As the largest virialized structures in the universe, galaxy clusters continue to grow and
accrete matter from the cosmic web. Due to the low gas density in the outskirts of clusters …

Transition Edge Sensors (TESs) are amongst the most sensitive cryogenic detectors and
can be easily optimized for the detection of massive particles or photons ranging from X-rays …

Optimal analyses of many signals in the cosmic microwave background (CMB) require map-
level extraction of individual components in the microwave sky, rather than measurements at …

Inflation is the leading theory of the first instant of the universe. Inflation, which postulates
that the universe underwent a period of rapid expansion an instant after its birth, provides …

We forecast constraints on cosmological parameters enabled by three surveys conducted
with SPT-3G, the third-generation camera on the South Pole Telescope. The surveys cover …

A promising idea to resolve the long standing Hubble tension is to postulate a new
subdominant dark-energy-like component in the prerecombination Universe which is …

The increasing statistical power of cosmic microwave background (CMB) datasets requires a
commensurate effort in understanding their noise properties. The noise in maps from ground …

The search for primordial gravitational waves in the cosmic microwave background (CMB)
will soon be limited by our ability to remove the lensing contamination to B-mode …

The next generation of cryogenic CMB and submillimeter cameras under development
require densely instrumented sensor arrays to meet their science goals. The readout of large …

Upcoming measurements of the small-scale primary cosmic microwave background (CMB)
temperature and polarization power spectra (TT/TE/EE) are anticipated to yield …