmology Seminar
Cosmology Seminars are held on Mondays at 11 am, on the 3rd floor Varian conference room. These are more focused and less didactic than the colloquium, and provide a stage for younger researchers to present their work in more detail.
Please contact Sandy Yuan, Delon Shen, or Risa Wechsler for more information.
How much information can be extracted from galaxy clustering at the field level?
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Location
Campus, Varian 355
Speaker
Minh Nguyen (University of Michigan) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Big Data cosmology meets AI
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Location
Varian 355
Speaker
Carolina Cuesta-Lazaro (MIT) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Cosmology at redshifts 50 and 1100
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Location
Campus, Varian 355
Speaker
Zack Li (UC Berkeley) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Zoom info: https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
At high redshift, we can cleanly separate physics from astrophysics. Things were simpler back then! I'll discuss two upcoming experiments that chase those good old days before star formation changed everything.
Multi-tracer cosmology at high redshift using galaxies and lensing
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Location
Campus, Varian 355
Speaker
Haruki Ebina (UC Berkeley) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Towards an Optimal Cosmological Detection of Neutrino Mass with Field-Level Inference
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Location
Campus, Varian 355
Speaker
Adrian Bayer (Princeton) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Simulation-Based Inference of Large Scale Structure with Neural Quantile Estimation
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Location
Campus, Varian 355
Speaker
He Jia (Princeton) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
CMB lensing power spectrum without noise bias
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Location
Campus, Varian 355
Speaker
Delon Shen (KIPAC) zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Structure growth from cross-correlation of DESI Luminous Red Galaxies and CMB lensing
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Location
Campus, Varian 355
Speaker
Noah Sailer (UC Berkeley) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09
Squeezing fNL out of the matter bispectrum with cosmological consistency relations
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Location
Campus, Varian 355
Speaker
Sam Goldstein (Columbia) In Person and zoom https://stanford.zoom.us/my/sihanyuan?pwd=QnpsUHZWWGJ2ekVYWmZVL3BmM0gzZz09