Speakers
Adam Anderson
(Fermi National Accelerator Laboratory)
Kirit Karkare
(SLAC)
Zhaodi Pan
(Argonne National Laboratory)
Description
Line intensity mapping at millimeter wavelengths is a promising method of measuring large-scale structure and constraining cosmology, potentially beyond the reach of future optical surveys. I will outline the path forward to deploying future instruments with the required sensitivity for next-generation cosmological constraints, including developing large-format on-chip spectrometers and analysis of current pathfinders.
Primary author
Kirit Karkare
(SLAC)
